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  • Articles  (289,467)
  • Wiley  (204,032)
  • American Meteorological Society  (83,344)
  • Annual Reviews
  • Geosciences  (289,467)
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Years
  • 1
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 10 (1982), S. 235-256 
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  • 2
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 13 (1985), S. 29-47 
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  • 3
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 13 (1985), S. 175-199 
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  • 4
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 13 (1985), S. 297-314 
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  • 5
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 15 (1987), S. 73-95 
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  • 6
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 15 (1987), S. 171-212 
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  • 7
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 13 (1985), S. 345-383 
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  • 8
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 13 (1985), S. 269-296 
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  • 9
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 13 (1985), S. 385-428 
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  • 10
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 15 (1987), S. 1-24 
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  • 11
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 15 (1987), S. 97-113 
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  • 12
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 17 (1989), S. 335-360 
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  • 13
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 17 (1989), S. 361-384 
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  • 14
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 17 (1989), S. 439-472 
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  • 15
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 17 (1989), S. 1-13 
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  • 16
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 19 (1991), S. 77-99 
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  • 17
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 19 (1991), S. 43-75 
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  • 18
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 19 (1991), S. 263-281 
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  • 19
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 19 (1991), S. 423-455 
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  • 20
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 19 (1991), S. 351-382 
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  • 21
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 1 (1973), S. 15-37 
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  • 22
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 1 (1973), S. 107-129 
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  • 23
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 1 (1973), S. 297-311 
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  • 24
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 1 (1973), S. 313-338 
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  • 25
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 21 (1993), S. 205-225 
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  • 26
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 21 (1993), S. 525-555 
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  • 27
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 22 (1994), S. 33-61 
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  • 28
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 22 (1994), S. 167-205 
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  • 29
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 22 (1994), S. 119-144 
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  • 30
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 22 (1994), S. 457-497 
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  • 31
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 22 (1994), S. 419-455 
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  • 32
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 23 (1995), S. 119-142 
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  • 33
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 23 (1995), S. 169-213 
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  • 34
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 23 (1995), S. 375-408 
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  • 35
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 23 (1995), S. 337-374 
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  • 36
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 22 (1994), S. 63-89 
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  • 37
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 22 (1994), S. 207-237 
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  • 38
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 23 (1995), S. 65-87 
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  • 39
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 26 (1998), S. 53-80 
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    Notes: Abstract Observations of suspected planet-forming disks provide estimates of protoplanetary disk masses, surface temperatures, and the rate at which mass is infalling onto the disks. Analyses of primitive meteorites and comets and their components constrain the solar nebula's temperature at the locations and times where those components were formed. Theoretical models of disks undergoing the accretion of mass from an infalling cloud envelope predict disk temperatures in good agreement with these constraints: a moderately warm (500-1500 K) inner disk, surrounded by a cool (50-150 K) outer disk. These models have important implications for the depletion of volatiles in the inner Solar System, for mechanisms of disk evolution, and for the orbital distances at which terrestrial and gas giant planets form.
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  • 40
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 23 (1995), S. 451-478 
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  • 41
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 24 (1996), S. 63-87 
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    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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  • 42
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    Annual Review of Earth and Planetary Sciences 28 (2000), S. 419-475 
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    Notes: Abstract This survey of the current status of research into Earth's orbitally forced paleoclimatic record summarizes recent developments in the theory of Earth's orbital parameters, and reviews how various techniques of data collection and analysis have fared in the search and recovery of orbital signals in ancient stratigraphy. The emerging significance of the quasi-periodicity of Earth's orbital variations as a principal tool in the analysis of orbitally forced stratigraphy is discussed in detail. Five case studies are presented that illustrate new directions in research: (a) time series analysis of discontinuous strata; (b) measurement of ultra-high resolution stratigraphic signals; (c) new perspectives on the 100 kyr Pleistocene glaciation problem; (d) stratigraphic evidence for solar system resonance modes; and (e) evaluating Phanerozoic length of day from orbitally forced stratigraphy.
