Articles | Volume 38, issue 2
https://doi.org/10.5194/angeo-38-297-2020
https://doi.org/10.5194/angeo-38-297-2020
Regular paper
 | 
06 Mar 2020
Regular paper |  | 06 Mar 2020

Electron heating by HF pumping of high-latitude ionospheric F-region plasma near magnetic zenith

Thomas B. Leyser, Björn Gustavsson, Theresa Rexer, and Michael T. Rietveld

Download

Interactive discussion

Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
Printer-friendly Version - Printer-friendly version Supplement - Supplement

Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision
ED: Publish as is (02 Feb 2020) by Nick Sergis
AR by Thomas Leyser on behalf of the Authors (03 Feb 2020)  Manuscript 
Download
Short summary
Powerful radio waves transmitted into the ionosphere give the strongest turbulence effects in geomagnetic zenith, antiparallel to the magnetic field in the Northern Hemisphere. Our results obtained with the EISCAT (European Incoherent SCATter association) Heating facility in Norway and the EISCAT UHF incoherent scatter radar together with modelling suggest that the pump wave propagates in the L mode, rather than in the O mode that is usually assumed to be involved in such experiments.