Magnetospheric disturbance induced equatorial plasma bubble development and dynamics: A case study in Brazilian sector
By M. Abdu, I. Batista, H. Takahashi, J. MacDougall, J. Sobral, A. Medeiros, N. Trivedi. 2003
205 citations recorded by the source corpus.
Subfields: Aerospace Engineering, Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/50a1656fb8f364e100b523d9fd60ea853004daa1
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Aerospace Engineering
In Astronomy and Astrophysics
Citations in the corpus
- South Atlantic magnetic anomaly ionization: A review and a new focus on electrodynamic effects in the equatorial ionosphere (2005, background): “Extensive analysis of the sporadic E-layer characteristics over Cachoeira Paulista has established that the occurrence, as well as the intensity of this layer, exhibits significant enhancements during magnetically disturbed conditions (Batista and Abdu, 1977; Abdu et al., 2003a).”
- 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): “In contrast, during a superstorm of 30 October 2003, it is observed that intense PP electric fields caused abnormally larger vertical drift of nearly more than 1000m/s, which did not produce any ESF signatures [Abdu et al., 2003; Abdu, 2012].”
- Midlatitude Plasma Bubbles Over China and Adjacent Areas During a Magnetic Storm on 8 September 2017 (2018, background): “Plasma bubbles with different scale sizes can manifest themselves as spread-F echoes on ionograms (Abdu et al., 2003), plume-like structures in radar backscatter maps (Woodman & La Hoz, 1976), airglow density depletions in all-sky images (Kelley et al., 2002), and very high frequency/ultrahigh…”
- 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].”
- Unusual early morning development of the equatorial anomaly in the Brazilian sector during the Halloween magnetic storm (2006, unknown): “Many authors have described drastic ionospheric effects at low latitudes related to strong magnetic storms, observed by various techniques such as ionosondes, optical measurements or satellite probes [see, e.g., Abdu et al., 2003; Basu JOURNAL OF GEOPHYSICAL RESEARCH, VOL.”
- A super bubble detected by dense GPS network at east Asian longitudes (2006, background): “Recently a magnetospheric disturbance induced bubble was observed in Brazilian sector to drift westward until early morning hours, and Hall electric field was discussed as possible cause [Abdu et al., 2003].”
- Global dayside ionospheric uplift and enhancement associated with interplanetary electric fields (2004, unknown): “…been identified as (1) prompt penetration zonal electric field often observed in the equatorial latitudes [Sastri, 1988; Fejer and Scherliess, 1995; Abdu et al., 1995, 2003; Sobral et al., 1997, 2001; Sastri et al., 2002; Kelley et al., 2003], following the early theoretical work of Blanc and…”