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

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 sun...

Full description

Bibliographic Details
Main Author: Suyeon Oh
Format: Article
Language:English
Published: Korean Space Science Society (KSSS) 2014-06-01
Series:Journal of Astronomy and Space Sciences
Subjects:
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2014/v31n2/OJOOBS_2014_v31n2_145.pdf
id doaj-d6e2aefe29f6481da99912ab73ecc449
record_format Article
spelling doaj-d6e2aefe29f6481da99912ab73ecc4492020-11-24T20:53:00ZengKorean Space Science Society (KSSS)Journal of Astronomy and Space Sciences2093-55872093-14092014-06-0131214514810.5140/JASS.2014.31.2.145Frequency of Solar Spotless Days and Flare Index as Indices of Solar Cycle ActivitySuyeon Oh0Department of Earth Science Education, Chonnam National University, Gwangju 500-757, KoreaThere 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.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2014/v31n2/OJOOBS_2014_v31n2_145.pdfsolar cyclic variationsolar activityspotless day23/24 solar cycle minimumflare index
collection DOAJ
language English
format Article
sources DOAJ
author Suyeon Oh
spellingShingle Suyeon Oh
Frequency of Solar Spotless Days and Flare Index as Indices of Solar Cycle Activity
Journal of Astronomy and Space Sciences
solar cyclic variation
solar activity
spotless day
23/24 solar cycle minimum
flare index
author_facet Suyeon Oh
author_sort Suyeon Oh
title Frequency of Solar Spotless Days and Flare Index as Indices of Solar Cycle Activity
title_short Frequency of Solar Spotless Days and Flare Index as Indices of Solar Cycle Activity
title_full Frequency of Solar Spotless Days and Flare Index as Indices of Solar Cycle Activity
title_fullStr Frequency of Solar Spotless Days and Flare Index as Indices of Solar Cycle Activity
title_full_unstemmed Frequency of Solar Spotless Days and Flare Index as Indices of Solar Cycle Activity
title_sort frequency of solar spotless days and flare index as indices of solar cycle activity
publisher Korean Space Science Society (KSSS)
series Journal of Astronomy and Space Sciences
issn 2093-5587
2093-1409
publishDate 2014-06-01
description 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.
topic solar cyclic variation
solar activity
spotless day
23/24 solar cycle minimum
flare index
url http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2014/v31n2/OJOOBS_2014_v31n2_145.pdf
work_keys_str_mv AT suyeonoh frequencyofsolarspotlessdaysandflareindexasindicesofsolarcycleactivity
_version_ 1716798386285314048