1.4k citations
- University of Colorado BoulderUS66 papers
- California Institute of TechnologyUS14 papers
- University of TorontoCA14 papers
- Goddard Space Flight CenterUS13 papers
- University of California, BerkeleyUS13 papers
- University of ChicagoUS11 papers
- University of ArizonaUS10 papers
- Center for Astrophysics Harvard & SmithsonianUS9 papers
- The University of Texas at AustinUS9 papers
- University of VictoriaCA9 papers
- Centre National de la Recherche ScientifiqueFR8 papers
- National Radio Astronomy ObservatoryUS8 papers
9 papers · 1 filter
Solar Wind Driving of Magnetospheric ULF Waves: Pulsations Driven by Velocity Shear at the Magnetopause
S. G. Claudepierre, S. R. Elkington, M. Wiltberger
We present results from global, three-dimensional magnetohydrodynamic (MHD) simulations of the solar wind/magnetosphere interaction. These MHD simulations are used to study ultra l…
Magnetospheric Cavity Modes Driven by Solar Wind Dynamic Pressure Fluctuations
S. G. Claudepierre, M. Wiltberger, S. R. Elkington +2
We present results from Lyon-Fedder-Mobarry (LFM) global, three-dimensional magnetohydrodynamic (MHD) simulations of the solar wind-magnetosphere interaction. We use these simulati…
Spitzer Mapping of PAHs and H2 in Photodissociation Regions
Brian T. Fleming, Kevin France, Roxana E. Lupu +1
The mid-infrared (MIR) spectra of dense photodissociation regions (PDRs) are typically dominated by emission from polycyclic aromatic hydrocarbons (PAHs) and the lowest pure rotati…
Influence of Hot Plasma Pressure on the Global Structure of Saturn's Magnetodisk
N. Achilleos, P. Guio, C. S. Arridge +4
Using a model of force balance in Saturn's disk-like magnetosphere, we show that variations in hot plasma pressure can change the magnetic field configuration. This effect changes…
Merging and Clustering of the Swift BAT AGN Sample
Michael Koss, Richard Mushotzky, Sylvain Veilleux +1
We discuss the merger rate, close galaxy environment, and clustering on scales up to a Mpc of the SWIFT BAT hard X-ray sample of nearby (z<0.05), moderate-luminosity active galacti…
The Evolution of the UV Luminosity Function from z ~ 0.75 to z ~ 2.5 using HST ERS WFC3/UVIS Observations
P. A. Oesch, R. J. Bouwens, C. M. Carollo +7
We present UV luminosity functions (LFs) at 1500 Angstrom derived from the HST Early Release Science WFC3/UVIS data acquired over ~50 arcmin^2 of the GOODS-South field. The LFs are…