HR: 0800h
AN: SH41B-1124 [Abstracts]
TI: Observing the Solar atmosphere with the Extreme Ultraviolet Imaging Spectrometer on Solar B
AU: * Korendyke, C M
EM: ckorendyke@ssd5.nrl.navy.mil
AF: Naval Research Laboratory, 4555 Overlook Ave, Washington, DC 20375
United States
AU: Brown, C
SH41B-1124
AF: Naval Research Laboratory, 4555 Overlook Ave, Washington, DC 20375
United States
AU: Dere, K
SH41B-1124
AF: George Mason University, 4400 University Drive, Fairfax, VA 22030
United States
AU: Doschek, G
SH41B-1124
AF: Naval Research Laboratory, 4555 Overlook Ave, Washington, DC 20375
United States
AU: Klimchuk, J
SH41B-1124
AF: Naval Research Laboratory, 4555 Overlook Ave, Washington, DC 20375
United States
AU: Landi, E
SH41B-1124
AF: Naval Research Laboratory, 4555 Overlook Ave, Washington, DC 20375
United States
AU: Mariska, J
SH41B-1124
AF: Naval Research Laboratory, 4555 Overlook Ave, Washington, DC 20375
United States
AU: Warren, H
SH41B-1124
AF: Naval Research Laboratory, 4555 Overlook Ave, Washington, DC 20375
United States
AU: Lang, J
SH41B-1124
AF: Rutherford Appleton Laboratory, CCLRC, Chilton, Didcott, OX11 OQX
United Kingdom
AB:
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.
DE: 7507 Chromosphere
DE: 7509 Corona
DE: 7513 Coronal mass ejections (2101)
DE: 7526 Magnetic reconnection (2723, 7835)
DE: 7546 Transition region
SC: SPA-Solar and Heliospheric Physics [SH]
MN: Fall Meeting 2005