Determinations of ionosphere and plasmasphere electron content for an African chain of GPS stations

The confluence of recent instrumentation deployments in Africa with developments for the determination of plasmasphere electron content using Global Positioning System (GPS) receivers has provided new opportunities for investigations in that region. This investigation, using a selected chain of...

Full description

Bibliographic Details
Main Authors: A. J. Mazzella Jr., J. B. Habarulema, E. Yizengaw
Format: Article
Language:English
Published: Copernicus Publications 2017-05-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/35/599/2017/angeo-35-599-2017.pdf
_version_ 1811226670167752704
author A. J. Mazzella Jr.
J. B. Habarulema
E. Yizengaw
author_facet A. J. Mazzella Jr.
J. B. Habarulema
E. Yizengaw
author_sort A. J. Mazzella Jr.
collection DOAJ
description The confluence of recent instrumentation deployments in Africa with developments for the determination of plasmasphere electron content using Global Positioning System (GPS) receivers has provided new opportunities for investigations in that region. This investigation, using a selected chain of GPS stations, extends the method (SCORPION) previously applied to a chain of GPS stations in North America in order to separate the ionosphere and plasmasphere contributions to the total electron content (TEC) during a day (24 July) in 2011. The results span latitudes from the southern tip of Africa, across the Equator, to the southern Arabian Peninsula, providing a continuous latitudinal profile for both the ionosphere and plasmasphere during this day.<br><br>The peak diurnal vertical ionosphere electron content (IEC) increases from about 14 TEC units (1 TEC unit  =  10<sup>16</sup> electrons m<sup>−2</sup>) at the southernmost station to about 32 TEC units near the geographic equator, then decreases to about 28 TEC units at the Arabian Peninsula. The peak diurnal slant plasmasphere electron content (PEC) varies between about 4 and 7 TEC units among the stations, with a local latitudinal profile that is significantly influenced by the viewing geometry at the station location, relative to the magnetic field configuration. In contrast, the peak vertical PEC varies between about 1 and 6 TEC units among the stations, with a more uniform latitudinal variation.<br><br>Comparisons to other GPS data analyses are also presented for TEC, indicating the influence of the PEC on the determination of latitudinal TEC variations and also on the absolute TEC levels, by inducing an overestimate of the receiver bias. The derived TEC latitudinal profiles, in comparison to global map profiles, tend to differ from the map results only about as much as the map results differ among themselves. A combination of ionosonde IEC and alternative GPS TEC measurements, which in principle permits a PEC determination through their difference, was compared to the composite and separate ionosphere and plasmasphere contributions derived solely by the SCORPION method for one station. Although there is considerably more scatter in the PEC values derived from the difference of the GPS TEC and ionosonde IEC measurements compared to the PEC values derived by the SCORPION method, the average overhead values for this day are comparable for the two methods, near 2 TEC units, at the South African site examined.<br><br>This initial investigation provides a basis for day-to-day TEC monitoring for Africa, with separate ionosphere and plasmasphere electron content determinations.
first_indexed 2024-04-12T09:29:02Z
format Article
id doaj.art-49504dd0553d4f6098a5c27b816186e2
institution Directory Open Access Journal
issn 0992-7689
1432-0576
language English
last_indexed 2024-04-12T09:29:02Z
publishDate 2017-05-01
publisher Copernicus Publications
record_format Article
series Annales Geophysicae
spelling doaj.art-49504dd0553d4f6098a5c27b816186e22022-12-22T03:38:24ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762017-05-013559961210.5194/angeo-35-599-2017Determinations of ionosphere and plasmasphere electron content for an African chain of GPS stationsA. J. Mazzella Jr.0J. B. Habarulema1E. Yizengaw2Watertown, Massachusetts, 02472-1049, USASANSA Space Science, Hermanus, 7200, South AfricaInstitute for Scientific Research, Boston College, Chestnut Hill, Massachusetts, 02459, USAThe confluence of recent instrumentation deployments in Africa with developments for the determination of plasmasphere electron content using Global Positioning System (GPS) receivers has provided new opportunities for investigations in that region. This investigation, using a selected chain of GPS stations, extends the method (SCORPION) previously applied to a chain of GPS stations in North America in order to separate the ionosphere and plasmasphere contributions to the total electron content (TEC) during a day (24 July) in 2011. The results span latitudes from the southern tip of Africa, across the Equator, to the southern Arabian Peninsula, providing a continuous latitudinal profile for both the ionosphere and plasmasphere during this day.<br><br>The peak diurnal vertical ionosphere electron content (IEC) increases from about 14 TEC units (1 TEC unit  =  10<sup>16</sup> electrons m<sup>−2</sup>) at the southernmost station to about 32 TEC units near the geographic equator, then decreases to about 28 TEC units at the Arabian Peninsula. The peak diurnal slant plasmasphere electron content (PEC) varies between about 4 and 7 TEC units among the stations, with a local latitudinal profile that is significantly influenced by the viewing geometry at the station location, relative to the magnetic field configuration. In contrast, the peak vertical PEC varies between about 1 and 6 TEC units among the stations, with a more uniform latitudinal variation.<br><br>Comparisons to other GPS data analyses are also presented for TEC, indicating the influence of the PEC on the determination of latitudinal TEC variations and also on the absolute TEC levels, by inducing an overestimate of the receiver bias. The derived TEC latitudinal profiles, in comparison to global map profiles, tend to differ from the map results only about as much as the map results differ among themselves. A combination of ionosonde IEC and alternative GPS TEC measurements, which in principle permits a PEC determination through their difference, was compared to the composite and separate ionosphere and plasmasphere contributions derived solely by the SCORPION method for one station. Although there is considerably more scatter in the PEC values derived from the difference of the GPS TEC and ionosonde IEC measurements compared to the PEC values derived by the SCORPION method, the average overhead values for this day are comparable for the two methods, near 2 TEC units, at the South African site examined.<br><br>This initial investigation provides a basis for day-to-day TEC monitoring for Africa, with separate ionosphere and plasmasphere electron content determinations.https://www.ann-geophys.net/35/599/2017/angeo-35-599-2017.pdf
spellingShingle A. J. Mazzella Jr.
J. B. Habarulema
E. Yizengaw
Determinations of ionosphere and plasmasphere electron content for an African chain of GPS stations
Annales Geophysicae
title Determinations of ionosphere and plasmasphere electron content for an African chain of GPS stations
title_full Determinations of ionosphere and plasmasphere electron content for an African chain of GPS stations
title_fullStr Determinations of ionosphere and plasmasphere electron content for an African chain of GPS stations
title_full_unstemmed Determinations of ionosphere and plasmasphere electron content for an African chain of GPS stations
title_short Determinations of ionosphere and plasmasphere electron content for an African chain of GPS stations
title_sort determinations of ionosphere and plasmasphere electron content for an african chain of gps stations
url https://www.ann-geophys.net/35/599/2017/angeo-35-599-2017.pdf
work_keys_str_mv AT ajmazzellajr determinationsofionosphereandplasmasphereelectroncontentforanafricanchainofgpsstations
AT jbhabarulema determinationsofionosphereandplasmasphereelectroncontentforanafricanchainofgpsstations
AT eyizengaw determinationsofionosphereandplasmasphereelectroncontentforanafricanchainofgpsstations