2.5k citations
- Goddard Space Flight CenterUS263 papers
- United States Naval Research LaboratoryUS182 papers
- Centre National de la Recherche ScientifiqueFR152 papers
- Center for Astrophysics Harvard & SmithsonianUS146 papers
- University of Maryland, College ParkUS143 papers
- California Institute of TechnologyUS136 papers
- Ames Research CenterUS107 papers
- Massachusetts Institute of TechnologyUS107 papers
- Princeton UniversityUS104 papers
- University of California, BerkeleyUS85 papers
- University of California, Santa CruzUS81 papers
- Search for Extraterrestrial IntelligenceUS74 papers
5 papers · 2 filters
Estimating the Chromospheric Absorption of Transition Region Moss Emission
Bart De Pontieu, Viggo H. Hansteen, Scott W. McIntosh +1
Many models for coronal loops have difficulty explaining the observed EUV brightness of the transition region, which is often significantly less than theoretical models predict. Th…
No Trace Left Behind: Stereo Observation of a Coronal Mass Ejection without Low Coronal Signatures
Eva Robbrecht, Spiros Patsourakos, Angelos Vourlidas
The availability of high quality synoptic observations of the EUV and visible corona during the SOHO mission has advanced our understanding of the low corona manifestations of CMEs…
Hinode/Extreme-Ultraviolet Imaging Spectrometer Observations of the Temperature Structure of the Quiet Corona
David H. Brooks, Harry P. Warren, David R. Williams +1
We present a Differential Emission Measure (DEM) analysis of the quiet solar corona on disk using data obtained by the Extreme-ultraviolet Imaging Spectrometer (EIS) on {\it Hinode…
Flows and Motions in Moss in the Core of a Flaring Active Region: Evidence for Steady Heating
David H. Brooks, Harry P. Warren
We present new measurements of the time variability of intensity, Doppler and non-thermal velocities in moss in an active region core observed by the EUV Imaging Spectrometer on Hi…
Numerical Simulations of Magnetized Winds of Solar-Like Stars
A. A. Vidotto, M. Opher, V. Jatenco-Pereira +1
We investigate magnetized solar-like stellar winds by means of self-consistent three-dimensional (3D) magnetohydrodynamics (MHD) numerical simulations. We analyze winds with differ…