14.2k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Goddard Space Flight CenterUS361 papers
- Marshall Space Flight CenterUS357 papers
- Centre National de la Recherche ScientifiqueFR280 papers
- Max Planck Institute for Extraterrestrial PhysicsDE240 papers
- University of Maryland, College ParkUS239 papers
- Universities Space Research AssociationUS214 papers
- Stanford UniversityUS212 papers
- National Institute for AstrophysicsIT196 papers
- University of Rome Tor VergataIT184 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR179 papers
- University of PaduaIT178 papers
- Istituto Nazionale di Fisica Nucleare, Roma Tor VergataIT175 papers
7 papers · 2 filters
Measurements of the Sun's High Latitude Meridional Circulation
Lisa Rightmire-Upton, David H. Hathaway, Katie Kosak
The meridional circulation at high latitudes is crucial to the build-up and reversal of the Sun's polar magnetic fields. Here we characterize the axisymmetric flows by applying a m…
The Morphologic Properties of Magnetic networks over the Solar Cycle 23
Chong Huang, Yihua Yan, Yin Zhang +2
The morphologic properties of the magnetic networks during Carrington Rotations (CR) 1955 to 2091 (from 1999 to 2010) have been analyzed by applying the watershed algorithm to magn…
Trajectories and Distribution of Interstellar Dust Grains in the Heliosphere
Jonathan D. Slavin, Priscilla C. Frisch, Hans-Reinhard Mueller +4
The solar wind carves a bubble in the surrounding interstellar medium (ISM), known as the heliosphere. Charged interstellar dust grains (ISDG) encountering the heliosphere may be d…
Study of the 3D Coronal Magnetic Field of Active Region 11117 Around the Time of a Confined Flare Using a Data-Driven CESE--MHD Model
Chaowei Jiang, Xueshang Feng, S. T. Wu +1
We apply a data-driven MHD model to investigate the three-dimensional (3D) magnetic field of NOAA active region (AR) 11117 around the time of a C-class confined flare occurred on 2…
Radio signatures of CME-streamer interaction and source diagnostics of type II radio burst
S. W. Feng, Y. Chen, X. L. Kong +4
It has been suggested that type II radio bursts are due to energetic electrons accelerated at coronal shocks. Radio observations, however, have poor or no spatial resolutions to pi…
A broken solar type II radio burst induced by a coronal shock propagating across the streamer boundary
Xiang-Liang Kong, Yao Chen, Gang Li +4
We discuss an intriguing type II radio burst that occurred on 2011 March 27. The dynamic spectrum was featured by a sudden break at about 43 MHz on the well-observed harmonic branc…
Precise Infrared Radial Velocities from Keck/NIRSPEC and the Search for Young Planets
John I. Bailey, Russel J. White, Cullen H. Blake +4
We present a high-precision infrared radial velocity study of late-type stars using spectra obtained with NIRSPEC at the W. M. Keck Observatory. Radial velocity precisions of 50 m/…