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H. Spruit

83 papers hereh-index 529.9k citations222 works total

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

author position
  • sole author18
  • first author11
  • middle author8
  • last author43

Across the 80 of 83 papers where every author was matched, so the position is known.

fields
  • astro-ph54
  • astro-ph.SR21
  • astro-ph.HE4
  • astro-ph.EP2
  • astro-ph.IM2
same name
  • H. Spruit — 4 papers, h 3

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
19952018
most citedDynamo action by differential rotation in a stably stratified stellar interior

1k citations · 7.5k across the 83 of their papers we have counts for

collaborators
Showing 2006 · astro-phShow all

4 papers · 2 filters

astro-ph2006★ 147 cited

Spectral and timing properties of a dissipative GRB photosphere

Dimitrios Giannios, Henk C. Spruit

We explore the observational appearance of the photosphere of an ultrarelativistic flow with internal dissipation of energy as predicted by the magnetic reconnection model. Previou…

astro-ph2006★ 92 cited

Magnetostatic penumbra models with field-free gaps

G. B. Scharmer, H. C. Spruit

We present numerical 2D magnetostatic models for sunspot penumbrae consisting of radially aligned field-free gaps in a potential magnetic field, as proposed by Spruit and Scharmer…

astro-ph2006★ 3 cited

Magnetic instability in a differentially rotating star

H. C. Spruit

Instabilities in magnetic fields wound up by differential rotation as reviewed in Spruit (1999) are discussed with some detail and new developments added. In stellar models which i…

astro-ph2006★ 188 cited

The role of kink instability in Poynting-flux dominated jets

Dimitrios Giannios, Henk C. Spruit

The role of kink instability in magnetically driven jets is explored through numerical one-dimensional steady relativistic MHD calculations. The instability is shown to have enough…

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