Can HF heating generate ESF bubbles?

Abstract

The injection of powerful HF waves into the ionosphere can lead to strong electron heating followed by a pressure perturbation which can locally reduce the plasma density. In the postsunset equatorial ionosphere, density perturbations can provide the seed to generate equatorial spread F (ESF) bubbles. In this paper, a modified version of the SAMI3/ESF ionosphere code is used to model the density depletions created by HF heating and to determine if ESF bubbles can be artificially generated. It is found that HF heating primarily redistributes plasma along the geomagnetic field and does not significantly perturb the flux tube integrated conductivities. Thus, HF heating does not appear to be a viable method to seed or generate ESF bubbles.

Document Details

Document Type
Pub Defense Publication
Publication Date
Dec 02, 2014
Source ID
10.1002/2014gl062293

Entities

People

  • Joseph D. Huba
  • Kate Zawdie

Organizations

  • United States Naval Research Laboratory

Tags

Fields of Study

  • Physics

Readers

  • Astronomy and Astrophysics.
  • Atmospheric Science / Meteorology, specifically Wind Wave Turbulence.
  • Plasma Physics.

Technology Areas

  • Microelectronics