Infrared solar physics from the South Pole

Details Infrared solar physics from the South Pole Infrared solar physics from the South Pole

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aipc..198..234d&link_type=abstract

IN: Astrophysics in Antarctica (A92-22401 07-89). New York, American Institute of Physics, 1989, p. 234-237.

Astronomy and Astrophysics

Astronomy

Antarctic Regions, Infrared Astronomy, Solar Physics, Space Observations (From Earth), Infrared Detectors, Magnetic Signatures, Solar Activity, Solar Magnetic Field, Solar Oscillations

Scientific paper

Infrared (IR) observations of the sun could greatly benefit from the quality of the South Pole as an IR site, and the potential for multi-day sequences of uninterrupted observations. A nearly continuous picture of the evolution of the magnetic field in solar active regions could be obtained using vector magnetographs, especially vector magnetographs which incorporate IR array detectors. Observations of the sun over a range of wavelengths in the IR continuum could also be used to study the vertical propagation characteristics of the solar p-mode oscillations.

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