Physics
Scientific paper
Apr 1973
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973p%26ss...21..703g&link_type=abstract
Planetary and Space Science, Volume 21, Issue 4, p. 703-707.
Physics
3
Scientific paper
An analysis on the variation of coronal λ5303 intensity relative to the solar magnetic sector boundaries is presented. The location of the boundaries has been extrapolated from the observed interplanetary sector structure. The results indicate that in the years 1962-1964 the solar activity is in general high to the west and low to the east of a solar sector boundary. Such a distribution of solar activity contradicts with the one assumed up to now. Nevertheless, this distribution is in general in agreement with results of investigations on the correlation between solar and geomagnetic activity. Now at: Department of Physics, Agricultural University of Norway, 1432 Ås-NLH, Norway.
No associations
LandOfFree
On the variation of the coronal λ5303 intensity relative to the interplanetary and solar magnetic sector structure, and to geomagnetic activity 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 On the variation of the coronal λ5303 intensity relative to the interplanetary and solar magnetic sector structure, and to geomagnetic activity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the variation of the coronal λ5303 intensity relative to the interplanetary and solar magnetic sector structure, and to geomagnetic activity will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-851273