Computer Science – Databases
Scientific paper
Sep 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.535..671k&link_type=abstract
In: Solar variability as an input to the Earth's environment. International Solar Cycle Studies (ISCS) Symposium, 23 - 28 June 2
Computer Science
Databases
Solar Corona, Cosmic Rays
Scientific paper
Two existing databases of green coronal brightness (Fe XIV, 530.3 nm line) are used to provide the correlative analysis with cosmic ray intensity during epochs of opposite IMF polarity from 1939 to 1988 for periods of small and moderate solar activity. The result well confirms the drift theory of cosmic rays during two epochs of A<0 (1959-1967, 1982-1988) when the correlation of cosmic ray intensity between the variability of corona characterized by the green coronal line appeared to be stronger closely to the equatorial plane than during positive epoch (A>0). Additionally we have compared two approachable coronal databases. It is shown that the cosmic radiation is mostly influenced by activity of the middle-heliolatitudinal coronal belts.
Izdebska J.
Kobylinski Z.
No associations
LandOfFree
Cosmic ray intensity response to variability of corona at different heliographic latitudes 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 Cosmic ray intensity response to variability of corona at different heliographic latitudes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cosmic ray intensity response to variability of corona at different heliographic latitudes will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1152985