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  • 43
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    Annual Review of Earth and Planetary Sciences 28 (2000), S. 571-610 
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    Notes: Abstract Theories of scaling apply wherever similarity exists across many scales. This similarity may be found in geometry and in dynamical processes. Universality arises when the qualitative character of a system is sufficient to quantitatively predict its essential features, such as the exponents that characterize scaling laws. Within geomorphology, two areas where the concepts of scaling and universality have found application are the geometry of river networks and the statistical structure of topography. We begin this review with a pedagogical presentation of scaling and universality. We then describe recent progress made in applying these ideas to networks and topography. This overview leads to a synthesis that attempts a classification of surface and network properties based on generic mechanisms and geometric constraints. We also briefly review how scaling and universality have been applied to related problems in sedimentology-specifically, the origin of stromatolites and the relation of the statistical properties of submarine-canyon topography to the size distribution of turbidite deposits. Throughout the review, our intention is to elucidate not only the problems that can be solved using these concepts, but also those that cannot.
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  • 44
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    Annual Review of Earth and Planetary Sciences 29 (2001), S. 47-69 
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    Notes: Abstract This paper reviews recent research focused on the Earth's inner core. Large inner-core traveltime anomalies and the anomalous splitting of core-sensitive free oscillations strongly suggest that the inner core is anisotropic. Initial models involved a simple, constant or depth-dependent cylindrical anisotropy at a level less than a few percent. Recent observations suggest that its eastern hemisphere is largely isotropic, whereas its western hemisphere is highly anisotropic, and there are indications that its top 100 km may be isotropic. The coda of inner-core reflected phases has been used to infer strong heterogeneities with a length scale of just a few kilometers. Thus, a complicated three-dimensional picture of the inner core is beginning to emerge, although it has been suggested that much of this complexity may be the misinterpretation of signals that have their origin in the lowermost mantle. Numerical models of the geodynamo suggest that the inner core may rotate at a slightly different rate than the mantle. Recent seismological estimates based upon traveltime and normal-mode data limit inner-core differential rotation to less than +0.2 degrees per year.
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  • 45
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    Annual Review of Earth and Planetary Sciences 29 (2001), S. 135-163 
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    Notes: Abstract The recycling of elements by plants and plant-induced biological activity cause the rates and products of weathering to be markedly different from what would result in abiotic processes. Plants directly control water dynamics, weathering, and the chemistry of weathering solutions, which is clearly exhibited in equatorial areas where old weathering mantles are greatly influenced by biological activity. Depending on the dynamics of plant-induced organometallic compounds, this weathering results in either clayey soils, which are in a dynamic equilibrium sustained by the forest's cycling of elements, or sandy soils. In most places (tropical as well temperate areas), the weathering mantle can be regarded as being in a dynamic equilibrium sustained by plants.
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  • 46
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    Annual Review of Earth and Planetary Sciences 30 (2002), S. 65-88 
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    Notes: Abstract Molecular and paleontological data provide independent means of estimating when groups of organisms evolved in the geological past, but neither approach can be considered straightforward. The single most fundamental obstacle to developing an accurate estimate of times of origination from gene sequence data is variation in rates of molecular evolution, both through time and among lineages. Although various techniques have been proposed to circumvent this problem, none unambiguously allow the components of time and rate to be separated. Furthermore, problems of establishing accurate calibration points, correctly rooted phylogenies, and accurate estimates of branch length remain formidable. Conversely, paleontological dates fix only the latest possible time of divergence, and so probabilistic methods are required to set a lower boundary on origination dates. Realistic confidence intervals that take preservational biases into account are only just becoming available. Although molecular and paleontological approaches to dating often agree reasonably well, there are two notable areas of disagreement; when mammal and bird orders originated and when the major phyla originated. The discrepancy in dating bird/mammal ordinal origins probably reflects a global rock-record bias. Paleontological sampling in the Late Cretaceous is still too restricted geographically to draw any firm conclusions about the existence of a pre-Tertiary record for modern orders of bird or mammal from anywhere other than North America. Dating the time of origin of phyla is more complicated, and is confounded by both preservational biases and problems of molecular clock estimation.
