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  • Articles  (2,750)
  • American Meteorological Society  (1,360)
  • American Geophysical Union  (1,202)
  • Annual Reviews
  • 1995-1999  (2,750)
  • 1975-1979
  • 1945-1949
  • 1996  (2,750)
  • Physics  (2,750)
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  • Articles  (2,750)
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  • 1995-1999  (2,750)
  • 1975-1979
  • 1945-1949
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  • 1
    Electronic Resource
    Electronic Resource
    Palo Alto, Calif. : Annual Reviews
    Annual Review of Biophysics and Biomolecular Structure 25 (1996), S. 55-78 
    ISSN: 1056-8700
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
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  • 2
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Biophysics and Biomolecular Structure 25 (1996), S. 113-136 
    ISSN: 1056-8700
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
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  • 3
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Biophysics and Biomolecular Structure 25 (1996), S. 163-195 
    ISSN: 1056-8700
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
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  • 4
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Biophysics and Biomolecular Structure 25 (1996), S. 231-258 
    ISSN: 1056-8700
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
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  • 5
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Biophysics and Biomolecular Structure 25 (1996), S. 259-286 
    ISSN: 1056-8700
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Biophysics and Biomolecular Structure 25 (1996), S. 197-229 
    ISSN: 1056-8700
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  • 7
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Biophysics and Biomolecular Structure 25 (1996), S. 287-314 
    ISSN: 1056-8700
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  • 8
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Biophysics and Biomolecular Structure 25 (1996), S. 315-342 
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  • 9
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Biophysics and Biomolecular Structure 25 (1996), S. 367-394 
    ISSN: 1056-8700
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  • 10
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Biophysics and Biomolecular Structure 25 (1996), S. 431-459 
    ISSN: 1056-8700
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  • 11
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Biophysics and Biomolecular Structure 25 (1996), S. 395-429 
    ISSN: 1056-8700
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  • 12
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    Annual Review of Astronomy and Astrophysics 34 (1996), S. 35-73 
    ISSN: 0066-4146
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Physics
    Notes: Abstract Two types of flows dominate the large-scale structure of the solar wind: corotating flows and transient disturbances. Corotating flows are associated with spatial variability in the coronal expansion and solar rotation, whereas transient disturbances are associated with episodic ejections of material into interplanetary space from coronal regions not previously participating in the solar wind expansion. Ulysses' recent epic journey over the poles of the Sun has provided new insights on the three-dimensional nature of both corotating flows and transient disturbances in the solar wind and their evolution with heliocentric distance and latitude. This paper provides a simple physical description of the origins and dynamics of both of these types of solar wind flows, highlighting new understanding gained from the unique Ulysses high-latitude observations.
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  • 13
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    Annual Review of Astronomy and Astrophysics 34 (1996), S. 207-240 
    ISSN: 0066-4146
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Physics
    Notes: Abstract We summarize the properties of FU Orionis variables, and show how accretion disk models simply explain many peculiarities of these objects. FU Ori systems demonstrate that disk accretion in early stellar evolution is highly episodic, varying from ~ 10-7 yr-1 in the low (T Tauri) state to 10-4 yr-1 in the high (FU Ori) state. This variability in mass accretion is matched by a corresponding variability in mass ejection, with mass loss rates reaching ~ 10-1 of the mass accretion rates in outburst. It appears that the FU Ori phenomenon is restricted to early phases of stellar evolution, probably with infall still occuring to the disk, which may help drive repetitive outbursts. Thermal instabilities are a promising way to produce FU Ori disk outbursts, although many uncertainties remain in the theory; triggering by interactions with companion stars on eccentric orbits may also play a role.
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  • 14
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    Annual Review of Astronomy and Astrophysics 34 (1996), S. 383-418 
    ISSN: 0066-4146
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Physics
    Notes: Abstract In most space environments, dust particles are exposed to plasmas and UV radiation and, consequently, carry electrostatic charges. Their motion is influenced by electric and magnetic fields in addition to gravity, drag, and radiation pressure. On the surface of the Moon, in planetary rings, or at comets, for example, electromagnetic forces can shape the spatial and size distribution of micron-sized charged dust particles. The dynamics of small charged dust particles can be surprisingly complex, leading to levitation, rapid transport, energization and ejection, capture, and the formation of new planetary rings. This review briefly discusses the most important processes that determine the charge state of dust particles immersed in plasmas and the resulting dynamics on exposed dusty surfaces and in planetary magnetospheres.
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  • 15
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    Annual Review of Astronomy and Astrophysics 34 (1996), S. 279-329 
    ISSN: 0066-4146
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Physics
    Notes: Abstract The Goddard High-Resolution Spectrograph (GHRS) aboard the Hubble Space Telescope (HST) has yielded precision abundance results for a range of interstellar environments, including gas in the local medium, in the warm neutral medium, in cold diffuse clouds, and in distant halo clouds. Through GHRS studies, investigators have determined the abundances of elements such as C, N, O, Mg, Si, S, and Fe in individual interstellar clouds. These studies have provided new information about the composition of interstellar dust grains, the origin of the Galactic high-velocity cloud system, and the processes that transport gas between the disk and the halo. Precision measurements of the interstellar D to H ratio and of the abundances of r- and s-process elements have also provided fiducial reference values for cosmological and stellar evolutionary observations and theoretical models.
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  • 16
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    Annual Review of Astronomy and Astrophysics 34 (1996), S. 645-701 
    ISSN: 0066-4146
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Physics
    Notes: Abstract The central half kiloparsec region of our Galaxy harbors a variety of phenomena unique to the central environment. This review discusses the observed structure and activity of the interstellar medium in this region in terms of its inevitable inflow toward the center of the Galactic gravitational potential well. A number of dissipative processes lead to a strong concentration of gas into a "Central Molecular Zone" of about 200-pc radius, in which the molecular medium is characterized by large densities, large velocity dispersions, high temperatures, and apparently strong magnetic fields. The physical state of the gas and the resultant star formation processes occurring in this environment are therefore quite unlike those occurring in the large-scale disk. Gas not consumed by star formation either enters a hot X ray-emitting halo and is lost as a thermally driven galactic wind or continues moving inward, probably discontinuously, through the domain of the few parsec-sized circumnuclear disks and eventually into the central parsec. There, the central radio source SgrA* currently accepts only a tiny fraction of the inflowing material, likely as a result of a limit cycle wherein the continual inflow of matter provokes star formation, which in turn can temporarily halt the inflow via mass-outflow winds.
