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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 2026Show all

4 papers · 1 filter

astro-ph.SR2026

Energy Partitioning at the Termination Shock

Judit Szente, Bart van der Holst, Gabor Toth +1

We show new results of a global 3D magnetohydrodynamic (MHD) simulation of the Boston University outer heliosphere model where we used a newly developed approach that distributes t…

astro-ph.SR2026

The Effects of Energy Conservation in Simulating Solar Eruptions

Xianyu Liu, Spiro K. Antiochos, Nishtha Sachdeva +6

Strict energy conservation is, perhaps, the most basic principle in all physics, but has proven to be difficult to satisfy in numerical simulations of solar eruptions. The Alfvén W…

astro-ph.SR2026

Effects of the Background Magnetic Field on Flux Rope Eruptions

Xianyu Liu, Spiro K. Antiochos, Igor V. Sokolov +5

Solar eruptive events are generally believed to involve magnetic flux ropes (MFR), formed either in the pre-eruptive phase of the event or during the eruption itself. These MFR eru…

astro-ph.SR2026

Global Multi-ion Solar Wind Model. I. Ion Temperatures

Bart van der Holst, Judit Szente, Enrico Landi

Over the past several decades, observations have shown that minor ions have a higher temperature and flow faster than protons in the solar wind. Theories based on turbulence have b…

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