Synoptic solar magnetic field maps for the interval including Carrington Rotation 1601-1680, May 5, 1973 - April 26, 1979

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Magnetic Signatures, Solar Magnetic Field, Solar Rotation, Sun, Coronal Holes, Skylab Program, Synoptic Measurement, Telescopes

Scientific paper

Regular observations of solar magnetic fields were made, primarily in response to the needs of the Skylab mission. Daily full disk observations were first combined into synoptic maps during the Skylab Solar Workshop on Coronal Holes and High Speed Wind Streams and were used for studies of the magnetic field strength below coronal holes and extrapolations of the magnetic field into the corona. Starting with Carrington rotation number 1681, the synoptic maps are produced and published regularly. Old data obtained prior to Carrington rotation number 1681 processed into synoptic maps in the same way as current data are processed, are presented in the same format.

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