Outflows and ejections in the solar transition zone

Details Outflows and ejections in the solar transition zone Outflows and ejections in the solar transition zone

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...310..456d&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 310, Nov. 1, 1986, p. 456-462.

Other

13

Jet Flow, Solar Atmosphere, Stellar Mass Ejection, Transition Points, Ultraviolet Spectra, Carbon, Normal Density Functions, Red Shift, Spectral Energy Distribution, Time Series Analysis

Scientific paper

Time series images of C IV transition zone intensities and velocities are analyzed to study the uncommon patterns of blueshifted emission. The images are constructed from stigmatic spectra obtained during the third flight of the NRL High Resolution Telescope and Spectrograph. A sample of 11 blueshifted events with near-Gaussian profiles are analyzed. Of these 11 cases, three are expulsions of material from the network, two are spicular flows, one is a simple jet, another is associated with a filament, and four are unexplained. It is not possible to identify a simple mechanism whereby upflows return to form the predominant downflows observed in the transition zone, and the upward mass flux is three orders of magnitude lower than the downward mass flux.

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