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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Date: 2004-09-29 09:19:51 Space plasmas Astrophysics Astronomy Coronal loop Corona Solar transition region Solar wind Solar variation Chromosphere Sun Physics Plasma physics		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 Add to Reading List Source URL: star.mpae.gwdg.de Download Document from Source Website File Size: 1,20 MB Share Document on Facebook

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