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    Annual Review of Earth and Planetary Sciences 30 (2002), S. 207-235 
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    Notes: Abstract The subducted lithosphere is composed of a complex pattern of chemical systems that undergo continuous and discontinuous phase transformation, through pressure and temperature variations. Volatile recycling plays a major geodynamic role in triggering mass transfer, melting, and volcanism. Although buoyancy forces are controlled by modal amounts of the most abundant phases, usually volatile-free, petrogenesis and chemical differentiation are controlled by the occurrence of minor phases, most of them volatile-bearing. Devolatilization of the subducted lithosphere is a continuous process distributed over more than 300 km of the slab-mantle interface. Melting of the subducted crust, if any, along sufficiently hot P-T paths, is governed by fluid-absent reactions, even though the difference between fluid and melt vanishes at pressures above the second critical end point. The density distribution at a depth of 660 km suggests episodic penetration in space and time of subducted slabs into the lower mantle and sinking down to the D" region at the core-mantle boundary.
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    Annual Review of Earth and Planetary Sciences 30 (2002), S. 307-345 
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    Notes: Abstract Pluto and Charon, once thought to be a singular system in an odd orbit at the edge of the solar system, are now known as members of a vast population of icy bodies beyond Neptune. Models for the occurrence of the odd orbit and formation of these bodies in the context of the total population are reviewed. Pluto's orbital characteristics, coupled with the existence of volatiles on the surface, suggest that large-scale seasonal change should occur on the surface. Models of seasonal variability are discussed, past and current observations are examined for evidence of variability, and a straw-man model of seasonal changes is proposed. Finally, recent observations of the surface composition of Charon are discussed and compared with observations of other similarly sized icy bodies in the outer Solar System.
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    Annual Review of Earth and Planetary Sciences 31 (2003), S. 555-577 
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    Notes: Abstract We present preliminary evidence for a ~10,000-year earthquake record from two major fault systems based on sediment cores collected along the continental margins of western North America. New stratigraphic evidence from Cascadia demonstrates that 13 earthquakes ruptured the entire margin from Vancouver Island to at least the California border since the eruption of the Mazama ash 7700 years ago. The 13 events above this prominent stratigraphic marker have an average repeat time of 600 years, and the youngest event ~300 years ago coincides with the coastal record. We also extend the record of past earthquakes to the base of the Holocene (at least 9800 years ago), during which 18 events correlate along the same region. The sequence of Holocene events in Cascadia appears to contain a repeating pattern of events, a tantalizing first look at what may be the long-term behavior of a major fault system. The northern California margin cores show a cyclic record of turbidite beds that may represent Holocene earthquakes on the northern segment of the San Andreas Fault. Preliminary results are in reasonably good agreement with onshore paleoseismic data that indicate an age for the penultimate event in the mid-1600s at several sites and the most likely age for the third event of ~AD 1300.
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    Annual Review of Earth and Planetary Sciences 32 (2004), S. 363-401 
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    Notes: The nation has over 40,000 metric tonnes (MT) of nuclear waste destined for disposal in a geologic repository at Yucca Mountain. In this review, we highlight some of the important geoscience issues associated with the project and place them in the context of the process by which a final decision on Yucca Mountain will be made. The issues include understanding how water could infiltrate the repository, corrode the canisters, dissolve the waste, and transport it to the biosphere during a 10,000-year compliance period in a region, the Basin and Range province, that is known for seismic and volcanic activity. Although the site is considered to be "dry," a considerable amount of water is present as pore waters and as structural water in zeolites. The geochemical environment is oxidizing, and the present repository design will maintain temperatures at greater than 100oC for thousands of years. Geoscientists in this project are challenged to make unprecedented predictions about coupled thermal, hydrologic, mechanical, and geochemical processes governing the future behavior of the repository and to conduct research in a regulatory and legal environment that requires a quantitative analysis of repository performance.
