Ionospheric outflow of plasma and compression relationship in the plasma sheet
Description
The authors are concerned in this article with the curious finding of Huang et al. [1989] which suggests a polytropic index of plasma compression of about 0.7 in the quiet time central plasma sheet. They show that the reduction of this index from its adiabatic value (=5/3) can be achieved through an ionospheric outflow of plasma which lowers the plasma temperature by virtue of energy partition. The observed correlation between the plasma temperature and density is best reproduced by an ionospheric source of ∼5x1025 ions/s, consistent with independent experimental estimates and smaller than the average solar wind source by a factor of two or more. Despite the change in the polytropic relationship, they find that the global energy equation PV5/3=constant (V=volume of a unit flux tube) still holds approximately (in the absence of other energy-loss mechanisms)
Additional details
Publishing Information
- Journal Title
- Geophysical Research Letters
- Journal Volume
- 17
- Journal Issue
- 11
- Series
- Geophys. Res. Lett.
- Journal Page Range
- 1849-1852
- ISSN
- 0094-8276
- CODEN
- GPRLA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 22080188
- Subject category
- S58: GEOSCIENCES;
- Descriptors DEI
- ADIABATIC PROCESSES; COLD PLASMA; COMPRESSION; CONVECTION; CORRELATIONS; EQUATIONS; HOT PLASMA; HYDROGEN IONS 1 PLUS; ION DRIFT; IONOSPHERE; MAGNETIC FLUX; ORIGIN; PLASMA DENSITY; PLASMA DRIFT; PLASMA SHEET; SOLAR WIND
- Descriptors DEC
- CATIONS; CHARGED PARTICLES; EARTH ATMOSPHERE; ENERGY TRANSFER; HEAT TRANSFER; HYDROGEN IONS; IONS; PLASMA; SOLAR ACTIVITY; STELLAR ACTIVITY; STELLAR WINDS