Solar Bright Point animation

The magnetic field temporal evolution of a bipolar region (top right-hand corner) associated with a coronal bright point. The MDI images have a 157 arcsec x 124 arcsec field-of-view, with the scaling from -25 to +25 G. These frames cover the time period from 16:10 UT on October 17 to 05:26 UT on October 18, 1996.

"An EUV Bright Point as seen by SUMER, CDS, MDI and EIT on-board SoHO"
M.S. Madjarska, J.G. Doyle, L. Teriaca, and D. Banerjee
Astronomy & Astrophysics (2002) in press
Full Paper - Postscript
Full Paper - PDF

See also:
Preprint Series
Latest SoHO Images

Last Revised: 2009 November 10th