Imaging spectroscopy of solar microwave radiation. 1: Flaring emission

A Thermal Origin of the Postburst Increases of Solar Microwave Radiation

The Solar Corona ◽

10.1016/b978-1-4832-2872-3.50022-x ◽

1963 ◽

pp. 143-149 ◽

Cited By ~ 4

Author(s):

KIN-AKI KAWABATA

Keyword(s):

Microwave Radiation ◽

Thermal Origin ◽

Solar Microwave

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Low-frequency modulations in the solar microwave radiation as a possible indicator of inductive interaction of coronal magnetic loops

Astronomy and Astrophysics ◽

10.1051/0004-6361:20041988 ◽

2005 ◽

Vol 433 (2) ◽

pp. 691-699 ◽

Cited By ~ 12

Author(s):

M. L. Khodachenko ◽

V. V. Zaitsev ◽

A. G. Kislyakov ◽

H. O. Rucker ◽

S. Urpo

Keyword(s):

Microwave Radiation ◽

Low Frequency ◽

Coronal Magnetic Loops ◽

Inductive Interaction ◽

Solar Microwave ◽

Frequency Modulations

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Simulated Solar Microwave Radiation Blocks the Formation of Biofilms

Natural Science ◽

10.4236/ns.2015.73014 ◽

2015 ◽

Vol 07 (03) ◽

pp. 127-131 ◽

Cited By ~ 1

Author(s):

Yulia S. Shishkova ◽

Stanislav N. Darovskih ◽

Nadezhda V. Vdovina ◽

Nadezhda L. Pozdnyakova ◽

I. A. Komarova ◽

...

Keyword(s):

Microwave Radiation ◽

Solar Microwave

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

Fourier Transform Applications ◽

10.5772/36919 ◽

2012 ◽

Author(s):

Maxim L. ◽

Albert G. ◽

Eugeny I.

Keyword(s):

Microwave Radiation ◽

Coronal Magnetic Loops ◽

Solar Microwave ◽

Periodic Fluctuations

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Cyclotron Line in Solar Microwave Radiation by Radio Telescope RATAN-600 Observations of the Solar Active Region NOAA 12182

Geomagnetism and Aeronomy ◽

10.1134/s0016793217070167 ◽

2017 ◽

Vol 57 (7) ◽

pp. 896-901

Author(s):

N. G. Peterova ◽

N. A. Topchilo

Keyword(s):

Active Region ◽

Microwave Radiation ◽

Radio Telescope ◽

Solar Active Region ◽

Active Region Noaa ◽

Solar Microwave ◽

Region Noaa ◽

Cyclotron Line

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SPATIO-SPECTRAL MAXIMUM ENTROPY METHOD: II. SOLAR MICROWAVE IMAGING SPECTROSCOPY

Journal of The Korean Astronomical Society ◽

10.5303/jkas.2005.38.4.445 ◽

2005 ◽

Vol 38 (4) ◽

pp. 445-462 ◽

Cited By ~ 2

Author(s):

Su-Chan Bong ◽

Jeong-Woo Lee ◽

Dale E. Gary ◽

Hong-Sik Yun ◽

Jong-Chul Chae

Keyword(s):

Maximum Entropy ◽

Maximum Entropy Method ◽

Imaging Spectroscopy ◽

Entropy Method ◽

Microwave Imaging ◽

Spectral Maximum ◽

Solar Microwave

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

Symposium - International Astronomical Union ◽

10.1017/s0074180900049238 ◽

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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