ALBERT

All Library Books, journals and Electronic Records Telegrafenberg

X
feed icon rss

Your email was sent successfully. Check your inbox.

An error occurred while sending the email. Please try again.

Proceed reservation?

Export
  • 1
    Unknown
    Primitive solar nebula and origin of planets (1993)
    Tokyo : TERRAPUB
    Details
    Keywords: primitive solar nebula ; origin of planets ; giant planets ; terrestrial planets ; origin of meteorites ; origin and evolution of the terrestrial atmosphere ; exploration of the solar system ; Halley Mission
    Description / Table of Contents: Chapter 1. Primitive Solar Nebula --- Evolution of Magnetized Dense Clouds / T. Nakano, T. Nakamura, T. Terasawa, and Y. Sano / pp. 1-28 --- Molecular Outflows—Observational Signature for the Earliest Phase of Stellar Evolution— / Y. Fukui, A. Mizuno, H. Ogawa, and K. Kawabata / pp. 29-45 --- Observational Evidence of Transition between Protostellar Objects and T Tauri Stars / S. Sato / pp. 47-57 --- Jet Formation and Enhanced Accretion due to Magnetic Effects in Protostellar Objects / Y. Uchida / pp. 59-77 --- Shear Instability of the Solar Nebula / M. Sekiya, S. M. Miyama, and Y. Nakagawa / pp. 79-88 --- Magnetic Fossil of the Solar Nebula Observed in Meteorites / T. Nagata / pp. 89-103 --- Experimental Demonstration of Formations of Tetrataenite and Pyrrhotite / C. Kaito and Y. Saito / pp. 105-112 --- Synthesis of Carbonaceous and Siliceous Materials / A. Sakata and S. Wada / pp. 113-127 --- Chapter 2. Origin of Giant Planets --- Scenario of Formation Processes of the Giant Planets / H. Oya / pp. 129-134 --- Giant Planetary Systems—A Review— / H. Oya / pp. 135-193 --- Accumulation of Materials for the Formation of the Giant Planets—Ring Model under the Flow-out Motion of Disc Gas— / H. Oya / pp. 195-220 --- Nonlinear Evolution of the Accumulation Processes of the Material for Formation of the Giant Planets in the Primeval Solar System / H. Oya and M. Iizima / pp. 221-240 --- Simulation Studies on the Formation Processes of the Saturnian Ringlets / H. Oya, M. Miyauchi, T. Imai, and M. Iizima / pp. 241-164 --- Chapter 3. Origin of the Terrestrial Planets --- Elementary Processes in Planetary Accretion / K. Nakazawa, S. Ida, and K. Ohtsuki / pp. 265-280 --- Experimental Simulation of Collisions / A. Fujiwara, A. Nakamura, M. Kato, and Y. Takagi / pp. 281-295 --- Scaling Law on Impact Phenomena / H. Mizutani / pp. 297-317 --- Numerical Simulation of Planetary Growth / M. Hayakawa and H. Mizutani / pp. 319-340 --- Deformation of Porous Ice-Rock Mixtures and an Application to the Densification of Icy Satellites / N. Maeno, M. Arakawa, and J. Leliwa-Kopystynski / pp. 341-353 --- Chapter 4. Origin of Meteorites --- Precise Determination of the Age of Formation of Meteorites / K. Takahashi and A. Masuda / pp. 355-373 --- Chemical Differentiation during Collision and Accretion of Meteorite Parent Bodies / H. Takeda / pp. 375-394 --- Isotope Variations of Light Elements in Chondrites—Ion Microprobe Studies— / C. Uyeda, H. Nishimura, and J. Okano / pp. 395-408 --- Trace Element Fractionation during the Formation of Chondrules / N. Nakamura / pp. 409-425 --- Vaporization and Condensation of Chondritic Materials—Experimental Studies— / H. Nagahara, 1. Kushiro, and B. O. Mysen / pp. 427-446 --- Metamorphic Processes in New CI Carbonaceous Chondrites from Antarctica: Mineralogy and Petrology / K. Tomeoka / pp. 447-464 --- Evolution and Alteration Process of the CM Carbonaceous Chondrites / H. Kojima and K. Yanai / pp. 465-477 --- Structure and Chemistry of Carbon in Meteorites / T. Murae, H. Kagi, and A. Masuda / pp. 479-501 --- Chapter 5. Origin and Evolution of the Terrestrial Atmosphere --- 244Pu Fission Xe in the Mantle and Mantle Degassing Chronology / M. Ozima, S. Azuma, S. Zashu, and H. Hiyagon / pp. 503-517 --- The Noble Gases in the Venusian Atmosphere and the Fukutomi Chondrite / N. Takaoka / pp. 519-526 --- Formation of Atmospheres of Terrestrial Planets from Volatiles in Solid (Meteoritelike) Material / N. Sugiura / pp. 527-543 --- Early Evolution of the Terrestrial Planets: Accretion, Atmosphere Formation, and Thermal History / T. Matsui / pp. 545-559 --- Existence of Life and Creation of Atmospheric Environment / S. Moriyama / pp. 561-577 --- Chapter 6. Exploration of the Solar System—Halley Mission— --- Interaction of Plasma of Halley's Comet with the Solar Wind / H. Oya / pp. 579-614 --- Plasma Environment of Comet Hally Observed by Suisei / T. Terasawa and S. Takahashi / pp. 615-628 --- Modelling Study of the Cometary Ly α Brightness from a Time-varying H2O Source / O. Ashihara / pp. 629-643 --- Cometary Dust / T. Mukai / pp. 645-662 --- The Origin of Comets as Viewed from the Gaseous Composition / T. Yamamoto / pp. 663-677
