Absolute flows in the solar transition region

Details Absolute flows in the solar transition region Absolute flows in the solar transition region

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.170..173e&link_type=abstract

(IAU, European Regional Astronomy Meeting, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics and Space Science (ISSN 0004-640

Astronomy and Astrophysics

Astrophysics

1

Magnetohydrodynamic Flow, Solar Limb, Solar Prominences, Stellar Spectra, H Alpha Line, Ultraviolet Spectra

Scientific paper

It is the objective of the present study to establish an absolute scale
for flows in the solar transition region in observations obtained with
the UVSP/SMM. By use of the polar limbs as reference it is found that
the downflows range between 3 and 10 km/s. The brighter regions show the
largest downward flows.

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