Occultation of a solar active region at 1.5 GHz during the eclipse of November 3, 1994

Details Occultation of a solar active region at 1.5 GHz during the eclipse of November 3, 1994 Occultation of a solar active region at 1.5 GHz during the eclipse of November 3, 1994

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006a%26a...447.1121s&link_type=abstract

Astronomy and Astrophysics, Volume 447, Issue 3, March I 2006, pp.1121-1123

Astronomy and Astrophysics

Astrophysics

1

Sun: Radio Radiation, Sun: Activity, Sunspots, Sun: Chromosphere

Scientific paper

We observed the solar eclipse of November 3, 1994 with a 4-m diameter antenna and a radio spectrograph operating at 1.5 ± 0.05 GHz with a time resolution of 100 ms. Here we present the observations of the occultation of the solar active region AR 7798 by the lunar limb. From the derivative of the eclipse curve, we found a source with an angular size of ≈ 12 s of arc associated with this active region.

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