    Pages: Online-Ressource (VII, 677 Seiten)
    ISBN: 4887041101
    URL: http://www.terrapub.co.jp/e-library/psnop/
    Language: English
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
    E-BOOK
  • 2
    Electronic Resource
    Electronic Resource
    The Escherichia coli cytochrome b556 gene, cybA, is assignable as sdhC in the succinate dehydrogenase gene cluster (1985)
    Oxford, UK : Blackwell Publishing Ltd
    FEMS microbiology letters 30 (1985), S. 0 
    Details
    ISSN: 1574-6968
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Biology
    Notes: Abstract The cytochrome b556-deficient mutant Escherichia coli K12 strain TK3D11 [7] could not grow with succinate as the sole carbon source, but could grow well on dl-lactate. This finding suggested that cytochrome b556 is primarily responsible for oxidative metabolism and utilization of succinate. 24 Amino acid residues at the amino-terminal of purified cytochrome b556 were determined. This sequence coincided completely with amino acid residues 4 to 27, predicted from the DNA sequence of the sdhC gene, one of the unassigned open reading frames of the sdh gene cluster recently reported by Wood et al. [16]. Based on these and other results, we concluded that cybA, the gene for cytochrome b556, is assignable as sdhC.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1111/j.1574-6968.1985.tb01101.x
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
    Paper (German National Licenses)
    Fulltext
  • 3
    Electronic Resource
    Electronic Resource
    Discovery of cometary kilometric radiations and plasma waves at comet Halley (1986)
    [s.l.] : Nature Publishing Group
    Nature 321 (1986), S. 307-310 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] The plasma-wave probe (PWP) system carried by the Sakigake spacecraft used two detectors: a 10-m tip-to-tip dipole antenna and a search coil-type magnetic field detector. The receivers of the PWP system comprised a swept frequency receiver and a 16-channel frequency analyser, referred to as the ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/321307a0
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
    Paper (German National Licenses)
    Fulltext
  • 4
    Electronic Resource
    Electronic Resource
    X-ray observation of the Jovian impacts of comet Shoemaker - Levy 9 (1994)
    Springer
    Earth, moon and planets 66 (1994), S. 75-81 
    Details
    ISSN: 1573-0794
    Keywords: Comet ; Jupiter ; X-Ray
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract An ASCA observation of the Jovian impact of the comet Shoemaker-Levy 9 is reported. Four impacts of H, L, Q1 and R were observed and four impacts of B, C, G, and Q2 were observed within 60 minutes after their impacts. No significant flaring of X-ray emission was observed. Upper limit X-ray fluxes of 90 % confidence level, averaged 5 minutes just after the impacts, were 2.4 × 10−13 erg sec−1 cm−2, 3.5 × 10−13 erg sec−1 cm−2, 1.6 × 10−13 erg sec−1 cm−2 and 2.9 × 10−13 erg sec−1 cm−2 for the impacts of H, L, Q1 and R, respectively, in the 0.5(0.7 for H and Q1)−10 keV energy range. However, a hint of X-ray enhancement around Jupiter from July 17 to July 19 was detected with about 2 ∼ 6 × 10−14 erg sec−1 cm−2 in the 0.5–10 keV energy range.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00612887
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
    Paper (German National Licenses)
    Fulltext
  • 5
    Electronic Resource
    Electronic Resource
    Analyses Of Jovian Decametric Radiation -Bursts Interacting With N-Bursts (2000)
    Springer
    Earth, moon and planets 88 (2000), S. 187-209 
    Details
    ISSN: 1573-0794
    Keywords: DAM ; Jupiter ; N-burst ; S-burst ; Tilted-V
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract Dynamic spectra of S-bursts of Jovian decametric radiations are obtained by using a high time resolution radio spectrograph which has a time resolutionof 2 msec and the bandwidth of 2 MHz.Within occurrence of 65 S-burst events observed in the period from 1983 to 1999, 26 events have been identified as the S-N burst events, which are characterized by the interaction between the S-burst emissions and the Narrow band emissions. In the dynamic spectra of the S-N burst, the trend of emissions with negative and slower frequency drift named as “Trailing Edge Emission” are often observed shortly after the appearance of the S-burst.Detailed analyses of these phenomena revealed that the Trailing Edge Emission is not a manifestation of S-burst with slower drift rate but a variation ofN-burst. The results suggested that S-burst and the associated Trailing Edge Emission are formed simultaneously started from a common region with different drift rates. It has been further suggested that the appearance of the S-burstsis not controlled by the geometrical effect between the source region and theobserver, but directly reflects the generation of the source region widelydistributed in an altitude range from a few thousands km to 30,000 km, alongthe Io flux tube.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1023/A:1019836016325
