The electrostatic probe experiment aboard the ISIS-1 satellite detects a quasi-stable dayside plasma trough in the protonosphere with a characteristic time of at least 2 weeks. This behavior contrasts with measurements at 1000 km from Explorer-22, which indicate a trough of a characteristic time less than a satellite orbit period. Associated with the protonospheric trough is an electron temperature maximum approximately 6000 K that is sharp at midnight and broad at noon. In spring and summer, a second noontime temperature maximum often appears poleward of 70 invariant latitude, accompanied by an enhancement in the ionization. The ISIS-1 data indicates that local processes such as dayside F-region photoionization and ionization by energetic ...
Models of ion flow in the topside ionosphere were developed. These models took both H(+) and O(+) in...
International audienceThe dayside high-latitude trough is a persistent feature of the post-noon wint...
The Earth’s plasmasphere variability is a consequence of the Sun’s forcing, determining our planet’s...
Observations of the electron concentration, N sub e, and temperature, T sub e, from the electrostati...
The ion mass spectrometer (IMS) on the ISIS-II satellite is described; it measures the composition a...
Magnetosheath plasma penetrating to low altitudes in the dayside cusp region of the magnetosphere ha...
Light ion trough measurements near midnight made by the RF ion mass spectrometer on OGO-4 operating ...
The structure of the plasmasphere was studied as seen by radiosounder measurements aboard the Alovet...
International audienceTomographic imaging provides a powerful technique for obtaining images of the ...
During August 1972, Explorer 45 orbiting near the equatorial plane with an apogee of about 5.2 R sub...
Thermal H+ distributions have been measured as the European Space Agency GEOS-1 satellite passed thr...
Langmuir probe data from Isis-1 satellite are used to study the latitudinal profiles of electron tem...
International audienceA combination of EISCAT CP-3 (latitude scans) and satellite (DMSP) data have b...
The radar sounder on the Mars Express Spacecraft is able to make measurements of electron densities ...
The upper atmosphere of the Earth is ionised by electromagnetic radiation and energetic charged part...
Models of ion flow in the topside ionosphere were developed. These models took both H(+) and O(+) in...
International audienceThe dayside high-latitude trough is a persistent feature of the post-noon wint...
The Earth’s plasmasphere variability is a consequence of the Sun’s forcing, determining our planet’s...
Observations of the electron concentration, N sub e, and temperature, T sub e, from the electrostati...
The ion mass spectrometer (IMS) on the ISIS-II satellite is described; it measures the composition a...
Magnetosheath plasma penetrating to low altitudes in the dayside cusp region of the magnetosphere ha...
Light ion trough measurements near midnight made by the RF ion mass spectrometer on OGO-4 operating ...
The structure of the plasmasphere was studied as seen by radiosounder measurements aboard the Alovet...
International audienceTomographic imaging provides a powerful technique for obtaining images of the ...
During August 1972, Explorer 45 orbiting near the equatorial plane with an apogee of about 5.2 R sub...
Thermal H+ distributions have been measured as the European Space Agency GEOS-1 satellite passed thr...
Langmuir probe data from Isis-1 satellite are used to study the latitudinal profiles of electron tem...
International audienceA combination of EISCAT CP-3 (latitude scans) and satellite (DMSP) data have b...
The radar sounder on the Mars Express Spacecraft is able to make measurements of electron densities ...
The upper atmosphere of the Earth is ionised by electromagnetic radiation and energetic charged part...
Models of ion flow in the topside ionosphere were developed. These models took both H(+) and O(+) in...
International audienceThe dayside high-latitude trough is a persistent feature of the post-noon wint...
The Earth’s plasmasphere variability is a consequence of the Sun’s forcing, determining our planet’s...