开启辅助访问 购买速递币 快速注册 找回密码 切换风格

科研速递论坛

287

主题

1

好友

21

积分

炉火纯青

Rank: 4

科研币
89
速递币
1530
娱乐币
4077
文献值
340
资源值
0
贡献值
1
跳转到指定楼层
楼主
发表于 2013-10-25 21:05:29 |只看该作者 |倒序浏览
速递书局
封面: -
题名: Solar Variability and Its Effect on Climate (Geophysical Monograph Series)
作者: Judit M. Pap (Editor), Peter Fox (Editor), Claus Frohlich (Editor), Hugh S. Hudson (Editor), Jeffrey Kuhn (Editor), John McCormack (Editor), Gerald R. North (Editor), William Sprigg (Editor), S. T. Wu (Editor)
出版社: American Geophysical Union
出版日期: January 9, 2004
ISBN: 978-0875904061
附属页: 齐全
书签:
格式: 图版PDF
内容简介: -
求助帖链接: -


ublished by the American Geophysical Union as part of the Geophysical Monograph Series, Volume 141.

This monograph presents a state-of-the-art description of the most recent results on solar variability and its possible influence on the Earth's climate and atmosphere. Our primary goal in doing so is to review solar energy flux variations (both electromagnetic and particle) and understand their relations to solar magnetic field changes and global effects, their impact on different atmospheric layers, and—as a collaboration of scientists working on solar-terrestrial physics—to note unresolved questions on an important interdisciplinary area.

One of the highest-level questions facing science today is whether the Earth's atmosphere and climate system changes in a way that we can understand and predict. The Earth's climate is the result of a complex and incompletely understood system of external inputs and interacting parts. Climate change can occur on various time scales as a consequence of natural variability—including solar variability—or anthropogenic causes, or both. The Sun's variability in the form of sunspots and related magnetic activity has been the subject of careful study ever since the earliest telescopic observations. High precision photometric observations of solar-type stars clearly show that year-to-year brightness variations connected with magnetic activity are a widespread phenomenon among such stars. As our nearest star, the Sun is the only star where we can observe and identify a variety of structures and processes which lead to variations in the solar energy output, in both radiative and particle fluxes. Studying event tiny changes in solar energy flux variations may teach us about internal processes taking place in the Sun's convective zone and below.

本帖子中包含更多资源

您需要 登录 才可以下载或查看,没有帐号?快速注册

已有 1 人评分速递币 文献值 收起 理由
科研虫虫 + 50 + 2

总评分: 速递币 + 50  文献值 + 2   查看全部评分

您需要登录后才可以回帖 登录 | 快速注册

发布主题 !fastreply! 返回列表 官方QQ群

QQ|Translate Forum into English|QQ群:821993|Archiver|手机版|申请友链| 科研速递论坛

GMT+8, 2024-11-1 23:29 , Processed in 0.059610 second(s), 30 queries .

© 2012-2099 www.expaper.cn

!fastreply! 回顶部 !return_list!