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researcher

J. Hoeksema

3 papers hereh-index 5015k citations281 works total

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

author position
  • middle author2

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3

identity via Semantic Scholar / OpenAlex

most citedWhy Is the Great Solar Active Region 12192 Flare-Rich But CME-Poor?

224 citations · 334 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2015★ 65 cited

The Coronal Global Evolutionary Model: Using HMI Vector Magnetogram and Doppler Data to Model the Buildup of Free Magnetic Energy in the Solar Corona

George H. Fisher, William. P. Abbett, David J. Bercik +11

The most violent space weather events (eruptive solar flares and coronal mass ejections) are driven by the release of free magnetic energy stored in the solar corona. Energy can bu…

astro-ph.SR2015★ 45 cited

The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: Magnetohydrodynamics Simulation Module for the Global Solar Corona

Keiji Hayashi, J. Todd Hoeksema, Yang Liu +3

Time-dependent three-dimensional magnetohydrodynamics (MHD) simulation modules are implemented at the Joint Science Operation Center (JSOC) of Solar Dynamics Observatory (SDO). The…

astro-ph.SR2015★ 224 cited

Why Is the Great Solar Active Region 12192 Flare-Rich But CME-Poor?

Xudong Sun, Monica G. Bobra, J. Todd Hoeksema +6

Solar active region (AR) 12192 of October 2014 hosts the largest sunspot group in 24 years. It is the most prolific flaring site of Cycle 24, but surprisingly produced no coronal m…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.