The large coronal transient of 10 June 1973. I - Observational description

Details The large coronal transient of 10 June 1973. I - Observational description The large coronal transient of 10 June 1973. I - Observational description

May 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...42..163h&link_type=abstract

Solar Physics, vol. 42, May 1975, p. 163-177.

Astronomy and Astrophysics

Astronomy

53

Solar Activity Effects, Solar Corona, Solar Prominences, Sunspot Cycle, Coronagraphs, Electron Density (Concentration), Mass Transfer, Skylab Program, Solar Radio Bursts, X Ray Astronomy

Scientific paper

Ground-based and Skylab coronagraph observations are used to trace a coronal loop transient from its inception near the surface to a distance of 5 solar radii. Events in the lower solar atmosphere associated with this feature are outlined chronologically, and its physical appearance is described. The densities, mass, and energy of the transient are estimated, its shape is determined, and its typical and atypical characteristics are noted. It is inferred that this transient was caused by the emergence of an active region. It is shown that it was not immediately preceded by a flare and that the material at its leading edge did not decelerate appreciably, even at approximately 5 solar radii.

Affiliated with

Also associated with

No associations

Rating

The large coronal transient of 10 June 1973. I - Observational description does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The large coronal transient of 10 June 1973. I - Observational description, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The large coronal transient of 10 June 1973. I - Observational description will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1050139