SMESE (SMall Explorer for Solar Eruptions):: A microsatellite mission with combined solar payload

被引：14

作者：

Vial, J. -C. ^{[1
]}

Auchere, F. ^{[1
]}

Chang, J. ^{[2
]}

Fang, C. ^{[3
]}

Gan, W. Q. ^{[2
]}

Klein, K. -L. ^{[4
]}

Prado, J. -Y. ^{[5
]}

Rouesnel, F. ^{[1
]}

Semery, A. ^{[4
]}

Trottet, G. ^{[4
]}

Wang, C. ^{[6
]}

机构：

[1] Univ Paris 11, CNRS, Inst Astrophys Spatiale, F-91405 Orsay, France

[2] Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China

[3] Nanjing Univ, Dept Astron, Nanjing 210093, Peoples R China

[4] Observ Paris, LESIA, F-92195 Meudon, France

[5] CNES, F-31055 Toulouse 4, France

[6] Chinese Acad Sci, Ctr Space Sci & Appl Res, Beijing 100080, Peoples R China

来源：

ADVANCES IN SPACE RESEARCH | 2008年 / 41卷 / 01期

关键词：

small satellite mission; solar flares; coronal mass ejections; UV; far infrared; X-rays; gamma-rays;

D O I：

10.1016/j.asr.2007.07.007

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

The SMESE (SMall Explorer for Solar Eruptions) mission is a microsatellite proposed by France and China. The payload of SMESE consists of three packages: LYOT (a Lyman alpha imager and a Lyman alpha coronagraph), DESIR (an Infra-red Telescope working at 35-80 and 100-250 mu m), and HEBS (a High Energy Burst Spectrometer working in X- and gamma-rays). The scientific objectives of the mission are shortly presented. We describe the three instrumental packages and the profile of the mission which accommodates them. With a launch around 2012-2013, the SMESE microsatellite mission will provide a unique tool for detecting and understanding eruptions (flares and coronal mass ejections). Observations should start around solar maximum, and continue in the declining phase of activity, at a time when the Solar Dynamics Observatory (SDO) should still be operating. (C) 2007 Published by Elsevier Ltd on behalf of COSPAR.

引用

页码：183 / 189

页数：7

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