Solar Orbiter Exploring the Sun-Heliosphere Connection

被引：385

作者：

Muller, D. ^{[1
]}

Marsden, R. G. ^{[1
]}

St Cyr, O. C. ^{[2
]}

Gilbert, H. R. ^{[2
]}

机构：

[1] European Space Agcy, Estec, NL-2200 AG Noordwijk, Netherlands

[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

来源：

SOLAR PHYSICS | 2013年 / 285卷 / 1-2期

关键词：

Sun; Heliosphere; Corona; Dynamics; Magnetic fields; CORONAL MASS EJECTIONS; MAGNETIC-FIELDS; TEMPERATURE ANISOTROPY; PARTICLE-ACCELERATION; ENERGETIC PARTICLES; TRANSITION REGION; FLUX EMERGENCE; SHOCK-WAVES; WIND; MISSION;

D O I：

10.1007/s11207-012-0085-7

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The heliosphere represents a uniquely accessible domain of space, where fundamental physical processes common to solar, astrophysical and laboratory plasmas can be studied under conditions impossible to reproduce on Earth and unfeasible to observe from astronomical distances. Solar Orbiter, the first mission of ESA's Cosmic Vision 2015 -aEuro parts per thousand 2025 programme, will address the central question of heliophysics: How does the Sun create and control the heliosphere? In this paper, we present the scientific goals of the mission and provide an overview of the mission implementation.

引用

页码：25 / 70

页数：46

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