18.1k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- University of California, BerkeleyUS1.3k papers
- Goddard Space Flight CenterUS457 papers
- California Institute of TechnologyUS379 papers
- Centre National de la Recherche ScientifiqueFR367 papers
- Lawrence Berkeley National LaboratoryUS262 papers
- Jet Propulsion LaboratoryUS260 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR240 papers
- National Institute for AstrophysicsIT239 papers
- University of CambridgeGB208 papers
- Imperial College LondonGB203 papers
- Institut de Recherche en Astrophysique et PlanétologieFR195 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR181 papers
6 papers · 2 filters
Reconnection Properties of Large-Scale Current Sheets During Coronal Mass Ejection Eruptions
B. J. Lynch, J. K. Edmondson, M. D. Kazachenko +1
We present a detailed analysis of the properties of magnetic reconnection at large-scale current sheets in a high cadence version of the Lynch & Edmondson (2013) 2.5D MHD simulatio…
Helioseismic and Magnetic Imager observations of linear polarization from a loop prominence system
Pascal Saint-Hilaire, Jesper Schou, Juan-Carlos Martínez Oliveros +4
White-light observations by the Solar Dynamics Observatory's Helioseismic and Magnetic Imager of a loop-prominence system occurring in the aftermath of an X-class flare on 2013 May…
The Photospheric Poynting Flux and Coronal Heating
B. T. Welsch
Some models of coronal heating suppose that convective motions at the photosphere shuffle the footpoints of coronal magnetic fields and thereby inject sufficient magnetic energy up…
A 33 year constancy of the X-ray coronae of AR Lac and eclipse diagnosis of scale height
Jeremy J. Drake, Peter Ratzlaff, Vinay Kashyap +3
Extensive X-ray and extreme ultraviolet (EUV) photometric observations of the eclipsing RS CVn system AR Lac were obtained over the years 1997 to 2013 with the Chandra X-ray Observ…
Flare Ribbon Energetics in the Early Phase of an SDO Flare
L. Fletcher, I. G. Hannah, H. S. Hudson +1
The sites of chromospheric excitation during solar flares are marked by extended extreme ultraviolet ribbons and hard X-ray footpoints. The standard interpretation is that these ar…
Statistical Properties of Super-hot Solar Flares
Amir Caspi, Säm Krucker, R. P. Lin
We use RHESSI high-resolution imaging and spectroscopy observations from ~6 to 100 keV to determine the statistical relationships between measured parameters (temperature, emission…