Spatial evolution of magnetic fields as seen in coronal streamers to 12 RO during the solar cycle

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Magnetic Field Configurations, Solar Corona, Solar Cycles, Solar Flares, Aerial Photography, Imaging Techniques, Solar Eclipses, Solar Magnetic Field, Solar Wind

Scientific paper

Outer coronal photographs made from high altitude aircraft at the solar eclipses of 1966, '70, '72, '73, and '79 which sample various times in the solar cycle are presented. Coronal streamers extending from the solar limb to 12 Ro are displayed. The evolution of the streamers as they distort magnetic field lines to large distances from the Sun is examined. Results show that the distortion is varied, that the polar plumes can be traced beyond 8 Ro, diverging apparently along dipole field lines, and that the divergence varies along the solar cycle. Various changes in nonpolar streamers are discussed including the tendency to become radial beyond 3 to 5 Ro as if controlled by the solar wind.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Spatial evolution of magnetic fields as seen in coronal streamers to 12 RO during the solar cycle 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 Spatial evolution of magnetic fields as seen in coronal streamers to 12 RO during the solar cycle, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spatial evolution of magnetic fields as seen in coronal streamers to 12 RO during the solar cycle will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1622912

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.