An important modification was made in the method for computing ion densities from DE1/RIMS observations, based on the observed relationship between total plasma density and spacecraft potential. An iterative technique was developed to require that this relationship be preserved in all individual observations, not just in the average sense observed. Results of employing this technique were examined closely and are found to generally improve the final densities in terms of agreement with densities obtained from PWI upper hybrid frequency observations. It also has the effect of reducing scatter in the density vs. L profiles
International audienceSpacecraft potential measurements by the EFW electric field experiment on the ...
Simultaneous observations of low energy electrons in the plasma sheet and in the auroral zone were a...
The Retarding Ion Mass Spectrometer (RIMS) on the Dynamics Explorer 1 spacecraft observes both the t...
Analysis techniques and software development, data analysis and modeling, laboratory plasma flow stu...
Methods employed in the analysis of plasmas and the magnetosphere are examined. Computer programs wh...
Temperature and density analysis in the Automated Analysis Program (for the global empirical model) ...
We introduce two novel techniques for estimating temperatures of very low energy space plasmas using...
During the course of this grant, work was performed on a variety of topics and there were a number o...
The density structure of the plasmapause was investigated using the two satellites ISEE-1 and DE-2 t...
This experimental study shows the validity of Sheridan’s method in determining plasma density in low...
The Thermal Ion Dynamics Experiment (TIDE) and the Plasma Source Instrument (PSI) have been develope...
Radio frequency emission has been detected near the power hybrid frequency of a bumpy torus plasma b...
The Plasma Science Experiment (PLS) on the Voyager spacecraft provide data on the plasma ions and el...
It is likely that after the THEMIS and MMS missions terminate, there will be no satellite dedicated ...
Thermal plasmaspheric densities and temperatures for five ion species have recently become available...
International audienceSpacecraft potential measurements by the EFW electric field experiment on the ...
Simultaneous observations of low energy electrons in the plasma sheet and in the auroral zone were a...
The Retarding Ion Mass Spectrometer (RIMS) on the Dynamics Explorer 1 spacecraft observes both the t...
Analysis techniques and software development, data analysis and modeling, laboratory plasma flow stu...
Methods employed in the analysis of plasmas and the magnetosphere are examined. Computer programs wh...
Temperature and density analysis in the Automated Analysis Program (for the global empirical model) ...
We introduce two novel techniques for estimating temperatures of very low energy space plasmas using...
During the course of this grant, work was performed on a variety of topics and there were a number o...
The density structure of the plasmapause was investigated using the two satellites ISEE-1 and DE-2 t...
This experimental study shows the validity of Sheridan’s method in determining plasma density in low...
The Thermal Ion Dynamics Experiment (TIDE) and the Plasma Source Instrument (PSI) have been develope...
Radio frequency emission has been detected near the power hybrid frequency of a bumpy torus plasma b...
The Plasma Science Experiment (PLS) on the Voyager spacecraft provide data on the plasma ions and el...
It is likely that after the THEMIS and MMS missions terminate, there will be no satellite dedicated ...
Thermal plasmaspheric densities and temperatures for five ion species have recently become available...
International audienceSpacecraft potential measurements by the EFW electric field experiment on the ...
Simultaneous observations of low energy electrons in the plasma sheet and in the auroral zone were a...
The Retarding Ion Mass Spectrometer (RIMS) on the Dynamics Explorer 1 spacecraft observes both the t...