High-latitude ionospheric response to the solar eclipse of 1 August 2008: EISCAT observations and TRANSCAR simulation

• Published in: Journal of atmospheric and solar-terrestrial physics 2013-12, Vol.105-106, p.336-349
• Main Authors: Pitout, F., Blelly, P.-L., Alcaydé, D.
• Format: Article
• Language: English
• Subjects: Ionosphere; Modelling; Plasma temperature and density; Solar radiation effects
• ISSN: 1364-6826; 1879-1824
• DOI: 10.1016/j.jastp.2013.02.004

On 1 August 2008, a total solar eclipse occurred and the footprint of its umbra passed North–East of the Svalbard archipelago, where the EISCAT Svalbard Radars (ESR) are installed. This eclipse is peculiar because it was seen at high-latitude, thus with large solar zenith angles and it was the first time that incoherent scatter radars were able to sound the ionospheric response at such a high latitude. The ESR data, after correction, show the typical signatures of a solar eclipse: depletion in electron density in the E- and F-regions, a decrease in electron temperature in the F-region, and a downflow of ions. Also, the UHF dish of the mainland EISCAT system measured a decrease in the same parameters, showing the influence of the penumbra (partial eclipse) on the ionosphere. We have modelled the response of the high-latitude ionosphere to this solar eclipse with the TRANSCAR code. Our simulations reproduce rather well the observations above the UHF radar in Tromsø and the ESR on Svalbard. In particular, we show the influence of particle precipitation above the ESR and we suspect an effect above Tromsø of the photoelectrons coming from the opposite hemisphere. Another interesting and quite unusual feature is the observation of the summer ionospheric cusp undergoing the eclipse. Radar data show structures of enhanced electron temperature, due to soft particle precipitation through the polar cusp. ► We have observed and modelled the ionospheric response to the eclipse of 1 August 2008. ► This eclipse occurred at high-latitude, which leads to specific features. ► The large magnetic dip angles favour downward ion diffusion due to plasma cooling. ► The totality affects open field lines that undergo escape of H+. ► The effects of both the eclipse and cusp precipitation are observed.