Occurrence rate of SAR arcs during the 23rd solar activity cycle |
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Authors: | V.N. Alexeyev I.B. IevenkoS.G. Parnikov |
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Affiliation: | Yu. G. Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch, Russian Academy of Sciences, 31 Lenin Ave., 677980 Yakutsk, Russia |
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Abstract: | The occurrence rate of SAR arcs during 1997–2007 has been analyzed based on the photometric observations at the Yakutsk meridian (Maimaga station, corrected geomagnetic coordinates: 57°N, 200°E). SAR arcs appeared in 114 cases (∼500 h) during ∼370 nights of observations (∼3170 h). The occurrence frequency of SAR arcs increases to 27% during the growth phase of solar activity and has a clearly defined maximum at a decline of cycle 23. The SAR arc registration probability corresponds to the variations in geomagnetic activity in this solar cycle. The dates, intervals of UT, and geomagnetic latitudes of SAR arc observations at the Yakutsk meridian are presented. |
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Keywords: | SAR arc Photometric observations Solar cycle Geomagnetic activity |
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