Observations and modeling of the prominence/corona transition region

Details Observations and modeling of the prominence/corona transition region Observations and modeling of the prominence/corona transition region

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987esasp.275...21e&link_type=abstract

In ESA, Proceedings of the 21st ESLAB Symposium on Small Scale Plasma Processes in the Solar Chromosphere/Corona, Interplanetary

Astronomy and Astrophysics

Astronomy

14

Astronomical Models, Solar Corona, Solar Prominences, Solar Temperature, Temperature Distribution, Energy Transfer, Skylab Program, Spacelab Payloads, Ultraviolet Astronomy

Scientific paper

The construction of inhomogeneous temperature transition region models for solar prominences is considered. Models based on UV line intensities from SO82B on Apollo Telescope Mount (ATM)/Skylab and the High Resolution Telescope and Spectrograph (HRTS) on Spacelab 2 are derived. The modeled structures of the transition region are in the form of thin tubes, similar to the prominence structures seen in the cool core. An expression for the thickness of the transition region around prominences is given, and mechanisms for energy transport are discussed. Uncertainties and possible improvements in the modeling are pointed out.

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