Magnetic field and turbulent velocities in the solar corona

Details Magnetic field and turbulent velocities in the solar corona Magnetic field and turbulent velocities in the solar corona

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ijga....6i1007d&link_type=abstract

International Journal of Geomagnetism and Aeronomy, Volume 6, Issue 1, CiteID GI1007

Astronomy and Astrophysics

Astrophysics

Solar Physics, Astrophysics, And Astronomy: Corona, Solar Physics, Astrophysics, And Astronomy: Coronal Holes, Solar Physics, Astrophysics, And Astronomy: Magnetic Fields

Scientific paper

[1] Observations conducted by the authors during total solar eclipses in 1968, 1981, and 1999 and the results of noneclipse observations in the visual, IR, and far UV regions of the solar spectrum obtained both on the ground and in the space (according to publications of other authors) are considered. The relation of nonthermal velocities to characteristics of the magnetic field is studied. The nonthermal velocities in coronal holes are found higher than in quiet corona. In quiet corona they are higher than in the coronal cavity around a quiet prominence. A conclusion is drawn that the difference in the turbulence in various structural formations in the corona is related to the magnetic field variability.

Affiliated with

Also associated with

No associations

Rating

Magnetic field and turbulent velocities in the solar corona 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 Magnetic field and turbulent velocities in the solar corona, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetic field and turbulent velocities in the solar corona will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1365372