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
11 papers · 2 filters
Estimating Electric Fields from Vector Magnetogram Sequences
G. H. Fisher, B. T. Welsch, W. P. Abbett +1
Determining the electric field (E-field) distribution on the Sun's photosphere is essential for quantitative studies of how energy flows from the Sun's photosphere, through the cor…
On the Brightness and Waiting-time Distributions of a Type III Radio Storm observed by STEREO/WAVES
J. P. Eastwood, M. S. Wheatland, H. S. Hudson +5
Type III solar radio storms, observed at frequencies below approximately 16 MHz by space borne radio experiments, correspond to the quasi-continuous, bursty emission of electron be…
Signatures of Interchange Reconnection: STEREO, ACE and Hinode Observations Combined
D. Baker, A. P. Rouillard, L. van Driel-Gesztelyi +8
Combining STEREO, ACE and Hinode observations has presented an opportunity to follow a filament eruption and coronal mass ejection (CME) on the 17th of October 2007 from an active…
Comparison of Hinode/XRT and RHESSI detection of hot plasma in the non-flaring solar corona
F. Reale, J. M. McTiernan, P. Testa
We compare observations of the non-flaring solar corona made simultaneously with Hinode/XRT and with RHESSI. The analyzed corona is dominated by a single active region on 12 Novemb…
Submillimeter and X-ray observations of an X Class flare
C. G. Gimenez de Castro, G. Trottet, A. Silva-Valio +5
The GOES X1.5 class flare that occurred on August 30,2002 at 1327:30 UT is one of the few events detected so far at submillimeter wavelengths. We present a detailed analysis of thi…
Magnetic fluctuation power near proton temperature anisotropy instability thresholds in the solar wind
S. D. Bale, J. C. Kasper, G. G. Howes +3
The proton temperature anisotropy in the solar wind is known to be constrained by the theoretical thresholds for pressure anisotropy-driven instabilities. Here we use approximately…
Coronal radiation belts
H. S. Hudson, A. L. MacKinnon, S. F. N. Frewen +1
The magnetic field of the solar corona has a large-scale dipole character, which maps into the bipolar field in the solar wind. Using standard representations of the coronal field,…
Acceleration of Relativistic Protons during the 20 January 2005 Flare and CME
S. Masson, K. -L. Klein, R. Buetikofer +4
The origin of relativistic solar protons during large flare/CME events has not been uniquely identified so far.We perform a detailed comparative analysis of the time profiles of re…
Multi-Wavelength Observation of Electron Acceleration in the 2006 December 13 Flare
T. Minoshima, S. Imada, T. Morimoto +8
We present a multi-wavelength observation of a solar flare occurring on 2006 December 13 with Hinode, RHESSI, and the Nobeyama Radio Observatory, to study the electron acceleration…
A Critical Assessment of Nonlinear Force-Free Field Modeling of the Solar Corona for Active Region 10953
Marc L. DeRosa, Carolus J. Schrijver, Graham Barnes +16
Nonlinear force-free field (NLFFF) models are thought to be viable tools for investigating the structure, dynamics and evolution of the coronae of solar active regions. In a series…
Imaging Spectroscopy on Preflare Coronal Nonthermal Sources Associated with the 2002 July 23 Flare
Ayumi Asai, Hiroshi Nakajima, Masumi Shimojo +3
We present a detailed examination on the coronal nonthermal emissions during the preflare phase of the X4.8 flare that occurred on 2002 July 23. The microwave (17 GHz and 34 GHz) d…