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researcher

G. Fleishman

94 papers hereh-index 303.1k citations236 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author5
  • first author28
  • middle author37
  • last author17

Across the 87 of 94 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR73
  • astro-ph13
  • astro-ph.IM4
  • astro-ph.HE2
  • astro-ph.CO1
  • physics.plasm-ph1
same name
  • G. Fleishman — 1 paper, h 7

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20052026
most citedMicrowave and Hard X-Ray Observations of the 2017 September 10 Solar Limb Flare

209 citations · 2.4k across the 94 of their papers we have counts for

collaborators
Showing 2009Show all

4 papers · 1 filter

astro-ph.SR2009★ 53 cited

Sub-THz radiation mechanisms in solar flares

Gregory D. Fleishman, Eduard P. Kontar

Observations in the sub-THz range of large solar flares have revealed a mysterious spectral component increasing with frequency and hence distinct from the microwave component comm…

astro-ph.SR2009★ 11 cited

Radio emission from acceleration sites of solar flares

Yixuan Li, Gregory D. Fleishman

The Letter takes up a question of what radio emission is produced by electrons at the very acceleration site of a solar flare. Specifically, we calculate incoherent radio emission…

astro-ph.SR2009★ 31 cited

Dynamic Magnetography of Solar Flaring Loops

Gregory D. Fleishman, Gelu M. Nita, Dale E. Gary

We develop a practical forward fitting method based on the SIMPLEX algorithm with shaking, which allows the derivation of the magnetic field and other parameters along a solar flar…

astro-ph.SR2009★ 41 cited

Particle acceleration by strong turbulence in solar flares: theory of spectrum evolution

A. M. Bykov, G. D. Fleishman

We propose a nonlinear self-consistent model of the turbulent non-resonant particle acceleration in solar flares. We simulate temporal evolution of the spectra of charged particles…

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