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    Annual Review of Earth and Planetary Sciences 32 (2004), S. 403-433 
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    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
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    Notes: The migration of the Mendocino triple junction through central and northern California over the past 25-30 million years has led to a profound change in plate interactions along coastal California. The tectonic consequences of the abrupt change from subduction plate interactions north of the triple junction to the development of the San Andreas transform system south of the triple junction can be seen in the geologic record and geophysical observations. The primary driver of this tectonism is a coupling among the subducting Juan de Fuca (Gorda), North American, and Pacific plates that migrates with the triple junction. This coupling leads to ephemeral thickening of the overlying North American crust, associated uplift and subsequent subsidence, and a distinctive sequence of fault development and volcanism.
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    Annual Review of Earth and Planetary Sciences 32 (2004), S. 151-185 
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    Notes: Bedrock rivers set much of the relief structure of active orogens and dictate rates and patterns of denudation. Quantitative understanding of the role of climate-driven denudation in the evolution of unglaciated orogens depends first and foremost on knowledge of fluvial erosion processes and the factors that control incision rate. The results of intense research in the past decade are reviewed here, with the aim of highlighting remaining unknowns and suggesting fruitful avenues for further research. This review considers in turn (a) the occurrence and morphology of bedrock channels and their relation to tectonic setting; (b) the physical processes of fluvial incision into rock; and (c) models of river incision, their implications, and the field and laboratory data needed to test, refine, and extend them.
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    Annual Review of Earth and Planetary Sciences 31 (2003), S. 399-427 
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    Notes: Abstract Considerable progress has been made over the past decade in understanding the static rheological properties of granitic magmas in the continental crust. Changes in H2O content, CO2 content, and oxidation state of the interstitial melt phase have been identified as important compositional factors governing the rheodynamic behavior of the solid/fluid mixture. Although the strengths of granitic magmas over the crystallization interval are still poorly constrained, theoretical investigations suggest that during magma ascent, yield strengths of the order of 9 kPa are required to completely retard the upward flow in meter-wide conduits. In low Bagnold number magma suspensions with moderate crystal contents (solidosities 0.1 〈=phi〈= 0.3), viscous fluctuations may lead to flow differentiation by shear-enhanced diffusion. AMS and microstructural studies support the idea that granite plutons are intruded as crystal-poor liquids (phi〈= 50%), with fabric and foliation development restricted to the final stages of emplacement. If so, then these fabrics contain no information on the ascent (vertical transport) history of the magma. Deformation of a magmatic mush during pluton emplacement can enhance significantly the pressure gradient in the melt, resulting in a range of local macroscopic flow structures, including layering, crystal alignment, and other mechanical instabilities such as shear zones. As the suspension viscosity varies with stress rate, it is not clear how the timing of proposed rheological transitions formulated from simple equations for static magma suspensions applies to mixtures undergoing shear. New theories of magmas as multiphase flows are required if the full complexity of granitic magma rheology is to be resolved.
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    Annual Review of Earth and Planetary Sciences 31 (2003), S. 579-594 
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    Notes: Abstract Is El Nino one phase of a continual, self-sustaining natural mode of the coupled ocean-atmosphere that has La Nina as the complementary phase? Or is El Nino a temporary departure from "normal" conditions "triggered" by a random disturbance such as a burst of westerly winds? A growing body of evidence-stability analyses, studies of the energetics, simulations that reproduce the statistics of sea surface temperature variations in the eastern equatorial Pacific-indicates that reality corresponds to a compromise between these two possibilities: The observed Southern Oscillation between El Nino and La Nina corresponds to a weakly damped mode that is sustained by random disturbances. This means that the predictability of El Nino is limited by the continual presence of "noise" so that forecasts should be probabilistic. The Southern Oscillation is also subject to decadal modulations. How it will be influenced by global warming is a matter of considerable uncertainty.
