Coronal holes inferred from the Fleurs East-West solar scans

Details Coronal holes inferred from the Fleurs East-West solar scans Coronal holes inferred from the Fleurs East-West solar scans

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979stp.....1..288f&link_type=abstract

In NOAA Solar-Terrest. Predictions Proc., Vol. 1 p 288-311 (SEE N80-18462 09-42)

Astronomy and Astrophysics

Astronomy

Coronal Holes, Solar Radio Emission, Solar Spectra, Radio Astronomy, Radio Spectra, Solar Rotation, Solar Terrestrial Interactions

Scientific paper

East-West solar scans produced daily on 692 and 1415 MHz are analyzed
for the period 1968 to 1973. The analysis confirms that coronal holes
are stable features displaying significantly reduced electromagnetic
emission which can persist for many solar rotations. The coronal hole
observations are summarized in a series of tables.

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