Ultraviolet observations of solar fine structure

Details Ultraviolet observations of solar fine structure Ultraviolet observations of solar fine structure

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987sci...238.1267d&link_type=abstract

Science (ISSN 0036-8075), vol. 238, Nov. 27, 1987, p. 1267-1269.

Computer Science

17

Chromosphere, Fine Structure, Satellite-Borne Instruments, Solar Spectra, Ultraviolet Spectroscopy, Emission Spectra, Spacelab Payloads, Temporal Distribution

Scientific paper

The High Resolution Telescope and Spectrograph was flown on the Spacelab-2 shuttle mission to perform extended observations of the solar chromosphere and transition zone at high spatial and temporal resolution. Ultraviolet spectroheliograms show the temporal development of macrospicules at the solar limb. The C IV transition zone emission is produced in discrete emission elements that must be composed of exceedingly fine (less than 70 kilometers) subresolution structures.

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