Journal articles
High-speed solar wind stream effects on the topside ionosphere over Arecibo: A case study during solar minimum
Abstract : The impact of a high-speed solar wind stream (HSS) on the topside near-equatorial ionosphere (Arecibo: 28.17°N, L = 1.3) is investigated for the first time. Although the HSS did not lead to any significant geomagnetic storm activity, the ionosphere over Arecibo became hotter and expanded significantly in altitude as compared to a non-HSS interval. The O+/H+ transition height hT increased by ~200 km in the daytime and by ~100 km at night. At the hT, the peak ionospheric electron and ion temperatures increased by ~200–500 K during day and by ~50–70 K at night. While the O+ ion concentration exhibited an overall enhancement, deep penetration of the H+ ions below hT are observed during the day. The noontime peak electron density was ~4 times higher during the HSS event compared to the non-HSS interval. We present three possible mechanisms to explain this topside ionospheric heating.
Cited literature [68 references]
https://hal-insu.archives-ouvertes.fr/insu-01670692
Contributor : Nathalie Rouchon Connect in order to contact the contributor
Submitted on : Monday, June 25, 2018 - 9:24:21 AM
Last modification on : Wednesday, November 17, 2021 - 12:32:06 PM
Long-term archiving on: : Wednesday, September 26, 2018 - 1:29:45 PM
Contributor : Nathalie Rouchon Connect in order to contact the contributor
Submitted on : Monday, June 25, 2018 - 9:24:21 AM
Last modification on : Wednesday, November 17, 2021 - 12:32:06 PM
Long-term archiving on: : Wednesday, September 26, 2018 - 1:29:45 PM
File
Hajra_et_al-2017-Geophysical_R...
Publisher files allowed on an open archive