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    Annual Review of Earth and Planetary Sciences 32 (2004), S. 47-66 
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    Notes: Computer models are used to mimic the early evolution of ancient vascular plants (tracheophytes). These models have three components: (a) an N-dimensional domain of all mathematically conceivable ancient morphologies (a morphospace); (b) a numerical assessment of the ability (fitness) of each morphology to intercept light, maintain mechanical stability, conserve water, and produce and disperse spores; and (c) an algorithm that searches the morphospace for successively more fit variants (an adaptive walk). Beginning with the most ancient known plant form, evolution is simulated by locating neighboring morphologies that progressively perform one or more tasks more efficiently. The resulting simulated adaptive walks indicate that early tracheophyte evolution involved optimizing the performance of many tasks simultaneously rather than maximizing the performance of one or only a few tasks individually, and that the requirement for optimization accelerated the tempo of morphological evolution in the Silurian and Devonian.
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    Annual Review of Earth and Planetary Sciences 32 (2004), S. 465-494 
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    Notes: Models of processes in the alpine snow cover fundamentally depend on the spatial distribution of the surface energy balance over areas where topographic variability causes huge differences in the incoming solar radiation and in snow depth because of redistribution by wind. At a spatial scale commensurate with that of the terrain, we want to know which areas are covered by snow, and we want to estimate the snow's spectral albedo, along with other properties such as grain size, contaminants, temperature, liquid water content, and depth or water equivalent. From multispectral and hyperspectral remote sensing at wavelengths from 0.4-15 mum, the retrievable properties include snow-covered area, albedo, grain size, liquid water very near the surface, and temperature. Spectral mixture analysis allows the retrieval of the subpixel variability of snow-covered area, along with the snow's albedo. Remaining research challenges include the remote sensing of absorbing impurities; accounting for variability in the bidirectional-reflectance distribution function and the variability of grain size with depth; retrieving snow cover in forested regions; reconciling field measurements of emissivity with snow properties; and adapting the algorithms to frequent, large-scale processing.
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    Annual Review of Earth and Planetary Sciences 32 (2004), S. 601-652 
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    Notes: We examine the genetics of marine diversification along the West Coast of North America in relation to the Late Neogene geology and climate of the region. Trophically important components of the diverse West Coast fauna, including kelp, alcid birds (e.g., auks, puffins), salmon, rockfish, abalone, and Cancer crabs, appear to have radiated during peaks of upwelling primarily in the Late Miocene and in some cases secondarily in the Pleistocene. Phylogeographic barriers associated with Mio-Pliocene estuaries of the mid-California coast, the Pliocene opening of the Gulf of California, tectonic and eustatic evolution of the California Bight, as well as the influence of Pleistocene and Holocene climate change on genetic structure are assessed in a geologic context. Comparisons to East Coast and western freshwater systems, as well as upwelling systems around the globe, provide perspective for the survey.
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    Annual Review of Earth and Planetary Sciences 32 (2004), S. 215-255 
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    Notes: Measurements of cosmogenic nuclides, predominately 10Be, allow new insights into the ways in which and the rates at which sediment is generated, transported, and deposited over timescales ranging from 103 to 106 years. Samples from rock exposures are used to estimate erosion rates at points on the landscape, whereas samples of fluvial sediment provide estimates of basin-scale rates of denudation integrated over 〈1 to 〉104 km2. Nuclide data show that hilltop, bare rock outcrops erode more slowly than basins as a whole, suggesting the potential for relief to increase over time as well-drained outcrops grow higher. More elaborate experiments and interpretive models provide insight into the distribution of hillslope processes, including the bedrock-to-soil conversion rate, which appears to increase under shallow soil cover and then decrease under deeper soils. Changes in average nuclide activity down slopes can be used to estimate grain speed over millennia, suggesting, for example, that sediment on desert piedmonts moves, on average, decimeters to meters per year. In other cases, changes in nuclide activity down river networks or along shorelines can be interpreted with mixing models to indicate sediment sources. Sediment deposition rates in otherwise undateable deposits can now be estimated by analyzing samples collected from depth profiles. Over the past decade, the analysis and interpretation of cosmogenic nuclides has given geomorphologists an unprecedented opportunity to measure rates and infer the distribution of geomorphic processes across Earth's varied landscapes. Long-standing models of landscape change can now be tested quantitatively.
