skip to main content

Title: Revisiting the question: Does high-latitude solar activity lead low-latitude solar activity in time phase?

Cross-correlation analysis and wavelet transform methods are used to investigate whether high-latitude solar activity leads low-latitude solar activity in time phase or not, using the data of the Carte Synoptique solar filaments archive from 1919 March to 1989 December. From the cross-correlation analysis, high-latitude solar filaments have a time lead of 12 Carrington solar rotations with respect to low-latitude ones. Both the cross-wavelet transform and wavelet coherence indicate that high-latitude solar filaments lead low-latitude ones in time phase. Furthermore, low-latitude solar activity is better correlated with high-latitude solar activity of the previous cycle than with that of the following cycle, which is statistically significant. Thus, the present study confirms that high-latitude solar activity in the polar regions is indeed better correlated with the low-latitude solar activity of the following cycle than with that of the previous cycle, namely, leading in time phase.
Authors:
;  [1] ;  [2]
  1. Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011 (China)
  2. College of Mathematics Physics and Information Engineering, Jiaxing University, Jiaxing 314001 (China)
Publication Date:
OSTI Identifier:
22340290
Resource Type:
Journal Article
Resource Relation:
Journal Name: Astronomical Journal (New York, N.Y. Online); Journal Volume: 147; Journal Issue: 5; Other Information: Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; CORRELATIONS; DATA ANALYSIS; FILAMENTS; POLAR REGIONS; ROTATION; SOLAR ACTIVITY; SUN