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Comparison of solar activity during last two minima on turn of Activity Cycles 22/23 and 23/24

Published online by Cambridge University Press:  18 July 2013

Magdalena Gryciuk
Affiliation:
Space Research Centre, Polish Academy of Sciences, 51-622, Kopernika 11, Wroclaw, Poland, e-mail: [email protected]
Szymon Gburek
Affiliation:
Space Research Centre, Polish Academy of Sciences, 51-622, Kopernika 11, Wroclaw, Poland, e-mail: [email protected]
Marek Siarkowski
Affiliation:
Space Research Centre, Polish Academy of Sciences, 51-622, Kopernika 11, Wroclaw, Poland, e-mail: [email protected]
Piotr Podgorski
Affiliation:
Space Research Centre, Polish Academy of Sciences, 51-622, Kopernika 11, Wroclaw, Poland, e-mail: [email protected]
Janusz Sylwester
Affiliation:
Space Research Centre, Polish Academy of Sciences, 51-622, Kopernika 11, Wroclaw, Poland, e-mail: [email protected]
Frantisek Farnik
Affiliation:
Astronomical Institute, Ondrejov Observatory, Czech Republic
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Abstract

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The subject of our work is the review and comparison of solar activity during the last two solar minima that occurred between recent activity cycles. We use the soft X-ray global solar corona observations covering the two nine-months long time intervals in 1997/98 and 2009. Data from RF15-I multichannel photometer are used for the penultimate minimum. For the last unusually deep and prolonged solar activity minimum in 2009 the data from SphinX spectrophotometer are used. Comparison of measurements from both minima takes place in the overlapping energy range 2–15 keV. We focus on the active region formation, evolution and flaring productivity during respective minima.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2013 

References

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