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Observing CMEs Without Coronagraphs

Hugh Hudson


A coronal mass ejection, strictly speaking, is a phenomenon observed in a white-light coronal imager. This paper reviews the likely signatures of CMEs in other forms of observation,  ranging from the photosphere to the interplanetary medium.

  Organization: SPRC
     Telephone: +81-42-759-8147
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        e-mail: hudson@isass1.solar.isas.ac.jp
       Address: ISAS 3-1-1 Yoshinodai
   Japan 229 Observing CMEs Without Coronagraphs

Above is background material for archival reference only.

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Curators: Robert Candey, Alex Young, Tamara Kovalick

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