2021
DOI: 10.1002/9781119815617.ch4
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Recent Advances in Polar Cap Density Structure Research

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Cited by 5 publications
(5 citation statements)
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“…The terrestrial ionosphere is dynamic and highly variable depending on multiple factors, i.e., solar, interplanetary and lower atmosphere conditions, as well as geographic locations. Eruptive solar events, such as coronal mass ejections (CMEs), have the greatest impact on short term but large scale ionospheric variability [1][2][3][4][5][6][7][8][9] . As one of the five major space weather threats in the National Space Weather Strategy and Action Plan, ionospheric disturbance could degrade or disrupt satellite navigation and communication systems as well as long-distance radio communication.…”
Section: Background and Summarymentioning
confidence: 99%
“…The terrestrial ionosphere is dynamic and highly variable depending on multiple factors, i.e., solar, interplanetary and lower atmosphere conditions, as well as geographic locations. Eruptive solar events, such as coronal mass ejections (CMEs), have the greatest impact on short term but large scale ionospheric variability [1][2][3][4][5][6][7][8][9] . As one of the five major space weather threats in the National Space Weather Strategy and Action Plan, ionospheric disturbance could degrade or disrupt satellite navigation and communication systems as well as long-distance radio communication.…”
Section: Background and Summarymentioning
confidence: 99%
“…In recent years, these two categories have become known as "cold" and "hot" PCPs respectively, referring to the fact that PCPs formed from precipitation will typically have a plasma temperature higher than the background plasma while those from dense dayside plasma are known to be cooler (Zhang et al, 2017). Zou et al (2021a) suggested that those two types of patches should be routinely distinguished and their relationship and space weather impact should be further studied, such as whether the classical patch evolves into the hot patch under the influence of particle precipitation and FACs, or these hot patches can be produced solely by particle precipitation.…”
Section: Polar Cap Patches Patch Definition and Classificationmentioning
confidence: 99%
“…However, because there are currently no continuous and high-resolution observations of the dayside convection convection that would map to the magnetospheric driver region, such as magnetopause reconnection region, and the entire patch formation sequence is complex and not well understood, it is currently impossible to make exact predictions as to when and where PCPs are generated. More statistical studies are needed to understand the most probable IMF conditions right at the time when the patches are produced, in order to single out the major segmenting mechanism of patch (Zou et al, 2021a).…”
Section: Patch Generation Mechanismsmentioning
confidence: 99%
“…The combination of these processes results in a large-scale ionospheric plasma density increase redistribution from mid-latitude or even the equator to high latitudes, and at dusk, the plasma of the EIA crests can contribute to the plumes of Storm Enhanced Density (SED, Huba et al 2017;Sandel et al 2001). These plumes can be transported through the dayside cusp and across the polar cap into the night side where they form structures called Tongues Of Ionisation (TOI, Foster et al 2005) or polar cap patches (Foster et al 2021;Zou et al 2021a).…”
Section: Ionospheric Weathermentioning
confidence: 99%