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    Annual Review of Earth and Planetary Sciences 32 (2004), S. 257-285 
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    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
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    Notes: Avulsion is the natural process by which flow diverts out of an established river channel into a new permanent course on the adjacent floodplain. Avulsions are primarily features of aggrading floodplains. Their recurrence interval varies widely among the few modern rivers for which such data exist, ranging from as low as 28 years for the Kosi River (India) to up to 1400 years for the Mississippi. Avulsions cause loss of life, property damage, destabilization of shipping and irrigation channels, and even coastal erosion as sediment is temporarily sequestered on the floodplain. They are also the main process that builds alluvial stratigraphy. Their causes remain relatively unknown, but stability analyses of bifurcating channels suggest that thresholds in the relative energy slope and Shields parameter of the bifurcating channel system are key factors.
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    Annual Review of Earth and Planetary Sciences 33 (2005), S. 605-643 
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    Notes: Various forms of atmospheric moist convection are reviewed through a consideration of three prevalent regimes: stratocumulus; trade-wind; and deep, precipitating, maritime convection. These regimes are chosen because they are structural components of the general circulation of the atmosphere and because they highlight distinguishing features of this polymorphous phenomenon. In particular, the ways in which varied forms of moist convection communicate with remote parts of the flow through mechanisms other than the rearrangement of fluid parcels are emphasized. These include radiative, gravity wave, and/or microphysical (precipitation) processes. For each regime, basic aspects of its phenomenology are presented along with theoretical frameworks that have arisen to help rationalize the phenomenology. Recent developments suggest that the increased capacity for numerical simulation and increasingly refined remote sensing capabilities bodes well for major advances in the coming years.
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    Annual Review of Earth and Planetary Sciences 3 (1975), S. 31-53 
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    Annual Review of Earth and Planetary Sciences 3 (1975), S. 79-98 
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    Annual Review of Earth and Planetary Sciences 3 (1975), S. 157-181 
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    Annual Review of Earth and Planetary Sciences 3 (1975), S. 361-385 
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    Annual Review of Earth and Planetary Sciences 33 (2005), S. 461-491 
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    Notes: Recent developments in volcanic seismology include new techniques to improve earthquake locations that have changed clouds of earthquakes to lines (faults) for high-frequency events and small volumes for low-frequency (LF) events. Spatial mapping of the b-value shows regions of normal b and high b anomalies at depths of 3-4 and 7-10 km. Increases in b precede some eruptions. LF events and very-long-period (VLP) events have been recorded at many volcanoes, and models are becoming increasingly sophisticated. Deep long-period (LP) events are fairly common, but may represent several processes. Acoustic sensors have greatly improved the study of volcanic explosions. Volcanic tremor is stronger for fissure eruptions, phreatic eruptions, and higher gas contents. Path and site effects can be extreme at volcanoes. Seismicity at volcanoes is triggered by large earthquakes, although mechanisms are still uncertain. A number of volcanoes have significant deformation with very little seismicity. Tomography has benefited from improved techniques and better instrumental arrays.
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    Annual Review of Earth and Planetary Sciences 33 (2005), S. 571-604 
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    Notes: Contrary to Earth, the interior of terrestrial planets is poorly known. This is mainly related to the lack of seismic data and of planetary seismic networks on these planets. So far, despite several attempts, only the Apollo Seismic Network has returned seismic information from the Moon. But even in this case, very few seismic signals were recorded after a propagation path through the deep interior and core owing to a hemispheric distribution of the stations on the near side and to a probably strongly attenuating lower mantle. This review presents the main results achieved by the analysis of the Apollo seismic data and the associated constraints on the internal structure of the Moon. It then presents the current knowledge on the Martian interior, the seismic activity of the planet, and possible source of seismic noise. This information can be used for preparing future Martian seismic network missions. A short review on existing space-qualified instruments and on possible seismic missions toward other telluric bodies, such as Venus, the giant planets' satellites, or small bodies, is then given.
