422 citations
- Goddard Space Flight CenterUS46 papers
- Centre National de la Recherche ScientifiqueFR33 papers
- Johns Hopkins University Applied Physics LaboratoryUS29 papers
- University of California, BerkeleyUS28 papers
- George Mason UniversityUS23 papers
- Catholic University of AmericaUS21 papers
- Laboratoire d’études spatiales et d’instrumentation en astrophysiqueFR21 papers
- Observatoire de ParisFR21 papers
- United States Naval Research LaboratoryUS19 papers
- University College LondonGB19 papers
- HeliophysicsUS18 papers
- University of New HampshireUS17 papers
6 papers · 1 filter
A multi-spacecraft view of a giant filament eruption during 26/27 September 2009
Sanjay Gosain, Brigitte Schmieder, Guy Artzner +2
We analyze multi-spacecraft observations of a giant filament eruption that occurred during 26 and 27 September 2009. The filament eruption was associated with a relatively slow cor…
Non-neutralized Electric Current Patterns in Solar Active Regions: Origin of the Shear-Generating Lorentz Force
Manolis K. Georgoulis, Viacheslav S. Titov, Zoran Mikic
Using solar vector magnetograms of the highest available spatial resolution and signal-to-noise ratio we perform a detailed study of electric current patterns in two solar active r…
2010 August 1-2 sympathetic eruptions: I. Magnetic topology of the source-surface background field
V. S. Titov, Z. Mikic, T. Török +2
A sequence of apparently coupled eruptions was observed on 2010 August 1-2 by SDO and STEREO. The eruptions were closely synchronized with one another, even though some of them occ…
Slow Rise and Partial Eruption of a Double-Decker Filament. I Observations and Interpretation
Rui Liu, Bernhard Kliem, Tibor Török +5
We study an active-region dextral filament which was composed of two branches separated in height by about 13 Mm. This "double-decker" configuration sustained for days before the u…
Contracting and Erupting Components of Sigmoidal Active Regions
Rui Liu, Chang Liu, Tibor Török +2
It is recently noted that solar eruptions can be associated with the contraction of coronal loops that are not involved in magnetic reconnection processes. In this paper, we invest…
MHD Waves and Coronal Heating: Unifying Empirical and MHD Turbulence Models
Igor V. Sokolov, Bart van der Holst, Rona Oran +6
We present a new global model of the solar corona, including the low corona, the transition region and the top of chromosphere. The realistic 3D magnetic field is simulated using t…