Equatorial plasma bubbles observed by DMSP satellites during a full solar cycle: Toward a global climatology

By Chao-Song Huang, W. J. Burke, J. Machuzak, L. Gentile, P. J. Sultan. 2002

167 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/b2aaf9ba004a98cfbf4efd9cb5160858ddf2677d

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

1. Michi Nishioka
2. Takuya Tsugawa
3. Akinori Saito
4. W. J. Burke
5. L. Gentile
6. Yuichi Otsuka

In Astronomy and Astrophysics

1. Michi Nishioka
2. Takuya Tsugawa
3. M. Denton
4. J. Borovsky
5. Akinori Saito
6. W. J. Burke
7. L. Gentile
8. Yuichi Otsuka

Citations in the corpus

• 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].”
• Occurrence characteristics of plasma bubble derived from global ground‐based GPS receiver networks (2007, methodology): “Atlantic regions. (1), (2), (3), and (4) after probabilities indicate that the results come from Huang et al. [2002] , Makela et al. [2004], Kim et al. [2002], and Sahai et al. [2000], respectively.”
• Seasonal-longitudinal variability of equatorial plasma bubbles (2004, methodology): “1 of Huang et al. (2002) demonstrates more than an order of magnitude range in rates of EPB occurrence between solar maximum and minimum, the annual variation ofα at a given longitude is independent of the solar cycle.”