scholarly journals Analysis of Long-Periodic Fluctuations of Solar Microwave Radiation, as a Way for Diagnostics of Coronal Magnetic Loops Dynamics

10.5772/36919 ◽  
2012 ◽  
Author(s):  
Maxim L. ◽  
Albert G. ◽  
Eugeny I.
Keyword(s):  
Microwave Radiation ◽  
Coronal Magnetic Loops ◽  
Solar Microwave ◽  
Periodic Fluctuations

Unusual preflare modulation of microwave radiation in coronal magnetic loops

2011 ◽  
Vol 54 (4) ◽  
pp. 219-234 ◽  
Author(s):  
V. V. Zaitsev ◽  
K. G. Kislyakova ◽  
A. T. Altyntsev ◽  
N. S.Meshalkina
Keyword(s):  
Microwave Radiation ◽  
Coronal Magnetic Loops

scholarly journals Simulated Solar Microwave Radiation Blocks the Formation of Biofilms

2015 ◽  
Vol 07 (03) ◽  
pp. 127-131 ◽  
Author(s):  
Yulia S. Shishkova ◽  
Stanislav N. Darovskih ◽  
Nadezhda V. Vdovina ◽  
Nadezhda L. Pozdnyakova ◽  
I. A. Komarova ◽  
...  
Keyword(s):  
Microwave Radiation ◽  
Solar Microwave

Imaging spectroscopy of solar microwave radiation. 1: Flaring emission

1994 ◽  
Vol 430 ◽  
pp. 425 ◽  
Author(s):  
Jeremy Lim ◽  
Dale E. Gary ◽  
Gordon J. Hurford ◽  
James R. Lemen
Keyword(s):  
Microwave Radiation ◽  
Imaging Spectroscopy ◽  
Solar Microwave

scholarly journals 48. The radial brightness distribution of the sun at 9·4 cm.

1957 ◽  
Vol 4 ◽  
pp. 273-278
Author(s):  
F. T. Haddock
Keyword(s):  
Microwave Radiation ◽  
Research Laboratory ◽  
Wave Length ◽  
Brightness Distribution ◽  
Naval Research Laboratory ◽  
Naval Research ◽  
The Sun ◽  
Eclipse Observation ◽  
Centre Line ◽  
Solar Microwave

The Naval Research Laboratory has supported four eclipse expeditions (in the years 1947, 1950, 1952 and 1954) under the direction of Dr J. P. Hagen. The principal purpose was to find the variation of the solar microwave radiation during a total optical eclipse of the sun. During the last two eclipses the sun was sufficiently inactive to enable us to derive the centre-to-limb brightness distribution at a wave-length of 9·4 cm., on the assumption that the distribution was circularly symmetrical. Since these two eclipses were of the same optical magnitude (within 0·12 %) and were measured with the same equipment located at each eclipse near the centre-line of mid-totality, it is of interest to compare their results. The 1954 eclipse observation was described in the last paper by Mayer, Sloanaker and Hagen. The 1952 observation has already been described [1].

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