Skip to search formSkip to main contentSkip to account menu
PEACE: A PLASMA ELECTRON AND CURRENT EXPERIMENT
An electron analyser to measure the three-dimensional velocity distribution of electrons in the energy range from 0.59 eV to 26.4 keV on the four spacecraft of the Cluster mission is described. The…
View on Springer
Corotating solar wind streams and recurrent geomagnetic activity: A review
[1] Solar wind fast streams emanating from solar coronal holes cause recurrent, moderate intensity geomagnetic activity at Earth. Intense magnetic field regions called Corotating Interaction Regions…
View via Publisher
The Cassini Cosmic Dust Analyzer
The Cassini-Huygens Cosmic Dust Analyzer (CDA) is intended to provide direct observations of dust grains with masses between 10−19 and 10−9 kg in interplanetary space and in the jovian and saturnian…
View on Springer
The Analyser of Space Plasmas and Energetic Atoms (ASPERA-4) for the Venus Express mission
View via Publisher
Composition and Dynamics of Plasma in Saturn's Magnetosphere
TLDR
Over the A and B rings, an ionosphere in which O2+ and O+ are dominant is found, which suggests the possible existence of a layer of O2 gas similar to the atmospheres of Europa and Ganymede.
View on Publisher
Cassini Plasma Spectrometer Investigation
The Cassini Plasma Spectrometer (CAPS) will make comprehensive three-dimensional mass-resolved measurements of the full variety of plasma phenomena found in Saturn’s magnetosphere. Our fundamental…
View on SPIE
The Analyzer of Space Plasmas and Energetic Atoms (ASPERA-3) for the Mars Express Mission
The general scientific objective of the ASPERA-3 experiment is to study the solar wind – atmosphere interaction and to characterize the plasma and neutral gas environment with within the space near…
View on Springer
Current understanding of magnetic storms: storm-substorm relationships
This paper attempts to summarize the current understanding of the storm/substorm relationship by clearing up a considerable amount of controversy and by addressing the question of how solar wind…
View via Publisher
A soft solid surface on Titan as revealed by the Huygens Surface Science Package
TLDR
Measurements made just above and on the surface of Titan by the Huygens Surface Science Package reveal a relatively smooth, but not completely flat, surface surrounding the landing site.
View on Springer
The loss of ions from Venus through the plasma wake
TLDR
Measurements of the atmosphere of Venus show that the dominant escaping ions are O+, He+ and H+.
View on Nature
...
...
By clicking accept or continuing to use the site, you agree to the terms outlined in our Privacy Policy, Terms of Service, and Dataset License