Ground and space observations of medium frequency auroral radio emissions

2014 ◽  
Author(s):  
Matthew C. Broughton
Keyword(s):  
Medium Frequency ◽  
Radio Emissions ◽  
Space Observations

A medium-frequency interferometer for studying auroral radio emissions

2000 ◽  
Vol 71 (8) ◽  
pp. 3200-3206 ◽  
Author(s):  
J. M. Hughes ◽  
J. LaBelle ◽  
M. L. Trimpi
Keyword(s):  
Medium Frequency ◽  
Radio Emissions

scholarly journals Experimental tests of the generation mechanism of auroral medium frequency burst radio emissions

2009 ◽  
Vol 114 (A9) ◽  
pp. n/a-n/a ◽  
Author(s):  
N. L. Bunch ◽  
J. LaBelle ◽  
A. T. Weatherwax ◽  
J. M. Hughes ◽  
D. Lummerzheim
Keyword(s):  
Experimental Tests ◽  
Generation Mechanism ◽  
Medium Frequency ◽  
Radio Emissions ◽  
Frequency Burst

scholarly journals Experimental tests of a topside generation mechanism for auroral medium frequency radio emissions

2012 ◽  
Vol 117 (A12) ◽  
pp. n/a-n/a ◽  
Author(s):  
M. C. Broughton ◽  
J. LaBelle ◽  
G. T. Roberg-Clark ◽  
M. McCready ◽  
N. L. Bunch
Keyword(s):  
Experimental Tests ◽  
Generation Mechanism ◽  
Medium Frequency ◽  
Radio Emissions

Theoretical constraints on the generation mechanism of auroral medium frequency burst radio emissions

2011 ◽  
Vol 116 (A1) ◽  
pp. n/a-n/a ◽  
Author(s):  
Nicholas L. Bunch ◽  
James LaBelle ◽  
Peter Yoon ◽  
Allan T. Weatherwax
Keyword(s):  
Generation Mechanism ◽  
Medium Frequency ◽  
Radio Emissions ◽  
Frequency Burst

Ground-level detection of low- and medium-frequency auroral radio emissions

1988 ◽  
Vol 93 (A1) ◽  
pp. 277 ◽  
Author(s):  
Robert F. Benson ◽  
Michael D. Desch ◽  
Robert D. Hunsucker ◽  
Gerald J. Romick
Keyword(s):  
Ground Level ◽  
Medium Frequency ◽  
Radio Emissions

Some Problems in Understanding the Solar Corona

1994 ◽  
Vol 144 ◽  
pp. 1-9
Author(s):  
A. H. Gabriel
Keyword(s):  
Solar Corona ◽  
Solar Atmosphere ◽  
Theoretical Modelling ◽  
Total System ◽  
Major Advance ◽  
X Ray ◽  
Proper Perspective ◽  
Space Observations

The development of the physics of the solar atmosphere during the last 50 years has been greatly influenced by the increasing capability of observations made from space. Access to images and spectra of the hotter plasma in the UV, XUV and X-ray regions provided a major advance over the few coronal forbidden lines seen in the visible and enabled the cooler chromospheric and photospheric plasma to be seen in its proper perspective, as part of a total system. In this way space observations have stimulated new and important advances, not only in space but also in ground-based observations and theoretical modelling, so that today we find a well-balanced harmony between the three techniques.

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