SWE, a comprehensive plasma instrument for the WIND spacecraft
@article{Ogilvie1995SWEAC, title={SWE, a comprehensive plasma instrument for the WIND spacecraft}, author={Keith W. Ogilvie and D. Chornay and R. J. Fritzenreiter and Floyd H. Hunsaker and J. W. Keller and J. Lobell and G. Miller and J. D. Scudder and Edward C. Sittler and Roy B. Torbert and D. Bodet and Gerald Needell and Alan J. Lazarus and J. T. Steinberg and John H. Tappan and A. Mavretic and E. Gergin}, journal={Space Science Reviews}, year={1995}, volume={71}, pages={55-77} }
The Solar Wind Experiment (SWE) on the WIND spacecraft is a comprehensive, integrated set of sensors which is designed to investigate outstanding problems in solar wind physics. It consists of two Faraday cup (FC) sensors; a vector electron and ion spectrometer (VEIS); a strahl sensor, which is especially configured to study the electron ‘strahl’ close to the magnetic field direction; and an on-board calibration system. The energy/charge range of the Faraday cups is 150 V to 8 kV, and that of…
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References
SHOWING 1-10 OF 10 REFERENCES
The plasma experiment on the 1977 Voyager Mission
- Physics
- 1977
This paper contains a brief description of the plasma experiment to be flown on the 1977 Voyager Mission, its principal scientific objectives, and the expected results.The instrument consists of two…
The Electron Spectrometer Experiment on ISEE-1
- PhysicsIEEE Transactions on Geoscience Electronics
- 1978
A six-axis electron spectrometer for the ISEE-1 spacecraft is described and some typical early results presented. This instrument, designed for three-dimensional plasma distribution function studies…
Kinetic Physics of the Solar Wind Plasma
- Physics
- 1991
The interplanetary medium has been continuously explored for more than two decades and substantial progress has been made, both with regard to in situ measurements and a theoretical understanding of…
Solar wind conditions in the outer heliosphere and the distance to the termination shock
- Physics
- 1993
The Plasma Science experiment on the Voyager 2 spacecraft has measured to date the properties of solar wind protons from 1 to 40.4 AU. We use these observations to discuss the probable location and…
A theory of local and global processes which affect solar wind electrons 2. Experimental support
- Physics
- 1979
We have extended the theoretical considerations of Scudder and Olbert (1979) (hereafter called paper 1) to show from the microscopic characteristics of the Coulomb cross section that there are three…
Experimental tests of a toroidal electrostatic analyzer
- Physics
- 1987
A toroidal electrostatic analyzer of a design suitable for space plasma instrumentation has been constructed and tested. Experimental results are compared with second-order ion optical theory and are…
A theory of local and global processes which affect solar wind electrons, 1. The origin of typical 1 AU velocity distribution functions—Steady state theory
- Physics
- 1979
A new detailed first principle kinetic theory for electrons is presented which is neither a classical fluid treatment nor an expospheric calculation. This new theory illustrates the global and local…