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  • 17
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Astronomy and Astrophysics 34 (1996), S. 749-792 
    ISSN: 0066-4146
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Physics
    Notes: Abstract At luminosities above 1011 , infrared galaxies become the dominant population of extragalactic objects in the local Universe (z〈 0.3), being more numerous than optically selected starburst and Seyfert galaxies and quasi-stellar objects at comparable bolometric luminosity. The trigger for the intense infrared emission appears to be the strong interaction/merger of molecular gas-rich spirals, and the bulk of the infrared luminosity for all but the most luminous objects is due to dust heating from an intense starburst within giant molecular clouds. At the highest luminosities (Lir〉 1012 ), nearly all objects appear to be advanced mergers powered by a mixture of circumnuclear starburst and active galactic nucleus energy sources, both of which are fueled by an enormous concentration of molecular gas that has been funneled into the merger nucleus. These ultraluminous infrared galaxies may represent an important stage in the formation of quasi-stellar objects and powerful radio galaxies. They may also represent a primary stage in the formation of elliptical galaxy cores, the formation of globular clusters, and the metal enrichment of the intergalactic medium.
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  • 18
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Fluid Mechanics 28 (1996), S. 83-128 
    ISSN: 0066-4189
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
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  • 19
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Fluid Mechanics 28 (1996), S. 11-43 
    ISSN: 0066-4189
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
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  • 20
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Fluid Mechanics 28 (1996), S. 187-213 
    ISSN: 0066-4189
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  • 21
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Fluid Mechanics 28 (1996), S. 215-248 
    ISSN: 0066-4189
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  • 22
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Fluid Mechanics 28 (1996), S. 323-360 
    ISSN: 0066-4189
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  • 23
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Fluid Mechanics 28 (1996), S. 477-539 
    ISSN: 0066-4189
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  • 24
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Biophysics and Biomolecular Structure 25 (1996), S. 1-28 
    ISSN: 1056-8700
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    Annual Review of Biophysics and Biomolecular Structure 25 (1996), S. 29-53 
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    Annual Review of Biophysics and Biomolecular Structure 25 (1996), S. 79-112 
    ISSN: 1056-8700
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    Annual Review of Biophysics and Biomolecular Structure 25 (1996), S. 137-162 
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    Annual Review of Biophysics and Biomolecular Structure 25 (1996), S. 343-365 
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    Annual Review of Astronomy and Astrophysics 34 (1996), S. 1-34 
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    Annual Review of Astronomy and Astrophysics 34 (1996), S. 75-109 
    ISSN: 0066-4146
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    Topics: Physics
    Notes: Abstract In the past decade a number of observational and theoretical studies have appeared that address the problem of how both the physical conditions in subsurface layers of the Sun and the nature of the magnetic flux tubes of active regions are reflected in the structure and behavior of these regions at the surface. This review discusses work in this area. Many characteristics of plages and sunspot groups are shown to be related to the conditions encountered by the region flux tube as it rises through the convective zone of the Sun to the surface. Size distributions, rotation and meridional flow rates and their covariances, and characteristics of growth and decay are among the factors that have been shown to depend on the nature of the source magnetic flux tube and the physical effects, such as the Coriolis force and magnetic tension, that act deep in the convection zone.
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Astronomy and Astrophysics 34 (1996), S. 331-381 
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    Annual Review of Astronomy and Astrophysics 34 (1996), S. 419-459 
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    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Physics
    Notes: Abstract The status of searches for gravitational microlensing events of the stars in our galaxy and in other galaxies of the Local Group, the interpretation of the results, some theory, and prospects for the future are reviewed. The searches have already unveiled ~ 100 events, at least two of them caused by binaries, and have already proven to be useful for studies of the Galactic structure. The events detected so far are probably attributable to the effects of ordinary stars, and possibly to substellar brown dwarfs; however, a firm conclusion cannot be reached yet because the analysis published to date is based on a total of only 16 events. The current searches, soon to be upgraded, will probably allow determination of the mass function of stars and brown dwarfs in the next few years; these efforts will also provide good statistical information about binary systems, in particular their mass ratios. They may also reveal the nature of dark matter and allow us to detect planets and planetary mass objects.
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  • 33
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    Annual Review of Astronomy and Astrophysics 34 (1996), S. 461-510 
    ISSN: 0066-4146
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Physics
    Notes: Abstract A careful assessment of current uncertainties in stellar physics (opacities, nuclear reaction rates, equation of state effects, diffusion, rotation, and mass loss), in the chemistry of globular cluster (GC) stars, and in the cluster distance scale, suggests that the most metal-poor (presumably the oldest) of the Galaxy's GCs have ages near 15 Gyr. Ages below 12 Gyr or above 20 Gyr appear to be highly unlikely. If these = 2 sigma limits are increased by ~ 1 Gyr to account for the formation time of the globulars, and if standard Friedmann cosmologies with the cosmological constant set to zero are assumed, then the GC constraint on the present age of the Universe (t0〉= 13 Gyr) implies that the Hubble constant H0〈= 51 km s-1 Mpc-1 if the density parameter Omega = 1 or 〈= 62 km s-1 Mpc-1 if Omega = 0.3.
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  • 34
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    Annual Review of Astronomy and Astrophysics 34 (1996), S. 241-277 
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    Topics: Physics
    Notes: Abstract The cooling flows or winds from evolved stars are ideal for the formation of molecules and dust. The main location of molecular synthesis is the outer circumstellar envelope, where UV radiation from the interstellar medium penetrates the envelope and, by photodissociating parent molecules, produces the high-energy radicals and ions that activate gas-phase neutral and ion-molecule chemistry. After introducing relevant observational results and theoretical ideas, the salient aspects of the photochemical model are described. The primary application is to the nearby C star, IRC + 10216, where 50 or more circumstellar molecules have been detected. Recent interferometer maps, with resolution approaching 1'', provide the means to verify the main ideas of the model and to indicate directions for its improvement.
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    Annual Review of Astronomy and Astrophysics 34 (1996), S. 703-747 
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    Topics: Physics
    Notes: Abstract Accretion disks are important for many astrophysical phenomena, including galactic nuclei, interacting binary stars, and young stellar objects. The central issue in the theory of accretion disks is to identify the dominant mechanisms that regulate angular momentum transfer and mass flow in a variety of contexts. In the first part of this review, we described some recent advances in the study of the physical processes that may be present in accretion disks. Concurrent with these theoretical developments, the arrival of high-resolution astronomical instruments has led to explosive progress on the observational side. In many cases, the study of accretion disks has evolved from their inferred presence based on circumstantial evidence to direct imaging and detailed spectral analyses. Here, we summarize the theoretical interpretation of these data. We review the constraints that may be imposed on the efficiency and nature of angular momentum transfer processes in a variety of astrophysical contexts.
