Affiliation:
1. Haystack Observatory Massachusetts Institute of Technology Westford MA USA
2. Department of Electrical and Computer Engineering and Center for Space Physics Boston University Boston MA USA
3. University of Tromsø Tromsø Norway
4. Atmospheric and Oceanic Sciences University of California, Los Angeles Los Angeles CA USA
5. Smead Aerospace Engineering Sciences Department University of Colorado Boulder Boulder CO USA
Abstract
AbstractA new observational phenomenon, named Simultaneous Global Ionospheric Density Disturbance (SGD), is identified in GNSS total electron content (TEC) data during periods of three typical geospace disturbances: a Coronal Mass Ejection‐driven severe disturbance event, a high‐speed stream event, and a minor disturbance day with a maximum Kp of 4. SGDs occur frequently on dayside and dawn sectors, with a ∼1% TEC increase. Notably, SGDs can occur under minor solar‐geomagnetic disturbances. SGDs are likely caused by penetration electric fields (PEFs) of solar‐geomagnetic origin, as they are associated with Bz southward, increased auroral AL/AU, and solar wind pressure enhancements. These findings offer new insights into the nature of PEFs and their ionospheric impact while confirming some key earlier results obtained through alternative methods. Importantly, the accessibility of extensive GNSS networks, with at least 6,000 globally distributed receivers for ionospheric research, means that rich PEF information can be acquired, offering researchers numerous opportunities to investigate geospace electrodynamics.
Funder
Heliophysics Division
Directorate for Geosciences
Air Force Office of Scientific Research
Office of Naval Research Global
Publisher
American Geophysical Union (AGU)
Subject
General Earth and Planetary Sciences,Geophysics
Cited by
4 articles.
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