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WHY ARE CORONAL HOLES INDISTINGUISHABLE FROM THE QUIET SUN IN TRANSITION REGION RADIATION? Thomas Wiegelmann and Sami K. Solanki Max-Planck-Institut f¨ur Sonnensystemforschung, 37191 Katlenburg-Lindau, Germany ABSTRACT
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Document Date: 2004-09-29 09:19:51

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Company

Sun / Krivova N. A. / Krieger A.S. / /

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USD / /

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law long loops / /

Organization

National Science Foundation / Sami K. Solanki Max-Planck-Institut f¨ur Sonnensystemforschung / /

Person

Natalie Krivova / Frank Recely / Thomas Wiegelmann / Karen Harvey / Bernd Inhester / Andreas Kopp / Sami K. Solanki / /

Position

straight forward / /

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S.K. / S. K. / /

Technology

RADIATION / /

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http /

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