Plans to Observe Flare-Associated Waves with Solar-B

Details Plans to Observe Flare-Associated Waves with Solar-B Plans to Observe Flare-Associated Waves with Solar-B

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..369..205n&link_type=abstract

New Solar Physics with Solar-B Mission ASP Conference Series, Vol. 369, proceedings of the conference held 8-11 November, 2005 a

Physics

1

Scientific paper

The textit{Solar-B} satellite has three scientific instruments: the Solar Optical Telescope (SOT), the X-ray Telescope (XRT) and the EUV Imaging Spectrograph (EIS). We expect SOT, XRT, and EIS to detect the origin of Moreton waves, coronal X-ray waves, and line-of-sight velocity of waves, respectively. In preparation for Solar-B, we examine the detectable possibility of waves with these telescopes and suggest methods for observation.

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