The 3rd Joint Solar Dynamics Project data summary: Solar magnetic field, chromospheric and coronal observations near the time of the 18 March 1988 solar eclipse

Details The 3rd Joint Solar Dynamics Project data summary: Solar magnetic field, chromospheric and coronal observations near the time of the 18 March 1988 solar eclipse The 3rd Joint Solar Dynamics Project data summary: Solar magnetic field, chromospheric and coronal observations near the time of the 18 March 1988 solar eclipse

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jsdp.rept.....s&link_type=abstract

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Physics

Chromosphere, Magnetic Fields, Photosphere, Solar Corona, Solar Eclipses, Density Measurement, Periodic Variations, Photography, Temperature Measurement

Scientific paper

The general goal of the HAO/University of Hawaii Joint Solar Dynamics Project is to establish the relationships that exist between the solar magnetic field which is detected in the photosphere and the structure and evolution of the corona. The SOLDYN programs of 1982 and 1983 demonstrated the ability to use existing instruments to gather data of value in the pursuit of that goal. The goals for the observations in 1988 are as follows: (1) Document the state of the sun, from the photosphere up through the chromosphere and out into the corona for the approximately four-week interval around the total solar eclipse of 18 March 1988, and (2) Identify the relationship between the photospheric magnetic fields and the temperature and density structure of the corona. The reduced observations made during this SOLDYN 3 period necessary to achieve these goals are provided. The observations are presented both in the form of daily photographic and photo-electric measurements, and in synoptic format for the period.

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