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Time development of a small solar X-ray burstThe 5.1-7.2 A X-ray emission from the sun was studied via OSO-8 with a high-resolution PET crystal spectrometer during the week of 17 November 1975, when the sun was active. The combination of good temporal and spectral resolution permitted the analysis of the data with multithermal coronal models over the course of a small X-ray burst.
Document ID
19760062970
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Cohen, G. G. (Columbia Univ. New York, NY, United States)
Kestenbaum, H. L. (Columbia Univ. New York, NY, United States)
Long, K. S. (Columbia Univ. New York, NY, United States)
Novick, R. (Columbia Univ. New York, NY, United States)
Weisskopf, M. C. (Columbia Univ. New York, NY, United States)
Wolff, R. S. (Columbia University New York, N.Y., United States)
Date Acquired
August 8, 2013
Publication Date
June 1, 1976
Subject Category
Solar Physics
Meeting Information
Meeting: COSPAR, Plenary Meeting
Location: Philadelphia, PA
Start Date: June 8, 1976
End Date: June 19, 1976
Sponsors: COSPAR
Accession Number
76A45936
Funding Number(s)
CONTRACT_GRANT: NAS5-22408
Distribution Limits
Public
Copyright
Other

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