The Solar Orbiter Mission and its Polarimetric and Helioseismic Imager (SO/PHI)

被引：29

作者：

Gandorfer, Achim ^{[1
]}

Solanki, Sami K. ^{[1
]}

Woch, Joachim ^{[1
]}

Pillet, Valentin Martinez ^{[2
,3
]}

Herrero, Alberto Alvarez ^{[3
]}

Appourchaux, Thierry ^{[4
]}

机构：

[1] Max Planck Inst Sonnensyst Forsch, Max Planck Str 2, D-37191 Katlenburg Lindau, Germany

[2] Inst Astrofis Canarias, E-38205 San Cristobal la Laguna, Tenerife, Spain

[3] Inst Nacl Tecn Aeroespacial, E-28850 Madrid, Spain

[4] Univ Paris XI, Inst Astrophys Spatiale, CNRS, UMR8617, F-91405 Orsay, France

来源：

GONG-SOHO 24: A NEW ERA OF SEISMOLOGY OF THE SUN AND SOLAR-LIKE STARS | 2011年 / 271卷

关键词：

D O I：

10.1088/1742-6596/271/1/012086

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We briefly outline the scientific and instrumental aspects of ESA's Solar Orbiter mission. Special emphasis is given to the Polarimetric and Helioseismic Imager, the instrument with the highest relevance for helioseismology applications, which will observe gas motions and the vector magnetic field in the photosphere at high spatial and temporal resolution.

引用

页数：8