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On the basis of the temporal behavior of the galactic cosmic rays and the heliospheric factors observed in 2007–2008 and 2014–2015, their average heliolongitude distributions are formed and compared. In… Click to show full abstract
On the basis of the temporal behavior of the galactic cosmic rays and the heliospheric factors observed in 2007–2008 and 2014–2015, their average heliolongitude distributions are formed and compared. In addition to the neutron monitor data, the provisional database of daily average galactic cosmic ray proton intensities measured by the PAMELA satellite-borne experiment in 2006–2015 is used. It is shown that the properties of the heliolongitude distributions in the above periods are substantially different.
Keywords:
distribution heliospheric;
longitude distribution;
2008 2014;
2007 2008;
relationship longitude;
2014 2015
Journal Title: Physics of Atomic Nuclei
Year Published: 2018
Link to full text (if available)
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Journal Title: Physics of Atomic Nuclei
Year Published: 2018
Link to full text (if available)
Share on Social Media: Sign Up to like & get
recommendations!