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Preliminary results of a balloon flight of the solar disk sextantPreliminary results of a balloon flight on October 11, 1991, of the solar disk sextant (SDS) experiment are reported. The SDS is an instrument which measures the solar diameter at different orientations with respect to the solar polar axis. Fitting straight lines through two fixed-angle data sets with time as the independent variable yields slopes of (7.1 +/ - 1.5) x 10 exp -3 and (6.7 +/- 1.6) x 10 exp -3/mas s, consistent with the value of 6.47 x 10 exp -3/mas s expected from the earth's approach to the sun due to the orbital motion toward perihelion. Upon the instrument's rotation on its axis a sinusoidal component of the diameter measurement was observed in each rotation cycle, with a variable amplitude of about 150 mas. The present result is epsilon of (5.6 +/- 6.3) x 10 exp -6, about 30 deg offset from the polar-equator position. The absolute diameter obtained by means of the FFT definition is found to be 1919.269 +/- 0.240 arcsec or 1919.131 +/- 0.240 arcsec, depending on the orientation mode of the measurement.
Document ID
19920050464
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Maier, E.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Twigg, L.
(Applied Research Corp. Landover, MD, United States)
Sofia, S.
(Yale University New Haven, CT, United States)
Date Acquired
August 15, 2013
Publication Date
April 10, 1992
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 389
ISSN: 0004-637X
Subject Category
Solar Physics
Accession Number
92A33088
Funding Number(s)
CONTRACT_GRANT: NAG5-736
CONTRACT_GRANT: AF-AFOSR-91-0053
Distribution Limits
Public
Copyright
Other

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