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
    Paper (German National Licenses)
    Fulltext
  • 6
    Electronic Resource
    Electronic Resource
    Chromosomal location of the Escherichia coli cytochrome b556 gene, cybA (1984)
    Springer
    Molecular genetics and genomics 196 (1984), S. 1-5 
    Details
    ISSN: 1617-4623
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology
    Notes: Summary The amounts of cytochrome b556 in the cytoplasmic membranes of several Escherichia coli K12 strains having F-prime factors and a lambda transducing phage were determined. The amount was amplified about two-fold in strains having F100-12 and F152, but not in strains having F100-11, F8 and λpsu + 2glnS +. The strain TK3D11, which lacks the kdp-gltA region (deletion D-01) of the E. coli chromosome, did not synthesize cytochrome b556 at all. From these results, the gene cybA encoding cytochrome b556 was located in the kdp-gltA region. In the cytochrome b556-deficient mutant, a novel b type cytochrome, cytochrome b561 which is a product of the gene cybB, was identified. It seems to function as a physiological electron transferring cytochrome in place of cytochrome b556 in this mutant.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00334084
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
    Paper (German National Licenses)
    Fulltext
  • 7
    Electronic Resource
    Electronic Resource
    The course ofAngiostrongylus cantonensis infection in athymic nude and neonatally thymectomized mice (1982)
    Springer
    Parasitology research 67 (1982), S. 217-226 
    Details
    ISSN: 1432-1955
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology , Medicine
    Notes: Abstract BALB/c athymic nude and thymus-reconstituted nude mice and neonatally thymectomized BALB/c mice were infected with stage 3 larvae ofAngiostrongylus cantonensis and the worm burdens of the mice were determined at various times after infection. When the nude and thymectomized mice were exposed to the parasite, some worms were found to migrate from the brain to lungs but died there without reaching maturity. This pulmonary arterial migration of the worms in the nude mice did not occur following thymic reconstitution. These data suggest that the inability of murine intracranial worms to migrate to the lungs is at least in part due to thymus-dependent mechanisms, and also that the failure of worm maturation in mouse lungs might be due to thymus-independent immune mechanisms and/or nonimmunological mechanisms.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00928117
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
    Paper (German National Licenses)
    Fulltext
  • 8
    facet.materialart.
    Unknown
    X-ray observation of the Jovian impacts of comet Shoemaker - Levy 9 (1994)
    Springer
    Details
    Publication Date: 1994-01-01
    Print ISSN: 0167-9295
    Electronic ISSN: 1573-0794
    Topics: Geosciences , Physics
    Published by Springer
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
    PAPER CURRENT
  • 9
    facet.materialart.
    Unknown
    Ionospheric plasma disturbances due to a moving space vehicle (1970)
    Elsevier
    Details
    Publication Date: 1970-06-01
    Print ISSN: 0032-0633
    Electronic ISSN: 1873-5088
    Topics: Geosciences , Physics
    Published by Elsevier
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
    PAPER CURRENT
  • 10
    facet.materialart.
    Unknown
    Relations between turbulent regions of interplanetary magnetic field and Jovian decametric radio wave emissions from the main source (1981)
    Elsevier
    Details
    Publication Date: 1981-07-01
    Print ISSN: 0032-0633
    Electronic ISSN: 1873-5088
    Topics: Geosciences , Physics
    Published by Elsevier
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
    PAPER CURRENT
Close ⊗
This website uses cookies and the analysis tool Matomo. More information can be found here...