Martian Top of the Atmosphere 10-420 </ce:hsp>nm spectral irradiance database and forecast for solar cycle 24

网站地图 | English | 公务邮箱

About the library

Background
History
Leadership
Organization

Opening Hours
Collections
Help Via Email

Electronic Information Resources

Martian Top of the Atmosphere 10-420 sp>nm spectral irradiance database and forecast for solar cycle 24

详细信息查看全文

作者：Alfonso Delgado-Bonal<sup>asup><sup> ; sup><sup>bsup><sup> ; sup><sup>alfonso.delgado-bonal@ltu.se" class="auth_mail" title="E-mail the corresponding authorsup> ; Marí ; a-Paz Zorzano<sup>bsup><sup> ; sup><sup>csup> ; F. Javier Martí ; n-Torres<sup>asup><sup> ; sup><sup>bsup>
关键词：Mars TOA ; UV radiation ; REMS ; Space exploration
刊名：Solar Energy
出版年：2016
出版时间：September 2016
年：2016
卷：134
期：Complete
页码：228-235
全文大小：653 K

文摘

ss="label">•: We have modeled the radiation reaching Mars Top of the Atmosphere in the range 10–420 nm for solar cycle 24.
ss="label">•: We use data and models to provide a database from 2003 to 2013.
ss="label">•: We have generated a radiation database forecast from 2013 to 2019.
ss="label">•: Using our database, we are able to estimate the dust content in the atmosphere.
ss="label">•: 225">Dedicated values for landing sites of upcoming missions to Mars are given.

NGLC 2004-2010.National Geological Library of China All Rights Reserved.
Add:29 Xueyuan Rd,Haidian District,Beijing,PRC. Mail Add: 8324 mailbox 100083
For exchange or info please contact us via email.