首页> 外文学位 >I. Temperatures of polar ice deposits on Mercury and the Moon. II. Jovian atmospheric dynamics from Galileo imaging.

【24h】

I. Temperatures of polar ice deposits on Mercury and the Moon. II. Jovian atmospheric dynamics from Galileo imaging.

机译：I.水星和月球上极地冰层的温度。二。来自伽利略成像的木星大气动力学。

获取原文

获取原文并翻译 | 示例

页面导航

摘要
著录项
相似文献
相关主题

摘要

Locations on Mercury that produce ice-like radar responses lie within impact craters that have very cold, permanently shaded floors. The retention of possible ice deposits is determined largely by their temperature. We present model-calculated temperatures of flat surfaces and surfaces within bowl-shaped and flat-floored polar impact craters. Our model includes appropriate insolation cycles, realistic crater shapes, multiple scattering of sunlight and infrared radiation, and depth and temperature-dependent regolith thermophysical properties. Meter-thick deposits of water ice are stable to evaporation over the age of the solar system if located in the permanently shaded portions of flat-floored craters within ;During the first six orbits of the Galileo spacecraft's prime mission, the Solid State Imaging system acquired multispectral image mosaics of Jupiter's Great Red Spot, an equatorial belt/zone boundary, a "5-

机译：水星上产生类似于冰的雷达响应的位置位于撞击坑内，撞击坑的地板非常冷且永久阴影。可能的冰沉积物的保留在很大程度上取决于其温度。我们介绍了模型计算得出的平坦表面以及碗形和平坦地板的极性撞击坑内表面的温度。我们的模型包括适当的日照周期，真实的陨石坑形状，日光和红外辐射的多次散射以及与深度和温度有关的重石热物理性质。如果将米厚的水冰沉积物放置在内部平底坑的永久阴影部分中，则在太阳系的整个年龄段内，其蒸发稳定；在伽利略号航天器主要任务的前六个轨道中，获得了固态成像系统木星大红色斑点，赤道带/区域边界，“ 5-

著录项

作者
Vasavada, Ashwin R.;
展开▼
作者单位

California Institute of Technology.;

展开▼
授予单位 California Institute of Technology.;
学科 Geology.;Physics Atmospheric Science.;Physics Astronomy and Astrophysics.
学位 Ph.D.
年度 1998
页码 103 p.
总页数 103
原文格式 PDF
正文语种 eng
中图分类
关键词

相似文献

外文文献
中文文献
专利

1. Jovian atmospheric dynamics: an update after Galileo and Cassini [J] . Vasavada AR, Showman AP Reports on Progress in Physics . 2005,第8期

机译：木星大气动力学：伽利略和卡西尼之后的更新
2. Comparison of areas in shadow from imaging and altimetry in the north polar region of Mercury and implications for polar ice deposits [J] . Deutsch Ariel N., Chabot Nancy L., Mazarico Erwan, Icarus: International Journal of Solar System Studies . 2016,第Null期

机译：水星北极地区成像和测高仪阴影区域的比较及其对极地冰沉积的影响
3. Constraining the thickness of polar ice deposits on Mercury using the Mercury Laser Altimeter and small craters in permanently shadowed regions [J] . Deutsch Ariel N., Head James W., Chabot Nancy L., Icarus: International Journal of Solar System Studies . 2018,第期

机译：利用汞激光高温仪和永久阴影区域使用汞激光高度计和小陨石坑的极地冰沉积物厚度
4. ATMOSPHERIC DYNAMICS OF THE JOVIAN LIKE PLANETS EPSILON ERIDANI b AND 55 CANCRI d [C] . A. Sanchez-Lavega, R. Hueso, S. Baeza Conference on Towards Other Earths DARWIN/TPF and the Search for Extrasolar Terrestrial Planets; 20030422-20030425; Heidelberg; DE . 2003

机译：类似于埃文斯通ERIDANI B和55 CANCRI d的大气动力学
5. Some aspects of the Martian climate in the Mars Orbiter Laser Altimeter (MOLA) investigation. Part I. Evolution of the polar residual ice caps. Part II. Polar night clouds. Part III. Interpretation of the MOLA reflectivity measurement in terms of the surface albedo and atmospheric opacity. [D] . Ivanov, Anton Borisovich. 2002

机译：火星轨道激光高度计（MOLA）研究中的火星气候某些方面。第一部分。极地残余冰盖的演变。第二部分极夜云。第三部分用表面反照率和大气不透明度解释MOLA反射率的测量结果。
6. Comparison of areas in shadow from imaging and altimetry in the north polar region of Mercury and implications for polar ice deposits [O] . Ariel N. Deutsch, Nancy L. Chabot, Erwan Mazarico, -1

机译：水星北极地区成像和测高仪阴影区域的比较及其对极地冰沉积的影响
7. Comparison of areas in shadow from imaging and altimetry in the north polar region of Mercury and implications for polar ice deposits [O] . Ariel N. Deutsch, Nancy L. Chabot, Erwan Mazarico, 2016

机译：北极汞北极地区成像和高度测量的阴影区域的比较及极冰沉积物的影响

I. Temperatures of polar ice deposits on Mercury and the Moon. II. Jovian atmospheric dynamics from Galileo imaging.

摘要

著录项

相似文献

相关主题

期刊订阅