Issue |
Europhys. Lett.
Volume 59, Number 4, August 2002
|
|
---|---|---|
Page(s) | 626 - 632 | |
Section | Geophysics, astronomy, and astrophysics | |
DOI | https://doi.org/10.1209/epl/i2002-00150-y | |
Published online | 01 August 2002 |
Global ionospheric -layer height monitoring
1
Institut für Meteorologie und Geophysik
- Feldberg straße 47 D-60323 Frankfurt am Main, Germany
2
STAR Laboratory
- Stanford University, Stanford, CA 94305, USA
3
Max-Planck Institut für Aeronomie
- Max-Planck Straße 2 D-37191 Katlenburg-Lindau, Germany
Received:
15
February
2002
Accepted:
27
May
2002
A global two-scale height ionospheric conductivity profile is inferred from the mean electromagnetic-wave propagation velocities of seven Earth-ionosphere cavity resonances in the frequency range . The time-varying reflection height for the electromagneticwaves is monitored on a diurnal basis. This D-layer height exhibits an increase at solar quiet conditions associated with decreased ionisation at mesospheric altitudes from solar short-wave radiation during the solar cycle and the solar rotation period. It is concluded that it is possible to monitor the global ionospheric D-layer heightvariability with naturally occurring electromagnetic waves in the atmosphere. A small network of magnetometers may detect and locate large-scale remote areas of mesospheric conductivity profile perturbations from short-lived extraterrestrial ionisation sources in the South Atlantic geomagnetic field anomaly, which are an appreciated hazard to spacecraft operation.
PACS: 94.20.Ee – D region / 52.35.Hr – Electromagnetic waves (e.g., electron-cyclotron, Whistler, Bernstein, upper hybrid, lower hybrid) / 41.20.Jb – Electromagnetic wave propagation; radiowave propagation
© EDP Sciences, 2002
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