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Intensity oscillation in H-alpha fine structure.Using a new technique of directly measuring the intensity variation from the 16 mm time-lapse filtergram movies taken in the blue wing and in the line center of H-alpha, we found periodic intensity oscillations in the center of H-alpha supergranulation network, in rosette centers and in plage granules. The oscillatory period of intensity in the network is of the order of 170 plus or minus 44 seconds while in regions of stronger magnetic field, such as in plages and in rosettes, the period was found to be longer, on the order of 300 plus or minus 50 seconds. It is suggested that observed intensity oscillation in the rosette center is related to the shooting out of dark mottles from rosettes. Oscillatory intensity fluctuations have been also observed in the sunspot umbra.
Document ID
19720052035
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Bhatnagar, A.
Tanaka, K.
(Big Bear Solar Observatory Washington, D.C., United States)
Date Acquired
August 6, 2013
Publication Date
May 1, 1972
Publication Information
Publication: Solar Physics
Volume: 24
Subject Category
Space Sciences
Accession Number
72A35701
Funding Number(s)
CONTRACT_GRANT: NSF GA-24015
CONTRACT_GRANT: NGL-05-002-071
Distribution Limits
Public
Copyright
Other

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