White light solar corona: an atlas of 1984 K-coronameter synoptic charts, December 1983 - January 1985

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Charts, High Altitude, Solar Corona, Synoptic Meteorology, Data Reduction, Light Scattering, Sky Brightness, Sky Radiation, Solar Limb

Scientific paper

The synoptic observing project of the High Altitude Observatory's Coronal Dynamics Project began on 5 August 1980. The data obtained by the Mark-3 K-coronameter located at the Mauna Loa Solar Observatory, Hawaii, are published yearly in volumes of the White Light Solar Corona: An Atlas of K-coronameter Synoptic Charts. The reader will notice a segment of overlapped data at both the beginning and the end of each volume. This is necessary to provide a complete data set of Carrington rotations covering a specific time period because west limb passage occurs 14 days after east limb passage. This set of synoptic data should be regarded as a preliminary presentation in which no corrections have been made for the day-to-day variations in sky transmission and scattering of polarized light by the Earth's atmosphere.

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