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Proposal ID Hara_255

Date of Proposal Nov 14 2001

firstname
Hirohisa

lastname
Hara

institute
National Astronomical Observatory, Japan

address
2-21-1 Osawa, Mitaka, Tokyo 181-8588

email
hara@solar.mtk.nao.ac.jp

phone
+81-422-34-3705

fax
+81-422-34-3700

proposal
A coronal bidirectional flow was observed at the east limb in
the spectroscopic observation of Fe X line on 12 Sep 2001. I
would like to study the change of coronal structures seen in
EIS images around the flow.

inside_collab
J.P. Delaboudinière

consortium
no

topic
Magnetic Reconnection

topic

title
Change of coronal structures around the bi-directional flow


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