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The Solar Wind Generation Experiment for Spartan Mission 201

Published online by Cambridge University Press:  12 April 2016

J.L. Kohl ,
H. Weiser ,
G.L. Withbroe  and
R.H. Munro
J.L. Kohl
Affiliation:
Harvard-Smithsonian Center for Astrophysics Cambridge, MA 02138
H. Weiser
Affiliation:
Harvard-Smithsonian Center for Astrophysics Cambridge, MA 02138
G.L. Withbroe
Affiliation:
Harvard-Smithsonian Center for Astrophysics Cambridge, MA 02138
R.H. Munro
Affiliation:
High Altitude Observatory Boulder, CO 80307

Extract

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The Solar Wind Generation Experiment consists of a UV Coronal Spectrometer (UVCS) provided by the Harvard-Smithsonian Center for Astrophysics and a White Light Coronagraph (WLC) of the High Altitude Observatory. The instruments are similar to those flown together on three sounding rocket flights [1,2,3] but they have enhanced capabilities to take advantage of Spartan’s 27 hour observing period. The two instruments comprise a payload for Spartan 2, which is a self-contained instrument carrier that provides on-board data storage, power, thermal control, sun pointing and an observing program sequencer. Spartan is launched and deployed by the Shuttle and spends about 27 orbits in a detached mode before it is recovered and returned to the ground for data tape retrieval and post-flight instrument calibration.

Type
Session 1. Solar Astrophysics
Information
International Astronomical Union Colloquium , Volume 86: Eighth International Colloquium on Ultraviolet and X-ray Spectroscopy of Astrophysical and Laboratory Plasmas , 1984 , pp. 29 - 31
Copyright
Copyright © Naval Research Laboratory 1984. Publication courtesy of the Naval Research Laboratory, Washington, DC.

References

1. Kohl, J.L., Weiser, H. Withbroe, G.L., Noyes, R.W., Parkinson, W.H., Reeves, E.M., MacQueen, R.M. and Munro, R.H., Astrophys. J. 241, L117 (1980).CrossRefGoogle Scholar
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