VLF phase and amplitude: daytime ionospheric parameters

By Wayne M. McRae, N. Thomson. 2000

159 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/d0fda918b4fbe7692d44ad4c4545d9e981ed5ffd

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Aerospace Engineering

1. M. Clilverd
2. N. Thomson

In Astronomy and Astrophysics

1. Umran S. Inan
2. R. Said
3. M. Clilverd
4. Craig J. Rodger
5. Kenneth L. Cummins
6. N. Thomson
7. V. Pasko
8. M. Cohen

In Geophysics

1. M. Clilverd
2. Craig J. Rodger
3. N. Thomson

Citations in the corpus

• Solar flare induced ionospheric D-region enhancements from VLF amplitude observations (2001, methodology): “These variations have been reported on in more detail by Thomson (1993) and McRae and Thomson (2000). A small solar 'are gives rise to only a small VLF amplitude change accompanying the small perturbation in the D-region ionisation; the resulting peak VLF amplitude clearly depends not only on the si”
• Large solar flares and their ionospheric D region enhancements (2005, background): “affect VLF phase and this occurs progressively with changing daytime solar zenith angle; it is not simply a matter of being either day or night [ McRae and Thomson, 2000, 2004 ].”
• Long‐range lightning geolocation using a VLF radio atmospheric waveform bank (2010, background): “1, for an increase in ionospheric height from 70 km for daytime [McRae and Thomson, 2000] to 85 km for nighttime [Thomson et al.”