NDLI: Rogue Active Regions and the Inherent Unpredictability of the Solar Dynamo

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Rogue Active Regions and the Inherent Unpredictability of the Solar Dynamo

Content Provider	Scilit
Author	Petrovay, Kristóf Nagy, Melinda
Copyright Year	2018
Description	New developments in surface flux transport modeling and theory of flux transport dynamos have given rise to the notion that certain large active regions with anomalous properties (location, tilt angle and/or Hale/non-Hale character) may have a major impact on the course of solar activity in subsequent years, impacting also on the amplitude of the following solar cycles. Here we discuss our current understanding of the role of such “rogue” active regions in cycle-to-cycle variations of solar activity.
Related Links	http://arxiv.org/pdf/1804.03427 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/D464ADAB34E18C4BB6F3937C74DFB13B/S1743921318001254a.pdf/div-class-title-rogue-active-regions-and-the-inherent-unpredictability-of-the-solar-dynamo-div.pdf
Ending Page	312
Page Count	6
Starting Page	307
ISSN	17439213
e-ISSN	17439221
DOI	10.1017/s1743921318001254
Journal	Proceedings of the International Astronomical Union
Issue Number	S340
Volume Number	13
Language	English
Publisher	Cambridge University Press (CUP)
Publisher Date	2018-02-01
Access Restriction	Open
Subject Keyword	Proceedings of the International Astronomical Union Astronomy and Astrophysics Atmospheric Sciences Activity Magnetic Fields Sunspots
Content Type	Text
Resource Type	Article
Subject	Astronomy and Astrophysics Space and Planetary Science

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