- SLAC National Accelerator LaboratoryUS5.1k papers
- Kavli Institute for Particle Astrophysics and CosmologyUS3.3k papers
- Centre National de la Recherche ScientifiqueFR2.2k papers
- University of California, BerkeleyUS2.2k papers
- California Institute of TechnologyUS2.1k papers
- Lawrence Berkeley National LaboratoryUS1.7k papers
- Massachusetts Institute of TechnologyUS1.7k papers
- Princeton UniversityUS1.5k papers
- The Ohio State UniversityUS1.5k papers
- University of California, Santa CruzUS1.5k papers
- University of Maryland, College ParkUS1.4k papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR1.4k papers
765 papers · 1 filter
Fermi Detection of γ-ray emission from the M2 Soft X-ray Flare on 2010 June 12
Fermi GBM Collaboration, Fermi LAT Collaboration, B. R. Dennis +2
The GOES M2-class solar flare, SOL2010-06-12T00:57, was modest in many respects yet exhibited remarkable acceleration of energetic particles. The flare produced an ~50 s impulsive…
Bipolar Magnetic Regions on the Sun: Global Analysis of the SOHO/MDI Data Set
J. O. Stenflo, A. G. Kosovichev
The magnetic flux that is generated by dynamo inside the Sun emerges in the form of bipolar magnetic regions. We have analyzed the whole set of solar magnetograms obtained with the…
Atoms in Flight and the Remarkable Connections between Atomic and Hadronic Physics
Stanley J. Brodsky
Atomic physics and hadron physics are both based on Yang Mills gauge theory; in fact, quantum electrodynamics can be regarded as the zero-color limit of quantum chromodynamics. I r…
Invariance properties of Miller-Morita-Mumford characteristic numbers of fibre bundles
Thomas Church, Martin Crossley, Jeffrey Giansiracusa
Characteristic classes of fibre bundles in the category of closed oriented manifolds give rise to characteristic numbers by integrating the classes over the base.…
Magnetic Flux Transport by turbulent reconnection in astrophysical flows
Elisabete M. de Gouveia Dal Pino, Márcia R. M. Leão, Reinaldo Santos-Lima +3
The role of MHD turbulence in astrophysical environments is still highly debated. An important question that permeates this debate is the transport of magnetic flux. This is partic…
Magnetic Fields in Population III Star Formation
Matthew J. Turk, Jeffrey S. Oishi, Tom Abel +1
We study the buildup of magnetic fields during the formation of Population III star-forming regions, by conducting cosmological simulations from realistic initial conditions and va…