Publication Date:
2006-01-16
Description:
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.
Keywords:
SOLAR PHYSICS
Type:
NOAA Solar-Terrest. Predictions Proc., Vol. 1; p 288-311
Format:
text
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