Meter and decameter wavelength positions of solar bursts of July 31?August 7, 1972

Solar Physics ◽  
1974 ◽  
Vol 36 (1) ◽  
pp. 179-189 ◽  
Author(s):  
M. R. Kundu ◽  
W. C. Erickson
Keyword(s):  
Decameter Wavelength ◽  
Solar Bursts

scholarly journals Meter and Decameter Wavelength Positions of Solar Radio Bursts of July 31–August 7, 1972

1974 ◽  
Vol 57 ◽  
pp. 231-233
Author(s):  
M. R. Kundu ◽  
W. C. Erickson
Keyword(s):  
Solar Phys ◽  
Solar Radio ◽  
Base Line ◽  
Radio Bursts ◽  
Frequency Range ◽  
Solar Radio Bursts ◽  
Spiral Antennas ◽  
Positional Analysis ◽  
Decameter Wavelength ◽  
Solar Bursts

(Solar Phys.). The positional analysis of solar bursts at meter and decameter wavelengths during the period July 31–August 7, 1972 is presented. The observations were taken with two arrays – a log periodic array of 16 elements situated on an E–W base line of 3.3 km and portions of the new Clark Lake array in the form of a Tee (an E–W arm of 32 log spiral antennas and a N–S arm of 16 similar antennas). The new array operates over the frequency range 10–120 MHz and has angular resolutions of approximately 3.′5 at 100 MHz and 8.′5 at 40 MHz in the E–W direction.

Source characteristics of main and post-burst-increase phases of solar bursts at 17 GHz

Solar Physics ◽  
1983 ◽  
Vol 87 (2) ◽  
Author(s):  
Takeo Kosugi ◽  
Keizo Kai ◽  
Takashi Suzuki
Keyword(s):  
Source Characteristics ◽  
Solar Bursts

scholarly journals Nonlinear analysis of decimetric solar bursts

2009 ◽  
Vol 5 (S264) ◽  
pp. 279-281
Author(s):  
Reinaldo R. Rosa ◽  
Mauricio J. A. Bolzan ◽  
Francisco C. R. Fernandes ◽  
H. S. Sawant ◽  
Marian Karlický
Keyword(s):  
Solar Radio ◽  
Inhomogeneous Plasma ◽  
Active Regions ◽  
Singularity Spectrum ◽  
Frequency Range ◽  
Radio Emissions ◽  
Magnetic Structures ◽  
Fine Structures ◽  
Solar Bursts ◽  
Solar Radio Emissions

AbstractThe solar radio emissions in the decimetric frequency range (above 1 GHz) are very rich in temporal and spectral fine structures due to nonlinear processes occurring in the magnetic structures on the corresponding active regions. In this paper we characterize the singularity spectrum, f(α), for solar bursts observed at 1.6, 2.0 and 3 GHz. We interpret our findings as evidence of inhomogeneous plasma turbulence driving the underlying plasma emission process and discuss the nonlinear multifractal approach into the context of geoeffective solar active regions.

Interplanetary-particle associations with type III solar bursts

1971 ◽  
Vol 76 (28) ◽  
pp. 6932-6938 ◽  
Author(s):  
T. E. Graedel ◽  
L. J. Lanzerotti
Keyword(s):  
Type Iii ◽  
Solar Bursts

Earliest recorded ground-based decameter wavelength observations of Saturn’s lightning during the giant E-storm detected by Cassini spacecraft in early 2006

Icarus ◽  
2013 ◽  
Vol 224 (1) ◽  
pp. 14-23 ◽  
Author(s):  
A.A. Konovalenko ◽  
N.N. Kalinichenko ◽  
H.O. Rucker ◽  
A. Lecacheux ◽  
G. Fischer ◽  
...  
Keyword(s):  
Decameter Wavelength ◽  
Cassini Spacecraft

Spectral Trends of Solar Bursts at Sub-THz Frequencies

Solar Physics ◽  
2017 ◽  
Vol 292 (1) ◽  
Author(s):  
L. O. T. Fernandes ◽  
P. Kaufmann ◽  
E. Correia ◽  
C. G. Giménez de Castro ◽  
A. S. Kudaka ◽  
...  
Keyword(s):  
Solar Bursts

scholarly journals Attenuation of decameter wavelength sky noise during x-ray solar flares in 2013–2017 based on the observations of midlatitude HF radars

2018 ◽  
Vol 173 ◽  
pp. 1-13 ◽  
Author(s):  
O.I. Berngardt ◽  
J.M. Ruohoniemi ◽  
N. Nishitani ◽  
S.G. Shepherd ◽  
W.A. Bristow ◽  
...  
Keyword(s):  
Solar Flares ◽  
X Ray ◽  
Decameter Wavelength
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