Group travel time for proton whistlers in the ionosphere
Description
A theoretical relation is derived for the group travel time of the proton whistlers to reach the satellite from their place of occurrence. The expression for the group travel time contains two terms. The first term is the dominant term and is inversely proportional to (Ω - ω)/sup 1/2/, where Ω and ω are the proton gyrofrequency and the wave frequency, respectively. The contribution from the second term, which is inversely proportional to (Ω - ω)/sup 7/2/, is about 10 percent of the first term. It is shown that the group travel time is sensitive to the variation of temperature, gradient of proton gyrofrequency, and ion density along the path of a proton whistler. The effect of variation in each of the above parameters on the group travel time is discussed, and it is shown that an estimate of proton temperature can be made from the measured data on the proton whistlers. (U.S.)
Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Geophysical Research
- Journal Volume
- 80
- Journal Issue
- 4
- Series
- J. Geophys. Res.
- Journal Page Range
- 694-695
- ISSN
- 0148-0227
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 6215063
- Subject category
- S58: GEOSCIENCES;
- Descriptors DEI
- GYROFREQUENCY; ION DENSITY; IONOSPHERE; PROTON TEMPERATURE; PROTONS; SPATIAL DISTRIBUTION; TIME-OF-FLIGHT METHOD; TRAVELLING IONOSPHERIC DISTURB; WHISTLERS
- Descriptors DEC
- BARYONS; CATIONS; CHARGED PARTICLES; DISTRIBUTION; DISTURBANCES; EARTH ATMOSPHERE; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; FERMIONS; HADRONS; HYDROGEN IONS; HYDROGEN IONS 1 PLUS; IONS; NOISE; NUCLEONS; RADIATIONS; RADIO NOISE; RADIOWAVE RADIATION
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent