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researcher

J. Schober

41 papers hereh-index 181.3k citations53 works total

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

author position
  • first author16
  • middle author12
  • last author12

Across the 40 of 41 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO13
  • astro-ph.GA11
  • physics.plasm-ph9
  • physics.flu-dyn5
  • astro-ph.IM1
  • astro-ph.SR1
same name
  • J. Schober — 8 papers, h 4

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
20112026
most citedMach Number Dependence of Turbulent Magnetic Field Amplification: Solenoidal versus Compressive Flows

249 citations · 1.7k across the 41 of their papers we have counts for

collaborators
Showing 2011Show all

3 papers · 1 filter

astro-ph.CO2011

Magnetic fields in the first galaxies: Dynamo amplification and limits from reionization

Dominik R. G. Schleicher, Jennifer Schober, Christoph Federrath +3

We discuss the amplification of magnetic fields by the small-scale dynamo, a process that could efficiently produce strong magnetic fields in the first galaxies. In addition, we de…

physics.flu-dyn2011★ 249 cited

Mach Number Dependence of Turbulent Magnetic Field Amplification: Solenoidal versus Compressive Flows

Christoph Federrath, Gilles Chabrier, Jennifer Schober +3

We study the growth rate and saturation level of the turbulent dynamo in magnetohydrodynamical simulations of turbulence, driven with solenoidal (divergence-free) or compressive (c…

astro-ph.CO2011★ 107 cited

Magnetic Field Amplification by Small-Scale Dynamo Action: Dependence on Turbulence Models and Reynolds and Prandtl Numbers

Jennifer Schober, Dominik Schleicher, Christoph Federrath +2

The small-scale dynamo is a process by which turbulent kinetic energy is converted into magnetic energy, and thus is expected to depend crucially on the nature of turbulence. In th…

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