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    Annual Review of Fluid Mechanics 28 (1996), S. 1-9 
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    Annual Review of Fluid Mechanics 28 (1996), S. 389-428 
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  • 38
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    Annual Review of Fluid Mechanics 28 (1996), S. 429-476 
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    Annual Review of Astronomy and Astrophysics 34 (1996), S. 511-550 
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    Topics: Physics
    Notes: Abstract The Magellanic Clouds have galactocentric distances of 50 and 63 kiloparsecs, making it possible to probe the older populations of clusters and stars in some detail. Although it is clear that both galaxies contain an old population, it is not yet certain whether this population is coeval with the date of formation of the oldest globulars in the Milky Way. The kinematics of this old population in the Large Magellanic Cloud (LMC) are surprising; no component of this old population is currently measured to be part of a hot halo supported by velocity dispersion. Spectroscopy of field stars is beginning to show the existence of a small population of stars with abundances [Fe/H] less than -1.4. These stars will help to unravel the star-formation history when the next generation of telescopes are commissioned. Asymptotic giant branch stars, long-period variables, planetary nebulae, and horizontal-branch clump stars can be used to trace the extent and kinematics of the intermediate-age population. Deep color-magnitude diagrams can be used to derive the relative proportions of stars older than 1 Gyr. The age distribution of populous clusters and the age-metallicity relation are used to compare the evolution of the two Magellanic Clouds to each other. The issue of where the LMC's metals originated is explored, as is the question of what triggers star formation in the Clouds.
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    Annual Review of Astronomy and Astrophysics 34 (1996), S. 607-644 
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Fluid Mechanics 28 (1996), S. 249-278 
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    Annual Review of Fluid Mechanics 28 (1996), S. 361-387 
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    Annual Review of Astronomy and Astrophysics 34 (1996), S. 111-154 
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    Topics: Physics
    Notes: Abstract A violent outflow of high-velocity gas is one of the first manifestations of the formation of a new star. Such outflows emerge bipolarly from the young object and involve amounts of energy similar to those involved in accretion processes. The youngest (proto-)stellar low-mass objects known to date (the Class 0 protostars) present a particularly efficient outflow activity, indicating that outflow and infall motions happen simultaneously and are closely linked since the very first stages of the star formation processes. This article reviews the wealth of information being provided by large millimeter-wave telescopes and interferometers on the small-scale structure of molecular outflows, as well as the most recent theories about their origin. The observations of highly collimated CO outflows, extremely high velocity (EHV) flows, and molecular "bullets" are examined in detail, since they provide key information on the origin and propagation of outflows. The peculiar chemistry operating in the associated shocked molecular regions is discussed, highlighting the recent high-sensitivity observations of low-luminosity sources. The classification schemes and the properties of the driving sources of bipolar outflows are summarized with special attention devoted to the recently identified Class 0 protostars. All these issues are crucial for building a unified theory on the mass-loss phenomena in young stars.
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    Annual Review of Astronomy and Astrophysics 34 (1996), S. 155-206 
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    Topics: Physics
    Notes: Abstract We discuss current observational and theoretical knowledge of magnetic fields, especially the large-scale structure in the disks and halos of spiral galaxies. Among other topics, we consider the enhancement of global magnetic fields in the interarm regions, magnetic spiral arms, and representations as superpositions of azimuthal modes, emphasizing a number of unresolved questions. It is argued that a turbulent hydromagnetic dynamo of some kind and an inverse cascade of magnetic energy gives the most plausible explanation for the regular galactic magnetic fields. Primordial theory is found to be unsatisfactory, and fields of cosmological origin may not even be able to provide a seed field for a dynamo. Although dynamo theory has its own problems, the general form of the dynamo equations appears quite robust. Finally, detailed models of magnetic field generation in galaxies, allowing for factors such as spiral structure, starbursts, galactic winds, and fountains, are discussed and confronted with observations.
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Astronomy and Astrophysics 34 (1996), S. 551-606 
    ISSN: 0066-4146
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Physics
    Notes: Abstract Stars over essentially the whole mass domain can become pulsationally unstable during various stages of their evolution. They will appear as variable stars with characteristics that are of much diagnostic value to astronomers. The analysis of such observations provides a challenging and unique approach to study aspects of the internal constitution and evolutionary status of these objects that are not accessible otherwise. This review touches on most classes of known pulsating variable stars and tries to elucidate connections to stellar physical aspects. To aid future investigations, we stress questions and problems that we believe are yet to be resolved satisfactorily.
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Fluid Mechanics 28 (1996), S. 129-185 
    ISSN: 0066-4189
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision Mechanics , Physics
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Fluid Mechanics 28 (1996), S. 45-82 
    ISSN: 0066-4189
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision Mechanics , Physics
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Fluid Mechanics 28 (1996), S. 279-321 
    ISSN: 0066-4189
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision Mechanics , Physics
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    Annual Review of Earth and Planetary Sciences 24 (1996), S. 63-87 
    ISSN: 0084-6597
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Geosciences , Physics
    Notes: Abstract Recent advances in computational physics allow numerical simulation of three-dimensional complex flows through arbitrarily complex geometries. Moreover, new technology for noninvasive imaging provides detailed three-dimensional tomographic reconstructions of porous rocks with a resolution approaching one micron. These two innovations are leading to new understanding of how the microscopic complexity of natural porous media influences fluid transport at a larger, macroscopic scale. This review describes new insights concerning single-phase and multiphase porous flow derived from numerical simulation. In particular, results concerning scaling relations between macroscopic parameters, the scale dependence of transport properties, and viscous coupling in multicomponent flow are emphasized.
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Nuclear and Particle Science 46 (1996), S. 1-30 
    ISSN: 0163-8998
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    Annual Review of Nuclear and Particle Science 46 (1996), S. 31-70 
    ISSN: 0163-8998
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    Topics: Physics
    Notes: Abstract A quantitative model, based on hadronic physics and Monte Carlo cascading, is described and applied to heavy ion collisions at BNL-AGS energies (~ 14 GeV/u). The model was found to be in excellent agreement with particle spectra where data previously existed, for Si beams, and was able to successfully predict the spectra where data were initially absent, for Au beams. For Si + Au collisions, baryon densities of three or four times the normal nuclear matter density (rho0) are seen in the theory, whereas for Au + Au collisions, matter at densities up to 10 rho0 is anticipated. The possibility that unusual states of matter may be created by the Au beams and potential signatures for its observation are considered.
