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20172024
most citedModeling the Transport of Nonthermal Particles in Flares Using Fokker-Planck Kinetic Theory

51 citations · 121 across the 13 of their papers we have counts for

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6 papers · 1 filter

astro-ph.SR2024

Reduction of the downward energy flux of non-thermal electrons in the solar flare corona due to co-spatial return current losses

Meriem Alaoui, Gordon D. Holman, Marc Swisdak

High energy electrons carry much of a solar flare's energy. Therefore, understanding changes in electron beam distributions during their propagation is crucial. A key focus of this…

astro-ph.SR2021★ 16 cited

Role of Suprathermal Runaway Electrons Returning to the Acceleration Region in Solar Flares

Meriem Alaoui, Gordon D. Holman, Joel C. Allred +1

During solar flares, a large flux of energetic electrons propagate from the tops of reconnecting magnetic flux tubes toward the lower atmosphere. Over the course of the electrons'…

astro-ph.SR2020★ 1 cited

Solar Flare Energy Partitioning and Transport -- the Gradual Phase (a Heliophysics 2050 White Paper)

Graham S. Kerr, Meriem Alaoui, Joel C. Allred +14

Solar flares are a fundamental component of solar eruptive events (SEEs; along with solar energetic particles, SEPs, and coronal mass ejections, CMEs). Flares are the first compone…

astro-ph.SR2020★ 4 cited

Solar Flare Energy Partitioning and Transport -- the Impulsive Phase (a Heliophysics 2050 White Paper)

Graham S. Kerr, Meriem Alaoui, Joel C. Allred +14

Solar flares are a fundamental component of solar eruptive events (SEEs; along with solar energetic particles, SEPs, and coronal mass ejections, CMEs). Flares are the first compone…

astro-ph.SR2020★ 51 cited

Modeling the Transport of Nonthermal Particles in Flares Using Fokker-Planck Kinetic Theory

Joel C. Allred, Meriem Alaoui, Adam F. Kowalski +1

We describe a new approach for modeling the transport of high energy particles accelerated during flares from the acceleration region in the solar corona until their eventual therm…

astro-ph.SR2017★ 33 cited

Understanding breaks in solar flares x-ray spectra: Evaluation of a co-spatial return-current model

Meriem Alaoui, Gordon Holman

Hard x-ray spectral breaks are explained in terms of a 1D model with a co-spatial return current. We study 19 flares observed by RHESSI (Ramaty High Energy Solar Spectroscopic Imag…