Future Mission Concepts for Helioseismology

被引：4
|
作者：
Sekii, Takashi [1 ]
Appourchaux, Thierry [2 ]
Fleck, Bernhard [3 ]
Turck-Chieze, Sylvaine [4 ]
机构：
[1] NAOJ, Div Solar & Plasma Astrophys, Mitaka, Tokyo 1818588, Japan
[2] Univ Paris 11, Inst Astrophys Spatiale, CNRS UMR8617, Orsay, France
[3] NASA, ESA Sci Operat Dept, GSFC, Greenbelt, MD 20771 USA
[4] CEA DSM IRFU, CE Saclay, F-91191 Gif Sur Yvette, France
来源：
SPACE SCIENCE REVIEWS | 2015年 / 196卷 / 1-4期
关键词：
Sun; Helioseismology; Space missions; SOLAR OSCILLATIONS; FLOWS BENEATH; SOHO MISSION; DYNAMICS; SUN; FREQUENCY; ROTATION; REGIONS; SUNSPOT; MODES;
D O I：
10.1007/s11214-015-0142-2
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Future space-mission concepts currently discussed in the helioseismology community are reviewed. One popular idea is to observe the Sun from high latitudes, to explore the polar regions as well as to probe the deep interior using stereoscopic techniques, by combining observations from high latitudes with observations from within the ecliptic plane. Another idea is to stay within the ecliptic plane but still aim for stereoscopic helioseismology for deep layers. A new instrument and a novel mission concept for studying the solar core regions are also discussed.
引用
收藏
页码：285 / 302
页数：18
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