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    Annual Review of Earth and Planetary Sciences 3 (1975), S. 55-77 
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    Annual Review of Earth and Planetary Sciences 3 (1975), S. 129-155 
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    Annual Review of Earth and Planetary Sciences 5 (1977), S. 357-369 
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    Annual Review of Earth and Planetary Sciences 6 (1978), S. 93-125 
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    Annual Review of Earth and Planetary Sciences 6 (1978), S. 325-351 
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    Annual Review of Earth and Planetary Sciences 33 (2005), S. 493-530 
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    Notes: We know that giant planets played a crucial role in the making of our Solar System. The discovery of giant planets orbiting other stars is a formidable opportunity to learn more about these objects, what their composition is, how various processes influence their structure and evolution, and most importantly how they form. Jupiter, Saturn, Uranus, and Neptune can be studied in detail, mostly from close spacecraft flybys. We can infer that they are all enriched in heavy elements compared to the Sun, with the relative global enrichments increasing with distance to the Sun. We can also infer that they possess dense cores of varied masses. The intercomparison of presently characterized extrasolar giant planets shows that they are also mainly made of hydrogen and helium, but that they either have significantly different amounts of heavy elements, have had different orbital evolutions, or both. Hence, many questions remain and need to be answered to make significant progress on the origins of planets.
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    Annual Review of Earth and Planetary Sciences 33 (2005), S. 645-671 
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    Notes: The influence of surface orography on patterns of precipitation gives rise to some of the most pronounced climate gradients on Earth, and plays a fundamental role in the interaction between the atmosphere and the rest of the Earth System on a wide variety of time scales. The physical mechanisms involved comprise a rich set of interactions encompassing fluid dynamics, thermodynamics, and micron-scale cloud processes, as well as being dependent on the larger-scale patterns of the atmospheric general circulation. Investigations into orographic precipitation have pursued three parallel tracks of inquiry: observations, theory, and modeling. Significant advances have been made in each over the last few decades, and these are summarized and synthesized here. While many aspects of the basic mechanisms responsible for orographic precipitation have been understood, important issues remain unresolved. The sheer number of contributing processes, together with their convoluted interactions, make the quantitative prediction of precipitation in complex terrain a very hard task. However, while prediction of precipitation amounts for any given event may be difficult, various lines of evidence suggest that the patterns of orgraphic precipitation, even on scales of a few kilometers, are much more robust.
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    Annual Review of Earth and Planetary Sciences 3 (1975), S. 317-342 
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    Annual Review of Earth and Planetary Sciences 3 (1975), S. 387-400 
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    Annual Review of Earth and Planetary Sciences 9 (1981), S. 59-80 
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    Annual Review of Earth and Planetary Sciences 4 (1976), S. 123-145 
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    Notes: The bulk of the Đ♯50-km-thick Martian crust formed at Đ♯4.5 Gyr B.P., perhaps from a magma ocean. This crust is probably a basaltic andesite or andesite and is enriched in incompatible and heat-producing elements. Later additions of denser basalt to the crust were volumetrically minor, but resurfaced significant portions of the Northern hemisphere. A significant fraction of the total thickness of the crust was magnetized prior to 4 Gyr B.P., with the magnetization later selectively removed by large impacts. Early large impacts also modified the hemispheric contrast in crustal thickness (the dichotomy), which was possibly caused by long-wavelength mantle convection. Subsequent Noachian modification of the crust included further impacts, significant fluvial erosion, and volcanism associated with the formation of the Tharsis rise. Remaining outstanding questions include the origin of the dichotomy and the nature of the magnetic anomalies.
