NDLI: Study of Variations in Solar Differential Rotation Based on Compact Magnetic Features and Hydrogen Hα Filaments

Content Provider	Springer Nature Link
Author	Japaridze, D. R. Chargeishvili, B. B.
Copyright Year	2016
Abstract	Data on compact magnetic features and hydrogen Hα filaments during solar activity cycles 20 and 21 are used to study variations in the solar differential rotation. The difference in the differential rotation rates of the compact magnetic features and hydrogen Hα filaments is greatest between the 20-30° and 30-40° latitude zones in both solar hemispheres. The rotation rates of the compact magnetic featuresat all latitudes are higher than those of the hydrogen Hα filaments and the difference between them increases with latitude.
Starting Page	389
Ending Page	397
Page Count	9
File Format	PDF
ISSN	05717256
Journal	Astrophysics
Volume Number	59
Issue Number	3
e-ISSN	15738191
Language	English
Publisher	Springer US
Publisher Date	2016-08-13
Publisher Place	New York
Access Restriction	One Nation One Subscription (ONOS)
Subject Keyword	Solar rotation hydrogen Hα filaments compact magnetic features Astronomy, Astrophysics and Cosmology Astrophysics and Astroparticles Extraterrestrial Physics, Space Sciences Astronomy, Observations and Techniques
Content Type	Text
Resource Type	Article
Subject	Astronomy and Astrophysics

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Study of Variations in Solar Differential Rotation Based on Compact Magnetic Features and Hydrogen Hα Filaments