An active solar prominence in 1.3 mm radiation

We present new millimeter-wavelength observations of an active solar prominence. Observations made over a two-day period with the James Clerk Maxwell Telescope on Mauna Kea, Hawaii, give a unique view in 1.3 mm radiation of the spectacular prominence that appeared on the west solar limb in the total...

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Veröffentlicht in:Astronomy and astrophysics (Berlin) 1993-07, Vol.274 (1), p.L9-L12
Hauptverfasser: HARRISON, R. A, CARTER, M. K, TOMPKINS, G. J, BRAUN, D, CLARK, T. A, LINDSEY, C, JEFFERIES, J. T, SIME, D. G, WATT, G, ROELLIG, T. L, BECKLIN, E. E, NAYLOR, D. A
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Sprache:eng
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Zusammenfassung:We present new millimeter-wavelength observations of an active solar prominence. Observations made over a two-day period with the James Clerk Maxwell Telescope on Mauna Kea, Hawaii, give a unique view in 1.3 mm radiation of the spectacular prominence that appeared on the west solar limb in the total solar eclipse of 11 July 1991.
ISSN:0004-6361
1432-0746