Modern representation of databases on the example of the Catalog of Solar Proton Events in the 23rd Cycle of Solar Activity

2017 ◽  
Vol 57 (6) ◽  
pp. 684-690
Author(s):  
V. N. Ishkov ◽  
L. P. Zabarinskaya ◽  
N. A. Sergeeva
Author(s):  
Yury Logachev ◽  
◽  
Galina Bazilevskaya ◽  
Eduard Vashenyuk ◽  
Elena Daibog ◽  
...  

Author(s):  
Yury Logachev ◽  
◽  
Galina Bazilevskaya ◽  
Eduard Vashenyuk ◽  
Elena Daibog ◽  
...  

2019 ◽  
Author(s):  
◽  
Vitaly Ishkov ◽  
Yury Logachev ◽  
Galina Bazilevskaya ◽  
Elena Daibog ◽  
...  

2019 ◽  
Author(s):  
◽  
Vitaly Ishkov ◽  
Yury Logachev ◽  
Galina Bazilevskaya ◽  
Elena Daibog ◽  
...  

2018 ◽  
Vol 13 (S340) ◽  
pp. 265-266
Author(s):  
S. Aranya ◽  
T. E. Girish ◽  
G. Gopkumar ◽  
N. G. Nisha

AbstractWe could identify three categories of solar proton events (SPE) with distinct solar origin from an analysis of direct and indirect observations during the years 1561-2016 CE spanning 42 sunspot cycles. They are (i) 10 MeV SPE whose number of occurrences closely follow the sunspot cycles (ii) 30 MeV SPE which show secular changes with peaks near Gleissberg solar cycle minima and inferred to be associated with distinct enhancements in the efficiency of the solar dynamo and (iii) those associated with Impulsive and irregular solar activity changes such as the Carrington event of September 1859. The relevance of above results for stars exhibiting cyclic and irregular activity changes will be also discussed.


Radiocarbon ◽  
1992 ◽  
Vol 34 (2) ◽  
pp. 255-262 ◽  
Author(s):  
M. A. Shea ◽  
D. F. Smart

A study of the solar proton event data between 1954 and 1986 indicates that the large fluence events at the Earth are usually associated with a sequence of solar activity and related geomagnetic storms. This association appears to be useful to infer the occurrence of major fluence proton events extending back to 1934, albeit in a non-homogeneous manner. We discuss the possibility of identifying major solar proton events prior to 1934, using geomagnetic records as a proxy.


1984 ◽  
Vol 5 (4) ◽  
pp. 593-594
Author(s):  
A. G. Fenton ◽  
K. B. Fenton ◽  
J. E. Humble

Six solar proton events have been observed by ground level cosmic ray detectors so far during solar cycle 21, a little less than one per year. All of these have been much smaller than the giant events observed in solar cycle 19. As with many other aspects of solar activity, the reason for the differences from cycle to cycle remain unknown.


2015 ◽  
Vol 79 (5) ◽  
pp. 573-576 ◽  
Author(s):  
G. A. Bazilevskaya ◽  
Yu. I. Logachev ◽  
E. V. Vashenyuk ◽  
E. I. Daibog ◽  
V. N. Ishkov ◽  
...  

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