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    Annual Review of Nuclear and Particle Science 46 (1996), S. 281-319 
    ISSN: 0163-8998
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Physics
    Notes: Abstract The demand for instrumentation capable of detecting and triggering on ionizing radiation in high-rate particle physics experiments at colliding-beam and fixed-target accelerator facilities and for spacecraft-borne instrumentation in astrophysics has led to the development of new tracking technologies. One of these, scintillating fiber tracking, combines the speed and efficiency of a scintillation detector with the flexibility and hermeticity afforded by fiber technology. A paradigm for a fiber-tracking detector that utilizes organic plastic fibers read out with visible-light photon counters is presented and critiqued. Alternate strategies are considered, and an overview of recent experimental applications is provided.
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    Annual Review of Nuclear and Particle Science 46 (1996), S. 197-235 
    ISSN: 0163-8998
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    Topics: Physics
    Notes: Abstract Recent data from the Tevatron collider have revealed that the production rate of prompt charmonium at large transverse momentum is orders of magnitude larger than the best theories of a few years ago had predicted. These surprising results can be understood by taking into account two recent developments that have dramatically revised the theoretical description of heavy-quarkonium production. The first is the realization that fragmentation must dominate at large transverse momentum, which implies that most charmonium in this kinematic region is produced by the hadronization of individual high-pT partons. The second is the development of a factorization formalism for quarkonium production based on nonrelativistic QCD that allows the formation of charmonium from color-octet pairs to be treated systematically. This review summarizes these theoretical developments and their implications for quarkonium production in high-energy colliders.
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    Annual Review of Nuclear and Particle Science 46 (1996), S. 395-469 
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    Topics: Physics
    Notes: Abstract We review recent experimental results on lifetimes and on hadronic decays of hadrons that contain c and b quarks. The theoretical implications of these results are also considered. An understanding of hadronic decays of heavy quarks is required to interpret the charge-parity-violating asymmetries in B decays that will be observed in experiments planned for the near future.
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    Annual Review of Nuclear and Particle Science 46 (1996), S. 609-645 
    ISSN: 0163-8998
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    Topics: Physics
    Notes: Abstract This review discusses the experimental and theoretical status of various parton-model sum rules. The basis of the sum rules in perturbative quantum chromodynamics is discussed. Their use in extracting the value of the strong coupling constant is evaluated, and the failure of the naive version of some of these sum rules is assessed.
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    Annual Review of Earth and Planetary Sciences 24 (1996), S. 15-40 
    ISSN: 0084-6597
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Geosciences , Physics
    Notes: Abstract Although the temperature at the top of the lower mantle is well constrained by phase equilibrium data for the transformation of transition zone minerals to the denser perovskite polymorphs, the temperature distribution in the lower mantle is poorly known. Models depend strongly on the assumptions of the amount of internal heating and the viscosity profile. New melting data on iron to pressures of the outer core (2 Mbar) and the observed strong decrease of eutectic melting depression in the Fe-FeO-FeS system with increasing pressure, however, tightly constrain the temperature at the inner-core boundary to slightly less than 5000 K. This estimate can be reconciled with all recent static melting measurements on iron and lays within the uncertainty of shock temperature measurements. The resulting temperature at the core-mantle boundary of about 4000 K then requires a large temperature gradient at the bottom of the lower mantle of about 1500 K. Recent findings of the very high melting temperatures of the major lower-mantle materials Mg-Si-perovskite and magnesiowustite indicate that this increase in temperature does not cause melting in the lower mantle.
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    Annual Review of Earth and Planetary Sciences 24 (1996), S. 225-262 
    ISSN: 0084-6597
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Geosciences , Physics
    Notes: Abstract Changes of the isotopic composition of water within the water cycle provide a recognizable signature, relating such water to the different phases of the cycle. The isotope fractionations that accompany the evaporation from the ocean and other surface waters and the reverse process of rain formation account for the most notable changes. As a result, meteoric waters are depleted in the heavy isotopic species of H and O relative to ocean waters, whereas waters in evaporative systems such as lakes, plants, and soilwaters are relatively enriched. During the passage through the aquifers, the isotope composition of water is essentially a conservative property at ambient temperatures, but at elevated temperatures, interaction with the rock matrix may perturb the isotope composition. These changes of the isotope composition in atmospheric waters, surface water, soil, and groundwaters, as well as in the biosphere, are applied in the characterization of hydrological system as well as indicators of paleo-climatological conditions in proxy materials in climatic archives, such as ice, lake sediments, or organic materials.
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    Annual Review of Earth and Planetary Sciences 24 (1996), S. 385-432 
    ISSN: 0084-6597
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Geosciences , Physics
    Notes: Abstract Seismic anisotropy beneath continents is analyzed from shear-wave splitting recorded at more than 300 continental seismic stations. Anisotropy is found to be a ubiquitous property that is due to mantle deformation from past and present orogenic activity. The observed coherence with crustal deformation implies that the mantle plays a major, if not dominant, role in orogenies. No evidence is found for a continental asthenospheric decoupling zone, suggesting that continents are coupled to general mantle circulation.
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 24 (1996), S. 1-13 
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    Annual Review of Earth and Planetary Sciences 24 (1996), S. 41-62 
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    Topics: Geosciences , Physics
    Notes: Abstract Over the past decade, significant progress has been made in understanding the rheological properties of partially molten mantle rocks. Laboratory experiments demonstrate that a few percent of melt can have an unexpectedly large effect on viscosity both in the diffusional creep regime and in the dislocation creep regime. In both cases, the enhancement in creep rate is much larger than anticipated based on deformation models because melt wets at least a fraction of the grain boundaries. For diffusion creep, the wetted interfaces provide a rapid diffusion path that is not included in analyses based on melt distribution in isotropic melt-crystal systems. For dislocation creep, two points require consideration. First, even without a melt phase present, fine-grained samples deformed in the dislocation creep field flow a factor of ~10 faster than coarse-grained rocks due to contributions from grain boundary mechanisms to the deformation process. Second, melt has only a small effect on creep rate for coarse-grained rocks but has a relatively large effect for fine-grained samples. Thus, because olivine has only a limited number of slip systems, grain boundaries contribute significantly to deformation of fine-grained rocks in the dislocation creep regime, provided that deformation occurs near the transition between diffusional creep and dislocation creep. Based on laboratory measurements, this transition is expected to occur at a grain size of about 6 mm for a differential stress of 0.1 MPa. Therefore, under mantle conditions, even a few percent melt should reduce the viscosity by as much as a factor of 10. A broad range of problems related to deformation beneath mid-ocean ridges and in the mantle wedge above subducting slabs can now be addressed using experimentally determined rheologies for partially molten mantle rocks.
