严厉
发表于 2025-3-21 16:16:30
书目名称Solar System History from Isotopic Signatures of Volatile Elements影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0871435<br><br> <br><br>书目名称Solar System History from Isotopic Signatures of Volatile Elements影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0871435<br><br> <br><br>书目名称Solar System History from Isotopic Signatures of Volatile Elements网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0871435<br><br> <br><br>书目名称Solar System History from Isotopic Signatures of Volatile Elements网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0871435<br><br> <br><br>书目名称Solar System History from Isotopic Signatures of Volatile Elements被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0871435<br><br> <br><br>书目名称Solar System History from Isotopic Signatures of Volatile Elements被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0871435<br><br> <br><br>书目名称Solar System History from Isotopic Signatures of Volatile Elements年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0871435<br><br> <br><br>书目名称Solar System History from Isotopic Signatures of Volatile Elements年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0871435<br><br> <br><br>书目名称Solar System History from Isotopic Signatures of Volatile Elements读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0871435<br><br> <br><br>书目名称Solar System History from Isotopic Signatures of Volatile Elements读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0871435<br><br> <br><br>
分开
发表于 2025-3-21 22:31:02
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Immunotherapy
发表于 2025-3-22 00:52:00
Isotopes of Volatiles in Pre-Solar Grainslements (noble gases). Their isotopic corn-positions generally are unlike anything seen in matter of solar-system origin. The large variations are indicative of the various stellar sources and various processes of nucleosynthesis by which they were created.
一条卷发
发表于 2025-3-22 07:17:03
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战役
发表于 2025-3-22 11:02:34
Deuterium in Molecules of the Interstellar Mediumecent observational studies of deuterated molecules ranging from the VUV to the millimeter wavelength range. We outline some sources of uncertainties on the deuterium fractionation and on the subsequent derivation of the elemental deuterium to hydrogen ratio. Steady state versus time dependent model
AFFIX
发表于 2025-3-22 14:37:50
Deuterium Fractionation in Interstellar Clouds a low temperature phenomenon and discuss how the degree of enhancement of the deuterium content of molecules is related to the physical conditions, particularly abundances, in molecular clouds. If significant amounts of abundant species, such as CO, are frozen out on to interstellar dust grains, th
integrated
发表于 2025-3-22 19:45:32
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Organization
发表于 2025-3-23 00:46:11
Evolution of the Protosolar Nebula and Formation of the Giant Planetsls of evolution of circumstellar disks are reviewed here with emphasis on the so-called “alpha models” in which angular momentum is transported outward by turbulent viscosity, parameterized by an dimensionless parameter a. A simple ID model of protoplanetary disks that includes gas and embedded part
全等
发表于 2025-3-23 01:45:47
Element Abundances and Isotope Ratios in the Giant Planets and Titanion about the formation and evolution of these objects. Element abundances, especially after the results of the Galileo Probe Mass Spectrometer in Jupiter, strongly support the formation model invoking an initial core formation (Mizuno, 1980; Pollack .. 1996). They also suggest that solar compositio
千篇一律
发表于 2025-3-23 05:34:48
Isotopic Abundances in Comets Solar Nebula. We review here measurements acquired on the D/H, .C/.C, .O/.O, .N/.N, .S/.S ratios in dust and gases, and discuss their cosmogonic implications. The prospects for future measurements from cometary space missions and remote sensing observations at millimeter and submillimeter wavelengt