Extreme-infrared brightness profile of the solar chromosphere obtained during the total eclipse of 1991

Details Extreme-infrared brightness profile of the solar chromosphere obtained during the total eclipse of 1991 Extreme-infrared brightness profile of the solar chromosphere obtained during the total eclipse of 1991

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992natur.358..308l&link_type=abstract

Nature (ISSN 0028-0836), vol. 358, no. 6384, July 23, 1992, p. 308-310. Research supported by NSF.

Physics

12

Brightness Distribution, Chromosphere, Infrared Radiation, Solar Atmosphere, Solar Eclipses, Atmospheric Temperature, Solar Observatories, Temperature Profiles

Scientific paper

A temperature profile in 1.3 mm radiation with about 300 km resolution
at the sun was obtained during the total eclipse of 1991. The
observations indicate that spicules reach a temperature of 8000 K at
3000-4000 km above the photosphere. This temperature is lower than those
of many spicule models.

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