165 citations
- Chulalongkorn UniversityTH16 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di CataniaIT8 papers
- Vidyasirimedhi Institute of Science and TechnologyTH8 papers
- Centre National de la Recherche ScientifiqueFR7 papers
- George Washington UniversityUS7 papers
- Los Alamos National LaboratoryUS7 papers
- Thailand Center of Excellence in PhysicsTH7 papers
- Université Paris-SaclayFR7 papers
- A. Alikhanyan National LaboratoryAM6 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR6 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR6 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma IIT6 papers
4 papers · 1 filter
Magnetic Field Line Separation by Random Ballistic Decorrelation in Transverse Magnetic Turbulence
Chutima Yannawa, Peera Pongkitiwanichakul, David Ruffolo +2
The statistics of the magnetic field line separation provide insight into how a bundle of field lines spreads out and the dispersion of non-thermal particles in a turbulent environ…
Role of Parallel Solenoidal Electric Field on Energy Conversion in 2.5D Decaying Turbulence with a Guide Magnetic Field
Peera Pongkitiwanichakul, David Ruffolo, Fan Guo +5
We perform 2.5D particle-in-cell simulations of decaying turbulence in the presence of a guide (out-of-plane) background magnetic field. The fluctuating magnetic field initially co…
Domains of Magnetic Pressure Balance in Parker Solar Probe Observations of the Solar Wind
David Ruffolo, Nawin Ngampoopun, Yash R. Bhora +4
The Parker Solar Probe (PSP) spacecraft is performing the first in situ exploration of the solar wind within 0.2 au of the Sun. Initial observations confirmed the Alfvénic nature o…
The Acceleration and Confinement of Energetic Electrons by a Termination Shock in a Magnetic Trap: An Explanation for Nonthermal Loop-top Sources during Solar Flares
Xiangliang Kong, Fan Guo, Chengcai Shen +6
Nonthermal loop-top sources in solar flares are the most prominent observational signature that suggests energy release and particle acceleration in the solar corona. Although seve…