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    Annual Review of Earth and Planetary Sciences 33 (2005), S. 247-276 
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    Notes: Processes operating beneath glaciers can have a greater influence on flow dynamics than those operating within them. The variety and complexity of these processes, which involve interactions among ice, water, and geological solids, resist efforts to establish simple truths and can lead to surprising outcomes. Thermal conditions at the ice-bed interface (melting or nonmelting) and the mechanical properties of the glacier substrate (soft or hard) determine which processes can be activated. The warm-soft case supports the greatest variety of processes and is the most important for fast-flow dynamics and for the mobilization of subglacial sediment. Process interactions can lead to oscillations and spatio-temporal switching behavior in glaciers and ice sheets as well as to the generation of subglacial landforms.
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    Notes: The Ediacara biota (575Đ??542 Ma) marks the first appearance of large, architecturally complex organisms in Earth history. Present evidence suggests that the Ediacara biota included a mixture of stem- and crown-group radial animals, stem-group bilaterian animals, "failed experiments" in animal evolution, and perhaps representatives of other eukaryotic kingdoms. These soft-bodied organisms were preserved under (or rarely within) event beds of sand or volcanic ash, and four distinct preservational styles (Flinders-, Fermeuse-, Conception-, and Nama-style) profoundly affected the types of organisms and features that could be preserved. Even the earliest Ediacaran communities (575Đ??565 Ma) show vertical and lateral niche subdivision of the sessile, benthic, filter-feeding organisms, which is strikingly like that of Phanerozoic and modern communities. Later biological and ecological innovations include mobility (〉555 Ma), calcification (550 Ma), and predation (〈549 Ma). The Ediacara biota abruptly disappeared 542 million years ago, probably as a consequence of mass extinction andor biological interactions with the rapidly evolving animals of the Cambrian explosion.
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    Annual Review of Earth and Planetary Sciences 33 (2005), S. 571-604 
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    Notes: Contrary to Earth, the interior of terrestrial planets is poorly known. This is mainly related to the lack of seismic data and of planetary seismic networks on these planets. So far, despite several attempts, only the Apollo Seismic Network has returned seismic information from the Moon. But even in this case, very few seismic signals were recorded after a propagation path through the deep interior and core owing to a hemispheric distribution of the stations on the near side and to a probably strongly attenuating lower mantle. This review presents the main results achieved by the analysis of the Apollo seismic data and the associated constraints on the internal structure of the Moon. It then presents the current knowledge on the Martian interior, the seismic activity of the planet, and possible source of seismic noise. This information can be used for preparing future Martian seismic network missions. A short review on existing space-qualified instruments and on possible seismic missions toward other telluric bodies, such as Venus, the giant planets' satellites, or small bodies, is then given.
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    Annual Review of Earth and Planetary Sciences 7 (1979), S. 357-384 
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    Annual Review of Earth and Planetary Sciences 7 (1979), S. 473-502 
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    Annual Review of Earth and Planetary Sciences 8 (1980), S. 65-93 
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    Annual Review of Earth and Planetary Sciences 8 (1980), S. 169-190 
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    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Geosciences , Physics
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 8 (1980), S. 205-230 
    ISSN: 0084-6597
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Geosciences , Physics
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 11 (1983), S. 415-457 
    ISSN: 0084-6597
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Geosciences , Physics
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 12 (1984), S. 133-153 
    ISSN: 0084-6597
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 12 (1984), S. 205-243 
    ISSN: 0084-6597
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 12 (1984), S. 337-357 
    ISSN: 0084-6597
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 12 (1984), S. 445-488 
    ISSN: 0084-6597
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 10 (1982), S. 327-353 
    ISSN: 0084-6597
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Geosciences , Physics
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 10 (1982), S. 409-440 
    ISSN: 0084-6597
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 11 (1983), S. 1-10 
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 11 (1983), S. 99-132 
    ISSN: 0084-6597
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 11 (1983), S. 215-240 
    ISSN: 0084-6597
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    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 11 (1983), S. 329-358 
    ISSN: 0084-6597
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Geosciences , Physics
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