Physics
Scientific paper
Dec 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufmsh41b1124k&link_type=abstract
American Geophysical Union, Fall Meeting 2005, abstract #SH41B-1124
Physics
7507 Chromosphere, 7509 Corona, 7513 Coronal Mass Ejections (2101), 7526 Magnetic Reconnection (2723, 7835), 7546 Transition Region
Scientific paper
The Extreme Ultraviolet Imaging Spectrometer (EIS) is part of the instrument complement on the Solar B satellite, scheduled for launch in the summer of 2006. The instrument has been calibrated and is presently mounted on the spacecraft. EIS is the most sensitive EUV solar spectrometer to be flown. The instrument is the first of a new generation of two optical element, solar spectrographs. Preliminary results from the laboratory focussing and calibration of the instrument will be shown. The instrument wavelength coverage includes reasonably bright spectral lines emitted by plasmas from 0.1 to 20 MK in temperature. The wavelength range also provides coronal density diagnostics. Temperature, density and velocity diagnostics will be discussed. An example observing program for exploring active region evolution and dynamics will be discussed.
Brown Campbell
Dere Ken
Doschek George
Klimchuk James
Korendyke Clarence Marinus
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