Longitudinal Structure of the Double Magnetic Cycle

Details Longitudinal Structure of the Double Magnetic Cycle Longitudinal Structure of the Double Magnetic Cycle

Aug 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998soph..181..479b&link_type=abstract

Solar Physics, v. 181, Issue 2, p. 479-489 (1998).

Physics

14

Scientific paper

The longitudinal structure of the double magnetic cycle of solar activity has been investigated using Stanford magnetograph data from 1976 to 1996 (cycles 21 and 22). It is shown that both high-frequency and low-frequency sources of the magnetic field are present in the data and that they reach their maxima in longitudinal zones that are separated by 20 deg. Some longitudinal zones are found to exist in which the high-frequency component is dominant and other longitudinal zones are found in which the low-frequency component is dominant.

Affiliated with

Also associated with

No associations

Rating

Longitudinal Structure of the Double Magnetic 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 Longitudinal Structure of the Double Magnetic Cycle, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Longitudinal Structure of the Double Magnetic Cycle will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1538607