NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
A statistical study of active regions 1967-1981A study is conducted of 15 years of active region data based on the Mount Wilson daily magnetograms in the interval 1967-1981. The analysis revealed the following: (1) The integral number of regions decreases exponentially with increasing region sizes, or N(A) = 4788 exp(-A/175) for the 15 years of data, where A is the area in square degrees and N(A) is the number of active regions with area equal to or greater than A; (2) the average area of active regions varies with the phase of the solar cycle. There are more larger regions during maximum than during minimum. (3) Regions in the north are 10 percent larger on average than those in the south during this interval. This coincides with a similar asymmetry in the total magnetic flux between the hemispheres. (4) Regions of all sizes and magnetic complexities show the same characteristic latitude variation with phase in the solar cycle. The largest regions, however, show a narrower latitude range.
Document ID
19840056747
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Tang, F.
(Big Bear Solar Observatory Pasadena, CA, United States)
Howard, R.
(Hale Observatories Pasadena, CA, United States)
Adkins, J. M.
(Mount Wilson and Las Campanas Observatories Pasadena, CA, United States)
Date Acquired
August 12, 2013
Publication Date
March 1, 1984
Publication Information
Publication: Solar Physics
Volume: 91
ISSN: 0038-0938
Subject Category
Solar Physics
Accession Number
84A39534
Funding Number(s)
CONTRACT_GRANT: NSF ATM-81-16964
CONTRACT_GRANT: N00014-81-C-0065
CONTRACT_GRANT: NGR-09-140-015
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available