Equatorial Ionization Anomaly X‐Pattern Occurrences Observed by the GOLD Mission During Its First 5 Years

Abstract The Global‐scale Observations of Limb and Disk (GOLD) mission has provided an unusual array of upper atmosphere observations from a geostationary platform, including the behavior of the low latitude nighttime ionosphere. One of the features observed by GOLD is the formation of an X‐pattern in the Equatorial Ionization Anomaly when its crests collapse near the magnetic equator. This paper discusses the X‐patterns that were observed during the first 5 years of the GOLD mission (2018–2023). This catalog reveals that X‐pattern occurrences are more frequent during low solar activity, and appear to be driven by changes in the normal low latitude zonal winds. In the longitude region observed by GOLD (approximately 75°W–5°E) they occurred exclusively during the September Equinox‐December Solstice‐March Equinox seasons, and they were more likely to occur near 45°W longitude, near the point where the geomagnetic equator crosses the geographic equator in the western hemisphere.

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Publication Details

Journal
Journal of Geophysical Research Space Physics
Published
2025-02-01
DOI
https://doi.org/10.1029/2024ja033299
Citations
1
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
1.15

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article

Equatorial Ionization Anomaly X‐Pattern Occurrences Observed by the GOLD Mission During Its First 5 Years

R. Eastes, C. R. Martinis, D. K. Karan, R. E. Daniell
1 citations
Journal of Geophysical Research Space Physics
Solar and Space Plasma Dynamics
1.15
article

Equatorial Ionization Anomaly X‐Pattern Occurrences Observed by the GOLD Mission During Its First 5 Years

R. Eastes, C. R. Martinis, D. K. Karan, R. E. Daniell
article en
1 citations

Abstract

Abstract The Global‐scale Observations of Limb and Disk (GOLD) mission has provided an unusual array of upper atmosphere observations from a geostationary platform, including the behavior of the low latitude nighttime ionosphere. One of the features observed by GOLD is the formation of an X‐pattern in the Equatorial Ionization Anomaly when its crests collapse near the magnetic equator. This paper discusses the X‐patterns that were observed during the first 5 years of the GOLD mission (2018–2023). This catalog reveals that X‐pattern occurrences are more frequent during low solar activity, and appear to be driven by changes in the normal low latitude zonal winds. In the longitude region observed by GOLD (approximately 75°W–5°E) they occurred exclusively during the September Equinox‐December Solstice‐March Equinox seasons, and they were more likely to occur near 45°W longitude, near the point where the geomagnetic equator crosses the geographic equator in the western hemisphere.

Journal of Geophysical Research Space PhysicsVol. 130(2)
Boston University (US), University of Colorado Boulder (US), Laboratory for Atmospheric and Space Physics (US)
National Aeronautics and Space Administration, Goddard Space Flight Center, Heliophysics Division
Openalex Percentile: Top 21%
Solar and Space Plasma Dynamics
1.15
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