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H-alpha macrospicules - Identification with EUV macrospicules and with flares in X-ray bright pointsThe paper presents observational evidence that two newly observed transient solar phenomena, EUV macrospicules and X-ray bright-point flares, are closely related. Time-lapse H-alpha filtergram observations of the limb in quiet regions show small surgelike eruptions called H-alpha macrospicules. From the similarity of H-alpha macrospicules and EUV macrospicules, and from comparison of simultaneous H-alpha and He II 304 A observations, we conclude that H-alpha macrospicules are EUV macrospicules viewed in H-alpha, although most EUV macrospicules are too faint in H-alpha to appear on H-alpha filtergrams of normal exposure. From comparison of simultaneous X-ray and H-alpha observations of flares in X-ray bright points situated on the limb, we show that flares in X-ray bright points often produce H-alpha macrospicules.
Document ID
19780030577
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Moore, R. L.
(Hulburt (E. O.) Center for Space Research Washington, DC, United States)
Tang, F.
(Big Bear Solar Observatory Pasadena, Calif., United States)
Bohlin, J. D.
(U.S. Navy, E. O. Hulburt Center for Space Research, Washington D.C., United States)
Golub, L.
(American Science and Engineering, Inc. Cambridge, Mass., United States)
Date Acquired
August 9, 2013
Publication Date
November 15, 1977
Publication Information
Publication: Astrophysical Journal
Subject Category
Solar Physics
Accession Number
78A14486
Funding Number(s)
CONTRACT_GRANT: F19628-76-C-0055
CONTRACT_GRANT: DPR-560404G
CONTRACT_GRANT: NGR-05-002-034
CONTRACT_GRANT: NSF ATM-74-13489
CONTRACT_GRANT: NAS8-27758
Distribution Limits
Public
Copyright
Other

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