Which magnetic storms produce relativistic electrons at geosynchronous orbit

By T. P. O'Brien, R. McPherron, Didier Sornette, G. Reeves, R. Friedel, H. Singer. 2001

226 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/941e2c6a78857b6979287035271473e9b808cbf2

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. R. Thorne
2. Nigel P. Meredith
3. R. Horne
4. Wen Li
5. Y. Shprits
6. Jacob Bortnik
7. Binbin Ni
8. Danny Summers

In Molecular Biology

1. R. Thorne
2. Nigel P. Meredith
3. Vania Jordanova
4. Tuija I. Pulkkinen
5. Craig Kletzing
6. J. Fennell
7. W. Kurth
8. G. Hospodarsky

Citations in the corpus

• THEMIS observations of long‐lived regions of large‐amplitude whistler waves in the inner magnetosphere (2008, background): “These conditions (high-speed solar wind, low to moderate geophysical activity) are associated with effective radiation belt particle acceleration [O’Brien et al., 2001; Onsager et al., 2007] and increased whistler-mode chorus emissions [Hwang et al.”
• Energization of relativistic electrons in the presence of ULF power and mev microbursts: Evidence for dual ULF and VLF acceleration (2003, methodology): “geosynchronous satellites, using the statistical local time mapping algorithm described by O’Brien et al. [2001b]. We first identify magnetic storms in the interval 1989 through”
• The Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) on RBSP (2013, background): “…diffusion is a potentially important mechanism for energetic electron acceleration (Rostoker et al. 1998; Elkington et al. 1999; Hudson et al. 2001; O’Brien et al. 2001; Shprits and Thorne 2004) or loss (Shprits et al. 2006; Jordanova et al. 2008; Loto’aniu et al. 2010) during storm conditions,…”
• Space Weather: Terrestrial Perspective (2007, background): “Furthermore, although there is a general correlation between storm activity and electron enhancement, there is no one-to-one correlation that would indicate that higher peak intensity would necessarily lead to higher electron flux levels (O’Brien et al., 2001).”
• On the relationship between relativistic electron flux and solar wind velocity: Paulikas and Blake revisited (2010, result): “as suggested by previous studies [O’Brien et al., 2001].”
• Statistical analysis of relativistic electron energies for cyclotron resonance with EMIC waves observed on CRRES (2003, unknown): “…Summers and Ma , 2000a, 2000b; Hudson et al. , 2001; Li and Temerin , 2001; Mathie and Mann , 2001; Meredith et al. , 2001, 2002a, 2002b, 2003; O’Brien et al. , 2001; Friedel et al. , 2002; Summers et al. , 2002; Horne et al. , 2003; Miyoshi et al. , 2003], due in part to the potentially…”