k vector measurements of VLF signals by the satellite EXOS-D

Details k vector measurements of VLF signals by the satellite EXOS-D k vector measurements of VLF signals by the satellite EXOS-D

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991georl..18..325y&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 18, Feb. 1991, p. 325-328.

Physics

1

Exos Satellites, Exos-D Satellite, Very Low Frequencies, Geomagnetism, Poynting Theorem, Refractivity

Scientific paper

This paper presents the results of determinations of the wave normal, or k vector, and the Poynting vector directions of VLF and ELF emissions, using data from the PFX receiver subsystem of VLF instruments aboard the EXOS-D satellite to measure two components of E and three components of B fields. It is shown that, using the Means (1972) method, the PFX subsystem can determine reasonably well the direction of the k vector and Poynting vector of coherent VLF signals. The refractive index deduced from the E and B fields agreed well with the refractive index calculated by the Appleton Hartree formula.

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