Paper:	Solar-B EUV Imaging Spectrometer (EIS)
Volume:	325, The Solar-B Mission and the Forefront of Solar Physics
Page:	27
Authors:	Hara, H.
Abstract:	The Extreme-ultraviolet Imaging Spectrometer (EIS) onboard Solar-B is designed and being developed under international collaboration to execute spectroscopic observations of the dynamical solar upper atmosphere in two extreme-ultraviolet wavelength ranges, 170-210 Å and 250-290 Å. These bands include strong emission lines that are formed at 104.7-107.3 K. A high-cadence spectroscopic observation with EIS is suitable for the studies of coronal heating process and it will reveal dynamical plasma motions in/around solar flares of all sizes. It is of particular importance to specify the key physics of coronal heating process and solar dynamic events through collaborative observations with SOT and XRT on the same spacecraft.

Astronomical Society of the Pacific
Conference Series

© Copyright 1988 - 2024 - Astronomical Society of the Pacific
No part of the material protected by this copyright may be reproduced or used in any form other than for personal use without written permission from the ASP.

Page generated in 0.040 seconds