DOI QR코드

DOI QR Code

Frequency of Solar Spotless Days and Flare Index as Indices of Solar Cycle Activity

  • Oh, Suyeon (Department of Earth Science Education, Chonnam National University)
  • Received : 2014.05.09
  • Accepted : 2014.05.30
  • Published : 2014.06.15

Abstract

There was a research on the prolongation of solar cycle 23 by the solar cyclic variation of solar, interplanetary geomagnetic parameters by Oh & Kim (2013). They also suggested that the sunspot number cannot typically explain the variation of total solar irradiance any more. Instead of the sunspot number, a new index is introduced to explain the degree of solar activity. We have analyzed the frequency of sunspot appearance, the length of solar cycle, and the rise time to a solar maximum as the characteristics of solar cycle. Then, we have examined the predictability of solar activity by the characteristics of preceding solar cycle. We have also investigated the hemispheric variation of flare index for the periods that the leading sunspot has the same magnetic polarity. As a result, it was found that there was a good correlation between the length of preceding solar cycle and spotless days. When the length of preceding solar cycle gets longer, the spotless days increase. It is also shown that the shorter rise time to a solar maximum is highly correlated with the increase of sunspots at a solar maximum. Therefore, the appearance frequency of spotless days and the length of solar cycle are more significant than the general sunspot number as an index of declining solar activity. Additionally, the activity of flares leads in the northern hemisphere and is stronger in the hemisphere with leading sunspots in positive polarity than in the hemisphere with leading sunspots in negative polarity. This result suggests that it is necessary to analyze the magnetic polarity's effect on the flares and to interpret the period from the solar maximum to solar maximum as the definition of solar cycle.

References

  1. Deng LH, Qu ZQ, Wang KR, The hemispheric variation of the flare index during solar cycles 20-23, Astron. Nachr., 334, 217-222 (2013). https://doi.org/10.1002/asna.201111786
  2. Feng S, Deng L-H, Xu S, Long-term hemispheric variation of the flare index, Res. in Astron. Astrophys., 13, 343-350 (2013). http://dx.doi.org/10.1088/1674-4527/13/3/009 https://doi.org/10.1088/1674-4527/13/3/009
  3. Gao PX, Xie JL, Zhong, H, Phase Relationships Between the CME-Energy Cycle, the Sunspot-Area Cycle and the Flare-Index Cycle, Solar Phys., 289, 1831-1841 (2014). https://doi.org/10.1007/s11207-013-0409-2
  4. Kleczek J, Publ. Inst. Centr. Astron., No. 22 (Czechoslovakia, Prague: Inst. Centr. Astron.) (1952).
  5. Oh S, Kim B, Variation of Solar, Interplanetary and Geomagnetic Parameters during Solar Cycles 21-24, JASS, 30, 101-106 (2013). http://dx.doi.org/10.5140/JASS.2013.30.2.101 https://doi.org/10.5140/JASS.2013.30.2.101