The Hale solar sector boundary

Details The Hale solar sector boundary The Hale solar sector boundary

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976stin...7711955s&link_type=abstract

Unknown

Physics

Solar Corona, Solar Magnetic Field, Brightness, Magnetic Flux, Photosphere, Solar Activity, Sunlight

Scientific paper

A Hale solar sector boundary is defined as the half (Northern Hemisphere or Southern Hemisphere) of a sector boundary in which the change of sector magnetic field polarity is the same as the change of polarity from a preceding spot to a following spot. Above a Hale sector boundary the green corona has maximum brightness, while above a non-Hale boundary the green corona has a minimum brightness. The Hale portion of a photospheric sector boundary tends to have maximum magnetic field strength, while the non-Hale portion has minimum field strength.

Affiliated with

Also associated with

No associations

Rating

The Hale solar sector boundary 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 Hale solar sector boundary, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Hale solar sector boundary will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1222149