An investigation of electron acceleration in the auroral precipitation region of the magnetosphere is made. In particular a determination of the mechanisms that could produce the observed power law distribution in energy and the positive slope in the distribution function are described
<p>Precipitating auroral electrons are believed to originate mainly from parallel electric fields se...
Electron precipitation observed by DMSP is categorized into five fundamental types in relation to it...
We propose to examine the relationship of geomagnetic storms and substorms and the transport of ener...
This paper discusses the major pathways of electron distribution function formation in the region of...
A review of recent observational and theoretical results on the problem of auroral particle accelera...
The precipitation of high-energy magnetospheric electrons (E greater than 500-600 electronvolts) in ...
Measurements with satellite and sounding rocket borne instruments contain important information on r...
Data from simultaneous observations (on 13 February 1996, 9 November 1998, and 12 February 1999) w...
Aurora is caused by the precipitation of energetic particles in a planetary atmosphere, the light in...
The relations between average energy and total energy flux of incident electrons are examined for th...
Vita.Low-energy particle measurements by the Soft Particle Spectrometer on the ISIS-1 polar orbiting...
We propose a simple explanation of the prolonged existence of pancake-like electron velocity distri...
Vita.Low-energy particle measurements by the Soft Particle Spectrometer on the ISIS-1 polar orbiting...
This study is a statistical analysis on energy distribution of precipitating electrons, based on CN...
Electron auroras are theoretically investigated by using the Monte Carlo method. The MSIS-86 model i...
<p>Precipitating auroral electrons are believed to originate mainly from parallel electric fields se...
Electron precipitation observed by DMSP is categorized into five fundamental types in relation to it...
We propose to examine the relationship of geomagnetic storms and substorms and the transport of ener...
This paper discusses the major pathways of electron distribution function formation in the region of...
A review of recent observational and theoretical results on the problem of auroral particle accelera...
The precipitation of high-energy magnetospheric electrons (E greater than 500-600 electronvolts) in ...
Measurements with satellite and sounding rocket borne instruments contain important information on r...
Data from simultaneous observations (on 13 February 1996, 9 November 1998, and 12 February 1999) w...
Aurora is caused by the precipitation of energetic particles in a planetary atmosphere, the light in...
The relations between average energy and total energy flux of incident electrons are examined for th...
Vita.Low-energy particle measurements by the Soft Particle Spectrometer on the ISIS-1 polar orbiting...
We propose a simple explanation of the prolonged existence of pancake-like electron velocity distri...
Vita.Low-energy particle measurements by the Soft Particle Spectrometer on the ISIS-1 polar orbiting...
This study is a statistical analysis on energy distribution of precipitating electrons, based on CN...
Electron auroras are theoretically investigated by using the Monte Carlo method. The MSIS-86 model i...
<p>Precipitating auroral electrons are believed to originate mainly from parallel electric fields se...
Electron precipitation observed by DMSP is categorized into five fundamental types in relation to it...
We propose to examine the relationship of geomagnetic storms and substorms and the transport of ener...
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