DMSP observations of equatorial plasma bubbles in the topside ionosphere near solar maximum

By C.-Y. F. Huang, W. J. Burke, J. Machuzak, L. Gentile, P. J. Sultan. 2001

187 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/432af51caaac01683fc9b34c1cb827a2ad7c5905

How researchers see this paper

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In Aerospace Engineering

1. L. P. Goncharenko
2. Philip J. Erickson
3. Guanyi Ma
4. Takashi Maruyama
5. Chaosong Huang
6. J. Foster
7. C. Valladares
8. W. J. Burke

In Astronomy and Astrophysics

1. L. P. Goncharenko
2. J. Foster
3. C. Valladares
4. M. Abdu
5. Philip J. Erickson
6. Guanyi Ma
7. Takashi Maruyama
8. M. Denton

Citations in the corpus

• A strong positive phase of ionospheric storms observed by the Millstone Hill incoherent scatter radar and global GPS network (2005, methodology): “Huang et al. [2001] studied seasonal/longitudinal occurrence of equatorial ionospheric spread F plasma bubbles using measurements of the DMSP satellites and found that far more bubbles were detected in the Atlantic sector than in the Pacific sector.”
• A super bubble detected by dense GPS network at east Asian longitudes (2006, background): “the prompt penetration of high latitude electric fields [Basu et al., 2005; Huang et al., 2001].”
• Differences between CME‐driven storms and CIR‐driven storms (2006, background): “[30] Large equatorial bubbles, which appear in the topside ionosphere when Dst is increasing in magnitude [Huang et al., 2002; Basu et al., 2005], have been reported for many CME-driven magnetic storms [e.g., Huang et al., 2001; Abdu et al., 2003; Basu et al., 2005].”
• South Atlantic magnetic anomaly ionization: A review and a new focus on electrodynamic effects in the equatorial ionosphere (2005, background): “They sought to associate the largest bubble occurrence rate to the weakest magnetic field intensity based on a previous suggestion by Huang et al. (2001) of a possible negative correlation between the two parameters.”
• C/NOFS: a Mission to Forecast Scintillations (2004, background): “Recent studies using the Defense Meteorological Satellite Program (DMSP) satellites in the evening sector have demonstrated that intense, fast-moving equatorial plasma bubbles (EPBs) occur frequently in the initial and main phases of geomagnetic storms [Huang et al., 2001].”
• Statistics of total electron content depletions observed over the South American continent for the year 2008 (2011, methodology): “of plasma depletions depend strongly on season and longitude [Aarons, 1993;Huang et al., 2001; Conker et al., 2004].”
• Seasonal-longitudinal variability of equatorial plasma bubbles (2004, methodology): “Strong seasonal-versuslongitudinal (S/L) variability characterizes the frequency of EPB occurrence (Aarons, 1993; Huang et al., 2001).”