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B. Van der Holst

28 papers hereh-index 00 citations0 works total

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

author position
  • first author4
  • middle author12
  • last author9

Across the 25 of 28 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR24
  • physics.space-ph3
  • physics.flu-dyn1
same name
  • B. van der Holst — 7 papers
  • B. van der Holst — 4 papers, h 17

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
20092026
most citedAlfven Wave Solar Model (AWSoM): Coronal Heating

483 citations · 1.5k across the 27 of their papers we have counts for

collaborators
Showing 2014Show all

3 papers · 1 filter

astro-ph.SR2014★ 46 cited

A Steady-State Picture of Solar Wind Acceleration and Charge State Composition Derived from a Global Wave-Driven MHD Model

Rona Oran, Enrico Landi, Bart van der Holst +7

The higher charge states found in slow (<400km s−1) solar wind streams compared to fast streams have supported the hypothesis that the slow wind originates in closed coronal…

physics.space-ph2014★ 63 cited

Global Numerical Modeling of Energetic Proton Acceleration in a Coronal Mass Ejection Traveling through the Solar Corona

Kamen A. Kozarev, Rebekah M. Evans, Nathan A. Schwadron +4

The acceleration of protons and electrons to high (sometimes GeV/nucleon) energies by solar phenomena is a key component of space weather. These solar energetic particle (SEP) even…

astro-ph.SR2014

Alfvén Wave Turbulence as a Coronal Heating Mechanism: Simultaneously Predicting the Heating Rate and the Wave-Induced Emission Line Broadening

R. Oran, E. Landi, B. van der Holst +2

In the present work, we test the predictions of the AWSoM model, a global extended-MHD model capable of calculating the propagation and turbulent dissipation of Alfvén waves in any…

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