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    Annual Review of Earth and Planetary Sciences 24 (1996), S. 89-123 
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    Topics: Geosciences , Physics
    Notes: Abstract Earth-based stellar occultations probe the temperature, pressure, and number-density profiles of planetary atmospheres in the microbar range with a vertical resolution of a few kilometers. Depending on the occultation data available for a given body and other information, the technique also allows determination of local density variations, extinction by aerosols and molecules, rotation period and zonal winds, atmospheric composition, and the temporal and spatial variability of an atmosphere. A brief quantitative description of the interaction of starlight with a planetary atmosphere is presented, and observational techniques are discussed. Observational results through 1995 are presented for Venus, Mars, Jupiter, Saturn, Titan, Neptune, Triton, Pluto, and Charon.
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    Annual Review of Physical Chemistry 47 (1996), S. 1-41 
    ISSN: 0066-426X
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Chemistry and Pharmacology , Physics
    Notes: Small effusive leaks in vacuum systems, as in Knudsen cells and classical molecular beam machines, are responsible for many contributions to science in the twentieth century. Beginning in the 1950s, big convective leaks have turned out to be even more powerful and versatile investigative tools. Forming supersonic free jets, they have greatly expanded molecular beam methods, become the cornerstone of cluster science and technology, rewritten the book on molecular spectroscopy, and are adding new dimension to mass spectrometry. This account is the story of one man's experiences as a bystander and participant in these developments.
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    Annual Review of Physical Chemistry 47 (1996), S. 205-241 
    ISSN: 0066-426X
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Chemistry and Pharmacology , Physics
    Notes: Abstract Various aspects of molecular solvation are reviewed from the perspective provided by gas-phase aromatic solute-(solvent)n clusters. Particular emphasis is placed on hydrogen-bonded clusters, varying from 1:1 aromatic-H2O complexes up to clusters containing several water or methanol molecules. Recent advances in experimental methods for obtaining accurate structures, binding energies, and intermolecular and intramolecular vibrational spectra are highlighted. Many of these methods provide size and conformation selectivity and can be readily extended to both ground and electronically excited neutral states. The pi hydrogen bond, hydrogen bonding to aromatic alcohols, water complexation to indole and its derivatives, and the hydrogen-bonded networks of benzene-(H2O)n and benzene-(CH3OH)n clusters are reviewed in special detail.
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    Annual Review of Physical Chemistry 47 (1996), S. 283-325 
    ISSN: 0066-426X
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Chemistry and Pharmacology , Physics
    Notes: Abstract The history of superconductivity, including superconductivity in the high-Tc cuprates, is reviewed very briefly, and the differences between conventional superconductors and the high-Tc cuprates are summarized. The basic crystal structures of the major series of high-Tc cuprates are described and compared. The relation of structures to superconducting properties is reviewed with an emphasis on the orthorhombic-tetragonal transition in (La2-x Srx)CuO4; the corresponding transition, and also the transition to the low-temperature tetragonal phase in (La2-xBax)CuO4; and the effects of oxygen vacancies, oxygen-vacancy ordering, frozen-in disorder, and occupation of the off-chain O(5) sites in YBa2Cu3O7-delta. The effects of chemical substitutions of lanthanide elements on the La/Sr sites in (La2-xSrx)CuO4 and on the Y sites in YBa2Cu3O7-delta, and of 3d elements and sp elements on the Cu sites in both systems are reviewed. The difference between the effects of the lanthanide substitutions, particularly Pr, in the two systems are considered. Major properties of the Bi-, Tl-, and Hg-cuprates, are described briefly. A comparison of the high-Tc cuprates with noncuprate oxide superconductors is given.
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    Annual Review of Earth and Planetary Sciences 24 (1996), S. 125-190 
    ISSN: 0084-6597
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    Topics: Geosciences , Physics
    Notes: Abstract Io, innermost of Jupiter's large moons, is one of the most unusual objects in the Solar System. Tidal heating of the interior produces a global heat flux 40 times the terrestrial value, producing intense volcanic activity and a global resurfacing rate averaging perhaps 1 cm yr-1. The volcanoes may erupt mostly silicate lavas, but the uppermost surface is dominated by sulfur compounds including SO2 frost. The volcanoes and frost support a thin, patchy SO2 atmosphere with peak pressure near 10-8 bars. Self-sustaining bombardment of the surface and atmosphere by Io-derived plasma trapped in Jupiter's magnetosphere causes escape of material from Io (predominantly sulfur, oxygen, and sodium atoms, ions, and molecules) at a rate of about 103 kg s-1. The resulting Jupiter-encircling torus of ionized sulfur and oxygen dominates the Jovian magnetosphere and, together with an extended cloud of neutral sodium, is readily observable from Earth.
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    Annual Review of Earth and Planetary Sciences 24 (1996), S. 263-337 
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    Topics: Geosciences , Physics
    Notes: Abstract Turkic-type orogeny is a class of collisional mountain building, in which the precollision history of one, or both, of the colliding continents involves the growth of very large, subcontinent-size subduction-accretion complexes, into which magmatic arc axes commonly migrate and thus enlarge the continent to which they are attached. A review of the evolution of two Phanerozoic (Altaids, Nipponides), one Neoproterozoic (East African), and one Archean (Yilgarn) Turkic-type orogens shows that this type of orogeny may have been the principal builder of the continental crust through recorded Earth history. The total juvenile material added to Turkic-type orogens at any one time in the Phanerozoic seems close to 1 km3/year, which about equals the amount of material annually fed into the mantle at subduction zones. As some 0.02 to 0.03% of that material is generally agreed to return to the crust by arc magmatism, these figures provide a minimum net growth rate for the continental crust during the Phanerozoic.
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    Annual Review of Earth and Planetary Sciences 24 (1996), S. 191-224 
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    Topics: Geosciences , Physics
    Notes: Abstract Geophysical estimates of mid-ocean ridge axial heat fluxes (2-4 x 1012 W) and of the total hydrothermal flux (9 +- 2 x 1012 W) are well established. Problems arise in calculation of water fluxes because of uncertainties in (a) values of off-axis fluxes and (b) the partition of axial heat flow between high-temperature black smoker and lower-temperature diffuse flow. Of the various geochemical methods of estimating fluxes, 3 He/heat data are extremely variable, the Mg method is sensitive to flank fluxes, Sr isotopes agree with geophysical estimates only if flank fluxes are important, Li isotopes data are consistent with geophysical values, and Ge/Si ratios give low fluxes, which may reflect low-temperature processes not yet fully quantified. Estimates of hydrothermal heat and water fluxes derived from these approaches are presented as are hydrothermal chemical fluxes at the ridge axis, off axis, and as affected by hydrothermal plumes.
