Solar North-South Asymmetry and Hilbert Transform Analysis

Citations

WEB OF SCIENCE

1
Citations

SCOPUS

1

초록

Here, we investigated the observed sunspot areas with respect to latitudes using the Hilbert transform technique. Conventional study of the cyclic patterns of sunspots is based on the Lomb-Scargle periodogram, which only obtains the amplitude information. In comparison, our approach characterizes the amplitude as well as the phase of solar activity. We demonstrated the solar Nor th-South asymmetry in the instantaneous amplitude by analyzing daily sunspot data set spanning from the solar cycles 11 to 24. Our findings confirm that the northern hemisphere is dominant in the solar cycles 14, 15, 16, 18, and 20. Unlike the amplitude, the Nor th-South asymmetry in the period of solar activity could not be established. We have also found that the standard deviation as a measure of fluctuation in the phase derivative is minimum in the latitude band 10 degrees < l < 20 degrees, and the fluctuations obtained for latitudes above 30 degrees are considerable.

키워드

Sun: sunspot; Sun: activity; methods: data analysis; N-S ASYMMETRY; MAGNETIC-FIELD REVERSAL; LONG-TERM VARIATIONS; NUMBERS R-N; LATITUDINAL DISTRIBUTION; DIFFERENTIAL ROTATION; PERIODIC BEHAVIOR; FLUX TRANSPORT; SUNSPOT CYCLE; DYNAMO
제목
Solar North-South Asymmetry and Hilbert Transform Analysis
저자
Chang, Heon-Young
DOI
10.5303/JKAS.2023.56.1.125
발행일
2023-04
유형
Article
저널명
Journal of the Korean Astronomical Society
권
56
호
1
페이지
125 ~ 135