Add to ORKGOver two years of data from the Lockheed Plasma Composition Experiment on the ISEE 1 spacecraft, covering ion energies between 100 eV/e and about 16 keV/e, have been analyzed in an attempt to extract new information about three geophysical issues: (1) solar wind penetration of the Earth's magnetic tail; (2) relationship between plasma sheet and tail lobe ion composition; and (3) possible effects of heavy terrestrial ions on plasma sheet stability
Progress is reported in the development of programs for statistical analysis of boundary and structu...
Moments calculated from the ion distributions (~0–40 keV) measured by the Cluster Ion Spectrometry (...
It is likely that after the THEMIS and MMS missions terminate, there will be no satellite dedicated ...
This report covers the initial phase of an investigation that was originally selected by NASA Headqu...
The plasma composition experiment covers energies from OeV to 17 keV/e and has a mass-per-charge ran...
This is a contract under the NASA Supporting Research and Technology Program for the analysis and in...
This serves as a final report entitled Energization and Transport of Ions of Ionospheric Origin in t...
During magnetospheric substorm events, the plasma and ion composition experiments in the ISEE-1 and ...
The structure of the magnetotail plasma sheet-plasma lobe boundary was studied by observing the prop...
Data from energetic ion mass spectrometers on the ISEE 1 and AMPTE/CCE spacecraft are combined with ...
International audienceBy using the data of two spacecraft, TC-1 and ACE (Advanced Composition Explor...
Abstract Solar wind particles and ionospheric O+ ions influence the near-Earth plasma sheet and inne...
A large set of energetic (0.1 to 16 keV/e) ion composition data from the central magnetotail, obtain...
Ion composition data sets from Lockheed instruments on a variety of spacecraft were used in combinat...
International audienceWe study here the injection and transport of ions in the convection-dominated ...
Progress is reported in the development of programs for statistical analysis of boundary and structu...
Moments calculated from the ion distributions (~0–40 keV) measured by the Cluster Ion Spectrometry (...
It is likely that after the THEMIS and MMS missions terminate, there will be no satellite dedicated ...
This report covers the initial phase of an investigation that was originally selected by NASA Headqu...
The plasma composition experiment covers energies from OeV to 17 keV/e and has a mass-per-charge ran...
This is a contract under the NASA Supporting Research and Technology Program for the analysis and in...
This serves as a final report entitled Energization and Transport of Ions of Ionospheric Origin in t...
During magnetospheric substorm events, the plasma and ion composition experiments in the ISEE-1 and ...
The structure of the magnetotail plasma sheet-plasma lobe boundary was studied by observing the prop...
Data from energetic ion mass spectrometers on the ISEE 1 and AMPTE/CCE spacecraft are combined with ...
International audienceBy using the data of two spacecraft, TC-1 and ACE (Advanced Composition Explor...
Abstract Solar wind particles and ionospheric O+ ions influence the near-Earth plasma sheet and inne...
A large set of energetic (0.1 to 16 keV/e) ion composition data from the central magnetotail, obtain...
Ion composition data sets from Lockheed instruments on a variety of spacecraft were used in combinat...
International audienceWe study here the injection and transport of ions in the convection-dominated ...
Progress is reported in the development of programs for statistical analysis of boundary and structu...
Moments calculated from the ion distributions (~0–40 keV) measured by the Cluster Ion Spectrometry (...
It is likely that after the THEMIS and MMS missions terminate, there will be no satellite dedicated ...