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    Annual Review of Earth and Planetary Sciences 24 (1996), S. 339-384 
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    Topics: Geosciences , Physics
    Notes: Abstract Continental North America's greatest earthquake sequence struck on the western frontier of the United States. The frontier was not then California but the valley of the continent's greatest river, the Mississippi, and the sequence was the New Madrid earthquakes of the winter of 1811-1812. Their described impacts on the land and the river were so dramatic as to produce widespread modern disbelief. However, geological, geophysical, and historical research, carried out mostly in the past two decades, has verified much in the historical accounts. The sequence included at least six (possibly nine) events of estimated moment magnitude M〉= 7 and two of M= 8. The faulting was in the intruded crust of a failed intracontinental rift, beneath the saturated alluvium of the river valley, and its violent shaking resulted in massive and extensive liquefaction. The largest earthquakes ruptured at least six (and possibly more than seven) intersecting fault segments, one of which broke the surface as a thrust fault that disrupted the bed of the Mississippi River in at least 2 (and possibly four) places. ...it is a riddle wrpped in a mystery inside an enigma. Winston Churchill
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    Annual Review of Earth and Planetary Sciences 24 (1996), S. 433-464 
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    Topics: Geosciences , Physics
    Notes: Abstract Paleontologists have always been concerned about the documentary quality of the fossil record, and this has also become an important issue for biologists, who increasingly look to accumulations of bones, shells, and plant material as possible ways to extend the time-frame of observation on species and community behaviors. Quantitative data on the postmortem behavior of organic remains in modern environments are providing new insights into death and fossil assemblages as sources of biological information. Important findings include: 1. With the exception of a few circumstances, usually recognizable by independent criteria, transport out of the original life habitat affects few individuals. 2. Most species with preservable hardparts are in fact represented in the local death assemblage, commonly in correct rank importance. Molluscs are the most durable of modern aquatic groups studied so far, and they show highest fidelity to the original community. 3. Time-averaging of remains from successive generations and communities often prevents the detection of short-term (seasons, years) variability but provides an excellent record of the natural range of community composition and structure over longer periods. Thus, although a complex array of processes and circumstances influences preservation, death assemblages of resistant skeletal elements are for many major groups good to excellent records of community composition, morphological variation, and environmental and geographic distribution of species, and such assemblages can record temporal dynamics at ecologically and evolutionarily meaningful scales.
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    Annual Review of Nuclear and Particle Science 46 (1996), S. 71-107 
    ISSN: 0163-8998
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Physics
    Notes: Abstract We provide an overview of the present understanding of the transition from hadrons to a quark-gluon plasma, its signatures, and the experimental results so far. We discuss results of numerical simulations of the lattice gauge theory and critically evaluate the various observables that have been proposed as signatures of the QCD phase transition. We place the existing data from relativistic heavy-ion experiments at the Brookhaven Alternating Gradient Synchrotron (AGS) and CERN Super Proton Synchrotron (SPS) into perspective and provide an overview of the techniques and strategies that will be employed in the search for the quark-gluon plasma at heavy-ion colliders, such as the Relativistic Heavy-Ion Collider (RHIC) and the Large Hadron Collider (LHC).
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    Annual Review of Nuclear and Particle Science 46 (1996), S. 351-393 
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    Topics: Physics
    Notes: Abstract New results from LEAR experiments on the search for glueballs and other non- states have attracted considerable attention, particularly the discovery of the f0(1500), which is an excellent candidate for the scalar glueball. This article gives an overview about the special features of annihilation for meson spectroscopy, and about the use of initial and final-state selection for quantum-number filtering. The general model underlying the partial-wave analysis is discussed. An overview about the Crystal Barrel, OBELIX, and Jetset experiments and their results is followed by a comparison of results from other production mechanisms. Finally, an interpretation of the new results is given.
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    Annual Review of Nuclear and Particle Science 46 (1996), S. 149-195 
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    Topics: Physics
    Notes: Abstract Since the discovery of the bottom quark in 1977, physicists have searched for the top quark, the weak isospin partner of the bottom quark. Indirect evidence and estimates of its mass have been made; however, direct observation eluded scientists until recently. In the spring of 1995, two experiments, CDF and DO, at Fermi National Accelerator Laboratory showed top-antitop quark pairs created from proton-antiproton collisions. In this report, we summarize the experimental status prior to 1995 and discuss the experiments and techniques that in March of 1995 resulted in discovery of the top quark. Studies of the top quark's properties, such as its mass and production cross section, are just beginning. We present an overview of the current status of these measurements and a perspective on the prospects for the future.
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    Annual Review of Nuclear and Particle Science 46 (1996), S. 321-350 
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    Topics: Physics
    Notes: Abstract The Coulomb dissociation process, induced by the intense source of quasi-real photons acting as nuclear particles pass through the field of a heavy nucleus, has attracted a great deal of attention. As a specific application, and as a means of access to the time-reversed radiative-capture reactions, which are of astrophysical interest at stellar energies, this process provides several advantages, based on larger cross sections and on the flexibilities of the breakup kinematics. Difficulties in the analysis arise from possible interference by nuclear interactions and final-state effects through multiphoton exchange (postacceleration), which need careful consideration. A number of theoretical and experimental investigations that have been performed, since the introduction of this novel approach have provided interesting new information, resulting in an improved and detailed understanding of the experimental conditions, and of the theoretical basis of the method. The progress in experiment and theory is reviewed, and various cases of actual interest and current applications are discussed.
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    Annual Review of Nuclear and Particle Science 46 (1996), S. 533-608 
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    Topics: Physics
    Notes: Abstract We describe the anticipated experimental program of an e+e- linear collider in the energy region 500 GeV-1.5 TeV, emphasizing topics relevant to the mystery of electroweak symmetry breaking.
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    Annual Review of Nuclear and Particle Science 46 (1996), S. 109-148 
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    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Physics
    Notes: Abstract We review progress in calculating the one-loop scattering amplitudes required for next-to-leading-order corrections to QCD processes. The underlying technical developments include the spinor helicity formalism, color decompositions, supersymmetry, string theory, factorization, and unitarity. We provide explicit examples that illustrate these techniques.
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    Annual Review of Nuclear and Particle Science 46 (1996), S. 237-279 
    ISSN: 0163-8998
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Physics
    Notes: Abstract A mesoscopic system with strong interaction between constituents, the atomic nucleus is a good candidate for studying the manifestations of quantum chaos. Recent experimental and theoretical developments give clear evidence of the dominant role chaotic dynamics plays not only in local level statistics, but also in the damping of collective motion, isospin and parity nonconservation, thermalization, and decay into continuum. In this review, those and other phenomena are discussed from the general viewpoint of quantum chaos and complexity. The complexity of eigenstates measured by information entropy in the mean-field basis is more informative than the standard signatures of chaos in the level statistics. It evolves regularly as a function of excitation energy and provides an alternative temperature scale. This sheds new light on the problems of foundations of statistical mechanics and quantum decoherence.
