找回密码
 To register

QQ登录

只需一步,快速开始

扫一扫,访问微社区

Titlebook: Atmospheres and Ionospheres of the Outer Planets and Their Satellites; Sushil K. Atreya Book 1986 Springer-Verlag Berlin Heidelberg 1986 c

[复制链接]
楼主: minuscule
发表于 2025-3-23 10:58:44 | 显示全部楼层
发表于 2025-3-23 14:52:20 | 显示全部楼层
Vertical Mixing,re . is the number density of the constituent, and . and . are respectively its molecular and eddy diffusion velocities. The latter can be expressed in terms of the density and thermal gradients (Colegrove et al. 1966), so that..
发表于 2025-3-23 20:25:56 | 显示全部楼层
Candida: A Disease of Antibiotics,ce and nature of the other clouds are at this time simply postulated on theoretical grounds. Preliminary numerical simulation of the cloud structure on the major planets was done by Weidenschilling and Lewis (1973), whereas the results of the most recent calculations have been published by Atreya and Romani (1985).
发表于 2025-3-24 00:47:52 | 显示全部楼层
Cloud Structure,ce and nature of the other clouds are at this time simply postulated on theoretical grounds. Preliminary numerical simulation of the cloud structure on the major planets was done by Weidenschilling and Lewis (1973), whereas the results of the most recent calculations have been published by Atreya and Romani (1985).
发表于 2025-3-24 03:10:59 | 显示全部楼层
Book 1986scovery was significant not only in the context of Jupiter; it gave credence to and was instrumental in firmly establishing the heliocentric system of Nicolaus Copernicus. Almost four centuries after Galileo‘s discovery, exten­ sive observations by the two Voyager spacecrafts have once again revolu­
发表于 2025-3-24 08:02:24 | 显示全部楼层
发表于 2025-3-24 10:59:09 | 显示全部楼层
Thermal Structure,s of basic planetary temperatures and radiative transfer are developed first, followed by principles of the most commonly used techniques for temperature determination on the major planets. Since considerably more information is presently available for Jupiter and Saturn, their results are treated s
发表于 2025-3-24 17:55:48 | 显示全部楼层
Cloud Structure,ered cloud structure. On Jupiter, for example, the predicted clouds in the region of the Galileo/Probe descent are ammonia ice (NH.-ice), ammonium hydrosulfide crystals (NH.SH-s), and water-ice (H.0-ice) as illustrated in Fig. 1.5. On Uranus and Neptune, clouds of methane ice (CH.-ice) and aqueous a
发表于 2025-3-24 22:53:39 | 显示全部楼层
发表于 2025-3-25 03:08:01 | 显示全部楼层
 关于派博传思  派博传思旗下网站  友情链接
派博传思介绍 公司地理位置 论文服务流程 影响因子官网 SITEMAP 大讲堂 北京大学 Oxford Uni. Harvard Uni.
发展历史沿革 期刊点评 投稿经验总结 SCIENCEGARD IMPACTFACTOR 派博系数 清华大学 Yale Uni. Stanford Uni.
|Archiver|手机版|小黑屋| 派博传思国际 ( 京公网安备110108008328) GMT+8, 2025-5-19 11:41
Copyright © 2001-2015 派博传思   京公网安备110108008328 版权所有 All rights reserved
快速回复 返回顶部 返回列表