2013
DOI: 10.1093/mnras/stt744
|View full text |Cite
|
Sign up to set email alerts
|

Solar-cycle-related variation of solar differential rotation

Abstract: Solar-cycle related variation of differential rotation is investigated through analyzing the rotation rates of magnetic fields, distributed along latitudes and varying with time at the time interval of August 1976 to April 2008. More pronounced differentiation of rotation rates is found to appear at the ascending part of a Schwabe cycle than at the descending part on an average. The coefficient B in the standard form of differential rotation, which represents the latitudinal gradient of rotation, may be divide… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
5

Citation Types

0
12
0

Year Published

2014
2014
2023
2023

Publication Types

Select...
7

Relationship

0
7

Authors

Journals

citations
Cited by 23 publications
(12 citation statements)
references
References 48 publications
0
12
0
Order By: Relevance
“…Certain differences in the characteristics of differential rotation in the northern and southern hemispheres have been reported by many authors (e.g., see Badalyan & Sýkora 2006;Zhang et al 2011;Rightmire-Upton et al 2012;Li et al 2013). Anyway, the theory does not forbid the violation of differential rotation.…”
Section: Main Conclusion and Discussionmentioning
confidence: 90%
“…Certain differences in the characteristics of differential rotation in the northern and southern hemispheres have been reported by many authors (e.g., see Badalyan & Sýkora 2006;Zhang et al 2011;Rightmire-Upton et al 2012;Li et al 2013). Anyway, the theory does not forbid the violation of differential rotation.…”
Section: Main Conclusion and Discussionmentioning
confidence: 90%
“…However, the higher values of sunspot can be found on the solar surface; thus, the more magnetic flux erupts from solar interior towards the solar surface, which provides favourable conditions for the appearance of Rieger-type periodicity. Moreover, the variation of differential rotation parameters on the solar surface does not show high amplitude near the maximum times of solar activity cycle (Brajša et al 2006;Li et al 2013aLi et al , 2013b. According to relation of the parameters on the solar surface and that in the tachocline (Howe et al 2000b;Howe 2009), the variation of differential rotation parameters in the tachocline is also small.…”
Section: Discussionmentioning
confidence: 94%
“…The authors considered that the variation of the differential rotation parameters through the solar cycle in the tachocline only permits the strong growth of the magnetic Rossby waves only during the solar maximum, and which can interpret the appearance of Rieger-type periodicity only during the solar maximum. It is difficult to study the temporal evolution of differential rotation parameters in the tachocline, but the studies on solar-cycle-related variation of differential rotation parameters based on investigation sunspots on the solar surface show that strong magnetic fields repress differential rotation, while weak magnetic fields more reflect differentiation of rotation rates; the differential rotation parameters are smaller near the maximum times of solar activity cycle (about the fourth to the seventh year after the minimum of a solar cycle) than that in the other solar activity phases (Brajša, Ruždjak, & Wöhl 2006;Li, Xie, & Shi, 2013b). Though the variation of differential rotation parameters in the tachocline which is due to torsional oscillations (LaBonte & Howard 1982;Howe et al 2000aHowe et al , 2005Howe 2009) is different from that on the solar surface, the relation of the parameters on the solar surface and that in the tachocline (Howe et al 2000b;Howe 2009) indicates that the results obtained from the early studies of sunspots on the solar surface may reflect the variation of differential rotation parameters in the tachocline to some extent.…”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…e sunspot number in the same period is decomposed into 5 IMF components, and there exists quasiperiodicity of about 102.2a, 52.2a, and 11a. e 11a cycle obtained by multiscale analysis of sunspot number by VMD and Hilbert transform is the famous Schwabe [31] cycle, and the variance contribution rate is as high as 57.91%. It is the most significant.…”
Section: Discussionmentioning
confidence: 99%