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    Annual Review of Nuclear and Particle Science 46 (1996), S. 471-532 
    ISSN: 0163-8998
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Physics
    Notes: Abstract The need for very good energy resolution in experiments in particle and astroparticle physics and the need to detect very small energy depositions are the major motivations for the development of low-temperature particle detectors. Because the energy quanta associated with superconductors and lattice vibrations (phonons) are more than one hundred times smaller, substantial improvements have been obtained in energy resolution and in sensitivity over conventional detectors. Furthermore, these detection schemes permit tailoring of target or absorber materials to match the physics requirements. In this article, the basic physics principles behind various methods of detecting excitations induced by particle interactions in bulk single-crystal materials at low temperatures are reviewed. We also present an overview of progress toward implementation of particle physics experiments, such as detection of low-energy neutrinos, search for dark-matter particles, search for neutrino-less double beta decay, and beta- and gamma-ray spectroscopy and X-ray astronomy using low-temperature detectors.
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  • 78
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    Annual Review of Physical Chemistry 47 (1996), S. 109-134 
    ISSN: 0066-426X
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Chemistry and Pharmacology , Physics
    Notes: Abstract Experimental and theoretical studies of polar solvation dynamics and spectral line broadening are described. Photon echo and fluorescence Stokes shift experiments are discussed, and the relationship between the information content of the two techniques clarified. The interaction of the chromophore with its solvent bath is described by a spectral density, and the connection of this spectral density with the liquid's instantaneous normal modes discussed. The ubiquity of the ultrafast phase of solvation dynamics is demonstrated, and a discussion of its physical origin given. The slower phases of solvation vary strongly from solvent to solvent. Molecular theories of liquid dynamics are able to rationalize such variations over at least a 2000-fold range of time scale. The review concludes with a brief discussion of the relevance of ultrafast solvation to chemical dynamics.
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    Annual Review of Physical Chemistry 47 (1996), S. 135-169 
    ISSN: 0066-426X
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Chemistry and Pharmacology , Physics
    Notes: Abstract The NMR chemical shift serves as a paradigm for molecular electronic properties. We consider the factors that determine the general magnitudes of the shifts, the state of the art in theoretical calculations, the nature of the shielding tensor, and the multidimensional shielding surface that describes the variation of the shielding with nuclear positions. We also examine the nature of the intermolecular shielding surface as a general example of a supermolecule property surface. The observed chemical shift in the zero-pressure limit is determined not only by the value of the shielding at the equilibrium geometry, but the dynamic average over the multidimensional shielding surface during rotation and vibration of the molecule. In the gas, solution, or adsorbed phase it is an average of the intermolecular shielding surface over all the configurations of the molecule with its neighbors. The temperature dependence of the chemical shift in the isolated molecule, the changes upon isotopic substitution, the changes with environment, are well characterized experimentally so that quantum mechanical descriptions of electronic structure and theories related to dynamics averaging of any electronic property can be subjected to stringent test.
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    Annual Review of Physical Chemistry 47 (1996), S. 397-419 
    ISSN: 0066-426X
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Chemistry and Pharmacology , Physics
    Notes: Abstract A simple method for calculating the electronic energy of extended solids is discussed in this review. This method is based on the Huckel or tight-binding theory in which an explicit pairwise repulsion is added to the generally attractive forces of the partially filled valence electron bands. An expansion based on the power moments of the electronic density of states is discussed, and the structural energy difference theorem is reviewed. The repulsive energy is found to vary linearly with the second power moment of the electronic density of states. These results are then used to show why there is such a diversity of structure in the solid state. The elemental structures of the main group are rationalized by the above methods. It is the third and fourth power moments (which correspond in part to triangles and squares of bonded atoms) that account for much of the elemental structures of the main group elements of the periodic table. This serves as an introduction to further rationalizations of transition for noble metal alloy, binary and ternary telluride and selenide, and other intermetallic structures.Thus a cohesive picture of both covalent and metallic bonding is presented in this review, illustrating the importance of atomic orbitals and their overlap integrals.
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  • 81
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    Annual Review of Physical Chemistry 47 (1996), S. 527-554 
    ISSN: 0066-426X
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Chemistry and Pharmacology , Physics
    Notes: Abstract It is technologically important to understand how halogens react with semiconductor surfaces because halogen compounds are commonly used to etch semiconductor wafers in the microelectronics industry. Halogens are also model adsorbates for studying chemisorption on covalently bonded materials, such as semiconductors, owing to the simple nature of the bonds that they form. The growing use of III-V materials in the manufacture of optoelectronic devices has prompted investigations of the reactions of molecular halogens (XeF2, Cl2, Br2, and I2) with III-V semiconductor surfaces (GaAs, GaSb, InP, InAs, and InSb). This review examines the more fundamental of these investigations, which involve model systems in ultra-high vacuum, focusing on the chemistry of the halogen surface reactions and the physical and electronic structure of the reacted surfaces.
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  • 82
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    Annual Review of Physical Chemistry 47 (1996), S. 171-204 
    ISSN: 0066-426X
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Chemistry and Pharmacology , Physics
    Notes: Abstract Crystallization is necessary to obtain the three-dimensional structure of proteins and nucleic acids; it often represents the bottleneck in structure determination. Our understanding of crystallization mechanisms is still incomplete. In this review, we emphasize fundamental aspects of the crystallization process. Protein-protein contacts in crystals are complex, involving a delicate balance of specific and nonspecific interactions. Depending on solution conditions, these interactions can lead to nucleation of crystals or to amorphous aggregation; this stage of crystallization has been successfully studied by light scattering. Post nucleation crystal growth may proceed by mechanisms involving crystal defects or two-dimensional nucleation, as observed by atomic force and interference microscopy. Cessation of growth has been observed but remains incompletely understood. Impurities may play important roles during all stages of crystallization. Phase diagrams can guide optimization of conditions for nucleation and subsequent crystal growth; a theoretical understanding relating these to the intermolecular interactions is beginning to develop.
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  • 83
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    Annual Review of Physical Chemistry 47 (1996), S. 327-367 
    ISSN: 0066-426X
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Chemistry and Pharmacology , Physics
    Notes: Abstract This review involves chemical kinetics of atmospheric reactions, with emphasis on gas phase and heterogeneous processes related to the following topics: (a) in the troposphere, chemistry of CFC/Halon replacement compounds and chemistry of sulfur species and (b) in the stratosphere, chemistry of fluorine, bromine, and iodine species and of heterogeneous processes occurring on sulfuric acid aerosols. The results of laboratory measurements of rate parameters are summarized, and current views are presented on the physical chemistry foundation underlying the interpretation of these kinetics parameters.
