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DTIC ADA1026821: Radio Studies of Coronal Holes.
by Defense Technical Information Center
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This report describes all the projects undertaken during
the entire period of the above contract, the scope of
which was to study coronal holes at radio wavelengths.
Chapters 1, 2 and 3 summarize work that has already been
described in our previous scientific reports and
published papers. Chapters 4 and 5 and comprehensive
descriptions of the more recent work that has not been
previously published. Chapter 1 describes the
determination of the radio spectrum (relative changes in
the brightness temperatures at different radio
wavelengths) of Coronal Hole 1 in the Stanford 9.1 cm
synoptic charts during the same period, when clear X-ray
data of coronal holes were available from Skylab. Chapter
2 summarizes our efforts to identify individual high
latitude. Chapter 3 describes our 1977 coronal hole
observations with the Haystack (1.94 and 3.81 cm) and
Arecibo (11.5 and 21.4 cm) radio telescopes. Chapter 4
describes the international effort we organized in the
summer of 1978 to obtain solar radio maps over a wide
range of wavelengths. These radio maps were made on the
same days at a number of radio observatories around the
world. Chapter 5 describes the use of the observed radio
spectra to produce models of the solor atmosphere inside
coronal holes. The results of this analysis indicate that
inside coronal holes the following changes occur: The
chromosphere expands in height by about a factor of 2,
while the temperatures and electron and neutral particle
densities decrease to about 80% of their quiet sun
values. The critical transition zone expands by a factor
of about 5-6, while the temperatures decrease to about
50% and the electron densities to about 20% of their
quiet sun values.
Date Published: 2020-02-14 00:04:40
Identifier: DTIC_ADA1026821
Item Size: 58494813
Language: english
Media Type: texts
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DTIC Archive; Papagiannis,Michael D ;...
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