Titlebook: Cometary Science after Hale-Bopp; Volume 1 Proceedings H. Boehnhardt,M. Combi,R. Schulz Conference proceedings 2003 Springer Science+Busine

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书目名称Cometary Science after Hale-Bopp影响因子(影响力)




书目名称Cometary Science after Hale-Bopp影响因子(影响力)学科排名




书目名称Cometary Science after Hale-Bopp网络公开度




书目名称Cometary Science after Hale-Bopp网络公开度学科排名




书目名称Cometary Science after Hale-Bopp被引频次




书目名称Cometary Science after Hale-Bopp被引频次学科排名




书目名称Cometary Science after Hale-Bopp年度引用




书目名称Cometary Science after Hale-Bopp年度引用学科排名




书目名称Cometary Science after Hale-Bopp读者反馈




书目名称Cometary Science after Hale-Bopp读者反馈学科排名

卡死偷电

Modeling the Comet Nucleus Interior,ious mathematical procedures and approximations are discussed, and different attempts to model the physical characteristics of cometary material, such as thermal conductivity, or permeability to gas flow, are described. The evolution and activity of comets is shown to depend on different classes of

dry-eye

incontinence

Hale-Bopp: What Makes a Big Comet Different? Coma Dynamics: Observations and Theory,omet both the chemical and dynamical influences of collisional processes are limited by the short time a parcel of gas sublimated from the nucleus remains in the dense part of the coma. The resulting large size of the collisional coma in comet Hale—Bopp had important consequences on the dynamics of

贪婪地吃

,Comet Splitting — Observations and Model Scenarios,eparation of major fragments (e.g., 73P/Schwassmann—Wachmann 3) and spill-offs of smaller boulders (e.g., C/2001 A2 LINEAR). Fragmentation of comets produces secondary products over a wide range of sizes (from cometesimals to sub-micron dust). It is detectable through the presence of fragments (with

Estrogen

Observational Constraints on Surface Characteristics of Comet Nuclei, and yielding new information on cometary surfaces. In this review, we focus on recent determinations of the albedos, reflectances, and thermal inertias of comet nuclei. There is not much diversity in the geometric albedo of the comet nuclei observed so far (a range of 0.025 to 0.06). There is a gre

Estrogen

广大

闹剧

Composition of Comets: Observations and Models,ent bright comets including Hale–Bopp (C/1995 O1) and Hyakutake (C/1996 B2), in light of the elemental abundances of the solar system. Nitrogen is underabundant in comets relative to the solar system because nitrogen tends to be in N., which is chemically relatively inert. While many details remain

EVEN