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    Annual Review of Physical Chemistry 47 (1996), S. 421-462 
    ISSN: 0066-426X
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Chemistry and Pharmacology , Physics
    Notes: Abstract Colloidal suspensions of uniformly sized microspheres can serve as powerful model systems for investigating many-body processes in condensed-matter physics. The ensemble of microspheres in such suspensions undergoes disorder-order transitions from fluids to crystals in direct analogy with the structural transitions experienced by atoms in conventional materials. Unlike atoms, however, colloidal spheres can be imaged and tracked using optical microscopy and computerized image processing. This review addresses issues in the physics of phase transitions that have been attacked through digital video microscopy of colloidal dispersions over the past decade. Particular emphasis is placed on microscopic mechanisms of melting and freezing and on the effects of geometric confinement on these fundamental processes.
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    Annual Review of Physical Chemistry 47 (1996), S. 81-108 
    ISSN: 0066-426X
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Chemistry and Pharmacology , Physics
    Notes: Abstract Radical-radical reactions generally proceed on potential energy surfaces that have no maximum. Collisional deactivation leads to a stable molecular product; alternatively, radical or molecular products can be formed via dissociation channels additional to those regenerating the reactants. Models of the transition states must take into account the loose internal motion of the fragments, and a variational approach is necessary. The competition between dissociation and collisional stabilization may be modeled using a master equation (ME). The types of behavior encountered in radical-radical reactions and their analysis using the ME are illustrated by reference to the reactions CH3 + H, CH3 + CH3, and CH3 + OH.
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    Annual Review of Physical Chemistry 47 (1996), S. 463-494 
    ISSN: 0066-426X
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Chemistry and Pharmacology , Physics
    Notes: Abstract The unprecedented high intensities made accessible by the development of ultrashort pulse laser systems have uncovered a host of new phenomena and changed the way that we think about atomic and molecular dynamics. We review these developments in the context of some of the basic models that have evolved to explain them. The successes and limitations of simple semiclassical models of strong-field atomic phenomena are discussed. Photodissociation dynamics have shown a rich complexity in strong fields-bond softening, above-threshold dissociation, coulomb explosion-which we review. The promise of the new laser systems in the field of coherent control of molecular dynamics is also discussed.
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    Annual Review of Physical Chemistry 47 (1996), S. 555-606 
    ISSN: 0066-426X
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Chemistry and Pharmacology , Physics
    Notes: Abstract The interaction of light within tissue has been used to recognize disease since the mid-1800s. The recent developments of small light sources, detectors, and fiber optic probes provide opportunities to quantitatively measure these interactions, which yield information for diagnosis at the biochemical, structural, or (patho)physiological level within intact tissues. However, because of the strong scattering properties of tissues, the reemitted optical signal is often influenced by changes in biochemistry (as detected by these spectroscopic approaches) and by physiological and pathophysiological changes in tissue scattering. One challenge of biomedical optics is to uncouple the signals influenced by biochemistry, which themselves provide specificity for identifying diseased states, from those influenced by tissue scattering, which are typically unspecific to a pathology. In this review, we describe optical interactions pursued for biomedical applications (fluorescence, fluorescence lifetime, phosphorescence, and Raman from cells, cultures, and tissues) and then provide a descriptive framework for light interaction based upon tissue absorption and scattering properties. Finally, we review important endogenous and exogenous biological chromophores and describe current work to employ these signals for detection and diagnosis of disease.
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    Annual Review of Physical Chemistry 47 (1996), S. 43-80 
    ISSN: 0066-426X
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Chemistry and Pharmacology , Physics
    Notes: Abstract The experimental and computational study of clusters has been an active field of research for over a decade. This review provides an overview of some of the methods that have been developed to study clusters and some of the results that have been obtained. Included are computational approaches to explore the potential energy surface for clusters, methods to extract thermodynamic properties from the potential surface information and approaches to insure simulation studies are performed in an ergodic fashion. The methods have proved to be useful in studying the structural transition from clusters to bulk phases, phase changes in small clusters and the importance of quantum effects. The review ends with a discussion of problems in cluster chemistry and physics that are of interest for future investigations.
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    Annual Review of Physical Chemistry 47 (1996), S. 243-282 
    ISSN: 0066-426X
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Chemistry and Pharmacology , Physics
    Notes: Abstract NMR relaxation experiments can provide information on overall and internal motions in proteins. This review consists of a concise report on the evolution of the theories for nuclear relaxation followed by an overview of mathematical models for internal motions in proteins. Next, the method of spectral density mapping with recent developments is reviewed. This is followed by a discussion of pulse sequences for relaxation experiments. Finally, we review recent studies correlating relaxation parameters, in particular spectral density functions, with structural features of proteins and with results of molecular dynamics simulations.
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    Annual Review of Physical Chemistry 47 (1996), S. 369-395 
    ISSN: 0066-426X
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Chemistry and Pharmacology , Physics
    Notes: Abstract NMR has emerged as an important tool for studies of protein folding because of the unique structural insights it can provide into many aspects of the folding process. Applications include measurements of kinetic folding events and structural characterization of folding intermediates, partly folded states, and unfolded states. Kinetic information on a time scale of milliseconds or longer can be obtained by real-time NMR experiments and by quench-flow hydrogen-exchange pulse labeling. Although NMR cannot provide direct information on the very rapid processes occurring during the earliest stages of protein folding, studies of isolated peptide fragments provide insights into likely protein folding initiation events. Multidimensional NMR techniques are providing new information on the structure and dynamics of protein folding intermediates and both partly folded and unfolded states.
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    Annual Review of Physical Chemistry 47 (1996), S. 495-525 
    ISSN: 0066-426X
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Chemistry and Pharmacology , Physics
    Notes: Abstract In recent years we have witnessed tremendous progress in our understanding of unimolecular reactions on a fully state-resolved level. Here we describe recent state-resolved experimental studies of resonances in unimolecular reactions, focusing on the transition from isolated to overlapping resonances. Depending on the well depth and extent of intramolecular vibrational energy redistribution, the resonances can exhibit properties ranging from mode- and state-selective to statistical behavior. In the statistical limit the resonances are usually overlapped, and interference effects may become prominent. We use recent studies of HCO, HFCO, and CH3O to examine the transition from mode-selective to statistical behavior in the isolated regime. Experimental and theoretical studies of NO2, including photofragment yield spectra, fully resolved NO quantum state distributions, and decomposition rates are used to examine unimolecular decomposition in the regime of overlapping resonances.
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  • 92
    Publication Date: 1996-08-01
    Description: No Abstract available.
    Print ISSN: 0065-9401
    Electronic ISSN: 1943-3646
    Topics: Geography , Geosciences , Physics
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    Print ISSN: 0066-4146
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