Physics
Scientific paper
Sep 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990stin...9110832h&link_type=abstract
Unknown
Physics
Chromosphere, Heliosphere, Photosphere, Solar Atmosphere, Solar Magnetic Field, Sun, Alignment, H Alpha Line, Image Processing, Solar Flares, Solar Instruments, Solar Observatories, Telescopes
Scientific paper
The objective was to develop the capability for and coaligned observations of the structure and evolution of the Sun's magnetic field at two different heights in the solar atmosphere: the photosphere, which is the lowest region observable with optical telescopes; and the chromosphere, which lies just above the photosphere and is the region where the magnetic field dominates the gas motion so that a well-ordered structure governed by the field is observed. By obtaining this three-dimensional picture of the solar magnetic field, a better understanding can be developed of the magnetic forces that produce and control the dynamic, high-energy phenomena occurring in the solar atmosphere that can affect the entire heliosphere, including the terrestrial environment.
Gary Gilmer A.
Hagyard Mona J.
Smith Edward. J.
West Edward A.
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