14.2k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- California Institute of TechnologyUS282 papers
- Goddard Space Flight CenterUS278 papers
- University of MichiganUS253 papers
- Centre National de la Recherche ScientifiqueFR249 papers
- University of Maryland, College ParkUS248 papers
- Pennsylvania State UniversityUS242 papers
- Northwestern UniversityUS236 papers
- University of Wisconsin–MilwaukeeUS235 papers
- Rochester Institute of TechnologyUS227 papers
- Stanford UniversityUS227 papers
- Columbia UniversityUS225 papers
- Max Planck Institute for Gravitational PhysicsDE225 papers
10 papers · 2 filters
Determination of the Coronal Magnetic Field by Hot Loop Oscillations
Tongjiang Wang, Davina E. Innes, Jiong Qiu
We apply a new method to determine the magnetic field in coronal loops using observations of coronal loop oscillations. We analyze seven Doppler shift oscillation events detected b…
A Solution to the Galactic Foreground Problem for LISA
Jeff Crowder, Neil Cornish
Low frequency gravitational wave detectors, such as the Laser Interferometer Space Antenna (LISA), will have to contend with large foregrounds produced by millions of compact galac…
Sloan/Johnson-Cousins/2MASS Color Transformations for Cool-Stars
James R. A. Davenport, Andrew A. West, Caleb K. Matthiesen +2
We present multi-color transformations and photometric parallaxes for a sample of 40 low mass dwarfs selected from the Sloan Digital Sky Survey (SDSS) and the General Catalog of Tr…
Production of high-energy μneutrinos from young neutron stars
G. F. Burgio, B. Link
Young, rapidly rotating neutron stars could accelerate protons to energies of PeV close to the stellar surface, which scatter with x-rays from the stellar surface through…
Fluxon Modeling of Low-Beta Plasmas
Craig E. DeForest, Charles C. Kankelborg
We have developed a new, quasi-Lagrangian approach for numerical modeling of magnetohydrodynamics in low to moderate plasmas such as the solar corona. We introduce the concept…
Evidence for Heating of Neutron Stars by Magnetic Field Decay
J. A. Pons, B. Link, J. A. Miralles +1
We show the existence of a strong trend between neutron star surface temperature and the dipolar component of the magnetic field extending through three orders of field magnitude,…
A strong correlation in radio pulsars with implications for torque variations
J. O. Urama, B. Link, J. M. Weisberg
We present an analysis of the spin-down parameters for 131 radio pulsars for which has been well determined. These pulsars have characteristic ages ranging from $10^{3} -…
Extending the WMAP Bound on the Size of the Universe
Joey Shapiro Key, Neil J. Cornish, David N. Spergel +1
Clues to the shape of our Universe can be found by searching the CMB for matching circles of temperature patterns. A full sky search of the CMB, mapped extremely accurately by NASA…
Recent Developments in Neutron Star Thermal Evolution Theories and Observation
Sachiko Tsuruta
Recent years have seen some significant progress in theoretical studies of physics of dense matter. Combined with the observational data now available from the successful launch of…
Magnetohydrodynamic Shocks in Non-Equatorial Plasma Flows around a Black Hole
Keigo Fukumura, Masaaki Takahashi, Sachiko Tsuruta
We study magnetohydrodynamic (MHD) standing shocks in inflowing plasmas in a black hole magnetosphere. Fast and intermediate shock formation is explored in Schwarzschild and Kerr g…