Terrestrial gamma‐ray flashes in the Fermi era: Improved observations and analysis methods

By M. Briggs, S. Xiong, V. Connaughton, D. Tierney, G. Fitzpatrick, S. Foley, J. Grove, A. Chekhtman, M. Gibby, G. Fishman and 15 more. 2013

136 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/454cbee73002a0fc3efb980ede1ca8d34f329e76

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. C. Wilson-Hodge
2. S. McBreen
3. Jordan B. Camp
4. T. Littenberg
5. J. Greiner
6. M. Briggs
7. M. Briggs
8. A. Kienlin

In Nuclear and High Energy Physics

1. S. McBreen
2. J. Greiner
3. R. Diehl
4. J. Racusin
5. A. Spitkovsky

Citations in the corpus

• THE FERMI GBM GAMMA-RAY BURST SPECTRAL CATALOG: FOUR YEARS OF DATA (2014, background): “…offers great capabilities to observe all kinds of high-energy astrophysical phenomena, such as, e.g., solar flares (e.g., Gruber et al. 2011b; Ackermann et al. 2012a), soft gamma repeaters (e.g., Lin et al. 2011; von Kienlin et al. 2012) and terrestrial gamma-ray flashes (e.g., Briggs et al. 2013).”
• THE THIRD FERMI GBM GAMMA-RAY BURST CATALOG: THE FIRST SIX YEARS (2016, background): “The rate of detection of TGFs increased to nearly 850 per year (Briggs et al. 2013).”
• FERMI GBM OBSERVATIONS OF LIGO GRAVITATIONAL-WAVE EVENT GW150914 (2016, methodology): “Typical durations for the gamma-ray and electron events are several hundred μs and several to tens of ms, respectively, much shorter than GW150914-GBM (Briggs et al. 2013).”