Solar mass flow in fine-scale structures

Details Solar mass flow in fine-scale structures Solar mass flow in fine-scale structures

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ssrv...70...21d&link_type=abstract

Space Science Reviews, Volume 70, Issue 1-2, pp. 21-30

Physics

12

Sun, Flows, Velocities

Scientific paper

Observations of transient and steady velocities at chromospheric, transition region and coronal temperatures in the quiet Sun and coronal holes are reviewed. The relevance of fine-scale structures in governing the mass balance of the solar atmosphere is stressed. At present, a coherent picture of these mass flows does not exist. However, the current observational base of transition region and coronal velocity information is limited but should greatly improve with measurements from the SOHO satellite.

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