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The Astrophysical Journal, 685:1262Y 1269, 2008 October 1 # 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A. PLASMA FLOWS GUIDED BY STRONG MAGNETIC FIELDS IN THE SOLAR CORONA Eckart Marsch
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Document Date: 2010-03-09 05:01:02


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City

Berlin / San Francisco / Cambridge / Beijing / Marsch et / Katlenburg-Lindau / Surrey / Solanki / /

Company

CHs / originating in CHs / /

Country

Poland / Germany / Norway / United Kingdom / /

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Facility

China Jian Sun UCL-Mullard Space Science Laboratory / Peking University / Heliospheric Observatory / /

IndustryTerm

magnetic network / ultraviolet imaging / chromospheric network / energy / /

Movie

A. I. / /

Organization

Japanese mission / Thomas Wiegelmann Max-Planck-Institut fu¨r Sonnensystemforschung / Department of Geophysics / Peking University / China Jian Sun UCL-Mullard Space Science Laboratory / National Natural Science Foundation of China / STFC / U.S.A. PLASMA FLOWS GUIDED BY STRONG MAGNETIC FIELDS IN THE SOLAR CORONA Eckart Marsch Max-Planck-Institut / ESA / Cambridge Univ. / National Oceanic and Atmospheric Administration / National Aeronautics and Space Administration / China Scholarship Council / American Astronomical Society / Max-Planck-Institut fu¨r Sonnensystemforschung / Hui Tian Max-Planck-Institut fu¨r Sonnensystemforschung / /

Person

Rabin / Mariska / ESA SP / Thomas Wiegelmann / Werner Curdt / Jian Sun / Hui Tian / AR NOAA / /

Position

driver / /

ProvinceOrState

Alabama / S. K. / /

PublishedMedium

The Astrophysical Journal / /

Technology

Geophysics / radiation / X-ray / condensation / spectroscopy / fluid dynamics / ESA / /

SocialTag