Evidence for the Significant Differences in Response Times of Equatorial Ionization Anomaly Crest Corresponding to Plasma Fountains During Daytime and Post‐Sunset Hours. Issue 3 (2nd March 2021)

• Record Type: Journal Article
• Authors: Kumar, A.; Chakrabarty, D.; Pandey, K.; Fejer, B. G.; Sunda, S.; Seemala, G. K.; Sripathi, S.; Yadav, A. K.
• Is Part Of: Journal of geophysical research. Volume 126:Issue 3(2021)
• Page Start: n/a
• Page End: n/a
• Publication Date: 2021-03-02
• Subjects: equatorial ionization anomaly -- equatorial plasma fountain -- low latitude ionosphere -- OI 630.0 nm airglow -- pre‐reversal enhancement -- total electron content; Magnetospheric physics -- Periodicals; Space environment -- Periodicals; Cosmic physics -- Periodicals; Planets -- Atmospheres -- Periodicals; Heliosphere (Astrophysics) -- Periodicals; Geophysics -- Periodicals; 523.01
• DOI: 10.1029/2020JA028628
• Languages: English
• ISSNs: 2169-9380

Abstract

Abstract: Based on 10 years' (2010–2019) of vertical total electron content (VTEC) data from Ahmedabad (23.0°N, 72.6°E, dip angle 35.2°) and campaign based OI 630.0 nm airglow intensity measurements from Mt. Abu (24.6°N, 72.7°E, dip angle 38.0°), it is shown that plasma density over the equatorial ionization anomaly (EIA) crest region increases in varying degrees during post‐sunset hours (2000–2100 LT) in magnetically quiet periods. The post‐sunset peak in VTEC precedes the corresponding peak in airglow intensity. By comparing post‐sunset VTEC enhancements with ionosonde observations from Tirunelveli (8.7°N, 77.7°E, dip angle 1.7°), it is shown that pre‐reversal enhancement (PRE) of the zonal electric field causes these enhancements over the EIA crest region. These observations are supported by TEC measurements by GAGAN (GPS Aided Geo Augmented navigation), the Indian Satellite‐based Augmentation System (SBAS). Comparison of average VTEC variations with global empirical model drifts reveals that the post‐sunset enhancements in VTEC occurs ∼1.7 h after the PRE and are significant only during December solstice and equinoctial months in high solar activity years similar to seasonal variations in PRE amplitudes. This time delay (response time of EIA crest) is almost half compared to the average response time (3–4 h) associated with the daytime fountain. Based on the latitudinal gradient in SBAS‐TEC, it is proposed that the PRE drives plasma from 5°N to 10°N magnetic latitudes to the EIA crest region leading to shorter response time. These results show the important role of the PRE in conditioning the EIA crest region. Plain Language Summary: The equatorial ionization anomaly (EIA) crest region is one of the most important regions in the globe as far as the L‐band scintillation during post‐sunset hours is concerned. The plasma density variations over this region have important ramifications for the positional systems, navigation, and communication applications. Therefore, understanding the plasma density variations over this region during post‐sunset hours is important. In this work, it is shown that the evening time electric field variations over the dip‐equator changes the plasma density variations over the EIA crest region during post‐sunset hours at a much faster time scale than what is expected based on daytime processes. The possible mechanism is discussed. Key Points: Post‐sunset enhancement in plasma density over the equatorial ionization anomaly (EIA) crest region are found during December solstice and Equinox in high solar epoch Pre‐reversal enhancement of the zonal electric field over the dip equator causes this enhancement in about 1.7 h Plasma transport from 5° to 10° magnetic latitude to the EIA crest region leads to shorter response time