Comparison between empirical and physical models of the topside ionospheric-plasmaspheric electron content above Antarctica

dc.contributor.author	Bergeot, N.
dc.contributor.author	Pierrard, V.
dc.contributor.author	Darrouzet, F.
dc.contributor.author	Chevalier, J.-M.
dc.date	2019
dc.date.accessioned	2019-07-23T11:32:15Z
dc.date.available	2019-07-23T11:32:15Z
dc.identifier.uri	https://orfeo.belnet.be/handle/internal/7329
dc.description	As the polar regions are Earth's windows to outer space, the Antarctic continent provides a unique opportunity for scientific research that cannot be performed at mid-and low-latitude regions. Moreover, the polar ionosphere-plasmasphere system, especially over Antarctica, is not well understood as compared to other regions due to a lack of experimental observations. Consequently, one of the present challenges of the Space Weather community is to better characterize the climatological behavior of the polar ionosphere and plasmasphere separately in response to variations in the solar activity at high latitudes.
dc.language	eng
dc.title	Comparison between empirical and physical models of the topside ionospheric-plasmaspheric electron content above Antarctica
dc.type	Conference
dc.subject.frascati	Physical sciences
dc.audience	Scientific
dc.source.title	Proceedings of the URSI Asia-Pacific Radio Science Conference (AP-RASC), New Delhi, India, 9-15 March 2019
Orfeo.peerreviewed	No
dc.identifier.doi	10.23919/URSIAP-RASC.2019.8738318