14.2k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Goddard Space Flight CenterUS361 papers
- Marshall Space Flight CenterUS357 papers
- Centre National de la Recherche ScientifiqueFR280 papers
- Max Planck Institute for Extraterrestrial PhysicsDE240 papers
- University of Maryland, College ParkUS239 papers
- Universities Space Research AssociationUS214 papers
- Stanford UniversityUS212 papers
- National Institute for AstrophysicsIT196 papers
- University of Rome Tor VergataIT184 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR179 papers
- University of PaduaIT178 papers
- Istituto Nazionale di Fisica Nucleare, Roma Tor VergataIT175 papers
11 papers · 2 filters
An observational revisit of band-split solar type-II radio bursts
Guohui Du, Xiangliang Kong, Yao Chen +3
Band split of solar type II radio bursts, discovered several decades ago, is a fascinating phenomenon with the type-II lanes exhibiting two almost-parallel sub-bands with similar m…
Toward more realistic analytic models of the heliotail: Incorporating magnetic flattening via distortion flows
Jens Kleimann, Christian Röken, Horst Fichtner +1
Both physical arguments and simulations of the global heliosphere indicate that the tailward heliopause is flattened considerably in the direction perpendicular to both the incomin…
A Comparison Study of a Solar Active-Region Eruptive Filament and a Neighboring Non-Eruptive Filament
Chaowei Jiang, S. T. Wu, Xueshang Feng +1
Solar active region (AR) 11283 is a very magnetically complex region and it has produced many eruptions. However, there exists a non-eruptive filament in the plage region just next…
Destabilization of a Solar Prominence/Filament Field System by a Series of Eight Homologous Eruptive Flares
Navdeep K. Panesar, Alphonse C. Sterling, Davina E. Innes +1
Homologous flares are flares that occur repetitively in the same active region, with similar structure and morphology. A series of at least eight homologous flares occurred in acti…
Near-Sun Speed of CMEs and the Magnetic Non-potentiality of their Source Active Regions
Sanjiv K. Tiwari, David A. Falconer, Ronald L. Moore +3
We show that the speed of the fastest coronal mass ejections (CMEs) that an active region (AR) can produce can be predicted from a vector magnetogram of the AR. This is shown by lo…
Evidence of the Solar EUV hot channel as a magnetic flux rope from remote-sensing and in-situ observations
Hongqiang Song, Yao Chen, Jie Zhang +5
Hot channels (HCs), high temperature erupting structures in the lower corona of the Sun, have been proposed as a proxy of magnetic flux ropes (MFRs) since their initial discovery.…
Nonthermally Dominated Electron Acceleration during Magnetic Reconnection in a Low-beta Plasma
Xiaocan Li, Fan Guo, Hui Li +1
By means of fully kinetic simulations, we investigate electron acceleration during magnetic reconnection in a nonrelativistic proton--electron plasma with conditions similar to sol…
Acceleration phases of a solar filament during its eruption
Hongqiang Song, Yao Chen, Jie Zhang +3
Filament eruptions often lead to coronal mass ejections (CMEs), which can affect critical technological systems in space and on the ground when they interact with the geo-magnetosp…
Magnetic Untwisting in Solar Jets that Go into the Outer Corona in Polar Coronal Holes
Ronald L. Moore, Alphonse C. Sterling, David A. Falconer
We study 14 large solar jets observed in polar coronal holes. In EUV movies from SDO/AIA, each jet appears similar to most X-ray jets and EUV jets that erupt in coronal holes, but…
Magnetic field-line lengths inside interplanetary magnetic flux ropes
Qiang Hu, Jiong Qiu, Sam Krucker
We report on the detailed and systematic study of field-line twist and length distributions within magnetic flux ropes embedded in Interplanetary Coronal Mass Ejections (ICMEs). Th…
First Taste of Hot Channel in Interplanetary Space
Hongqiang Song, Jie Zhang, Yao Chen +3
Hot channel (HC) is a high temperature (10 MK) structure in the inner corona revealed first by Atmospheric Imaging Assembly (AIA) on board \textit{Solar Dynamics Observatory}…