Affiliation:
1. Université Paris Cité Institut de physique du globe de Paris CNRS Paris France
2. Institute of Atmospheric Physics of the Czech Academy of Sciences Prague Czechia
Abstract
AbstractPowerful lightning strikes generate broadband electromagnetic signals. At Extremely Low Frequencies (ELF), the signal partly leaks into the ionosphere and produces whistlers that can be detected by satellites. Indeed, the satellites of the European Space Agency (ESA) Swarm Earth Explorer mission can detect those signals during 250 Hz burst‐mode acquisition campaigns of their Absolute Scalar Magnetometers (ASM). The dispersion of these whistlers depends on their propagation path and the distribution of ionization in the ionosphere crossed along that path. In this paper, we introduce a technique to derive a new measure of ionosphere electron content, the Total square‐Root Electron Content (TREC), using the arrival times of two frequencies of the whistler signal. We validate this approach by using data from ionosondes and from in situ measurements of the electron density at Swarm location. This technique brings new opportunities for sounding the ionosphere in regions poorly observed by other techniques.
Funder
European Space Agency
Danmarks Tekniske Universitet
Centre National d’Etudes Spatiales
Publisher
American Geophysical Union (AGU)