Long‐duration penetration of the interplanetary electric field to the low‐latitude ionosphere during the main phase of magnetic storms

By Chaosong Huang, J. Foster, M. Kelley. 2005

359 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/13b44c989133a727227a2214dd3970f29d2af261

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. B. Fejer
2. Jorge L. Chau
3. Y. Yamazaki
4. Astrid Maute
5. J. W. Jensen
6. M. Abdu
7. P. Park
8. Shuanggen Jin

In Geophysics

1. B. Fejer
2. J. W. Jensen
3. Jorge L. Chau
4. Y. Yamazaki
5. Shuanggen Jin
6. Astrid Maute
7. M. Abdu
8. Shin-Yi Su

Citations in the corpus

• Low‐latitude ionosphere response to super geomagnetic storm of 17/18 March 2015: Results from a chain of ground‐based observations over Indian sector (2015, background): “…turning of the z component of the interplanetary magnetic field (i.e., IMF Bz), from a steady northward configuration, produces a dawn to dusk convection electric field at high latitudes resulting in an undershielding condition [Somayajulu et al., 1987; Huang et al., 2005; Kikuchi et al., 2008].”
• Equatorial Ionospheric Electric Fields During the November 2004 Magnetic Storm (2007, positive): “On the other hand, the large variability of these electric fields is not well understood [e.g., Fejer, 2002; Huang et al., 2005 ], which indicates that their magnitudes and lifetimes are also affected by additional solar wind, magnetospheric, and high and low latitude ionospheric processes [e.g., S”
• Penetration of magnetospheric electric fields to the equator during a geomagnetic storm (2008, neutral): “[29] 2. The shielding became effective one hour after the onset of the equatorial DP2, in contrast to several hours of the shielding time constant suggested by Huang et al. [2005] .”
• Sq and EEJ—A Review on the Daily Variation of the Geomagnetic Field Caused by Ionospheric Dynamo Currents (2017, background): “Disturbance winds can persist for more than a day after a geomagnetic storm (Huang et al. 2005a).”
• Midlatitude Plasma Bubbles Over China and Adjacent Areas During a Magnetic Storm on 8 September 2017 (2018, background): “Second, recent studies have shown that the PPEF can persist with considerably longer durations of ∼8–10 hr if the IMF Bz is sustained southward for prolonged periods (Huang et al., 2005; Huang, 2008).”
• GPS observations of the ionospheric F2-layer behavior during the 20th November 2003 geomagnetic storm over South Korea (2008, background): “... change at 9:00 UT and increases from 10:00 UT until 19:00 UT. The F2-layer peak height (hmF2) suddenly rises from 8:00 UT when the shock of this storm just started, and reaches the maximum height at about 16:00 UT with a maximum Kp value of nine, and then gradually descends until 21:00 UT. The s”