La Posta Solar Radio Maps (2nd Quarter, 1979)

The La Posta 18.3-m antenna has been used since 1972 to acquire radio maps of the solar disk at wavelengths of 0.86 and 2.0 cm. The NOSC in-house research program is supporting the continuation of this program through the peak of the present solar activity cycle (about 1981). During this period of o...

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Bibliographische Detailangaben
Hauptverfasser:	Argo ,P E, Wefer,F L
Format:	Report
Sprache:	eng
Schlagworte:	Antenna temperature Astronomy Cybernetics Dicke radiometers Electrical and Electronic Equipment FBS(Flare Buildup Study) K BAND La Posta antenna LPN-NOSC-ZS-17 MAPPING NOISE GENERATORS PASSIVE SYSTEMS RADAR RECEIVERS RADIO ASTRONOMY Radio maps RADIOMETERS SOLAR ACTIVITY SOLAR FLARES SOLAR RADIATION SOLAR RADIO MAPS SUN
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Beschreibung
Zusammenfassung:	The La Posta 18.3-m antenna has been used since 1972 to acquire radio maps of the solar disk at wavelengths of 0.86 and 2.0 cm. The NOSC in-house research program is supporting the continuation of this program through the peak of the present solar activity cycle (about 1981). During this period of operation, daily (5 days per week) radio maps at both wavelengths will be acquired. This report presents the radioheliogram data for the second quarter of 1979. (Author)