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PLoS ONE, ISSN 1932-6203, 2013, Volume 8, Issue 2, p. e57395
Journal Article
Journal of Geophysical Research - Space Physics, ISSN 0148-0227, 04/2010, Volume 115, Issue A4, p. n/a
Observations of the solar wind plasma at 0.3 AU and beyond show that a turbulent spectrum of magnetic fluctuations is present. Remote sensing observations of... 
Solar Physics | wave heating | hybrid simulation studies | solar wind | ACCELERATION | DISTRIBUTIONS | SPECTROMETER | ASTRONOMY & ASTROPHYSICS | CORONAL LOOPS | CONSTRAINTS | IONS | SIMULATIONS | ELECTROMAGNETIC PROTON/PROTON INSTABILITIES | ANISOTROPY | ULYSSES | Space | Plasma physics | Astrophysics | Kinetics | Planetology
Journal Article
Journal of Geophysical Research: Space Physics, ISSN 2169-9380, 04/2019, Volume 124, Issue 4, pp. 2393 - 2405
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 03/2009, Volume 694, Issue 1, pp. 502 - 511
The multithreaded structure of active region coronal loops was deduced from past spectroscopic observations. Recent high-resolution observations by Transition... 
Sun: flares | MHD | Sun: corona | Waves | Sun: magnetic fields | waves | RESONANT ABSORPTION | TRACE | SOLAR ATMOSPHERE | KINK OSCILLATIONS | SEISMOLOGY | ALFVEN WAVES | ASTRONOMY & ASTROPHYSICS | TRANSVERSE OSCILLATIONS | MAGNETIC-FIELD | ACTIVE-REGION | SCALING LAWS
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 03/2019, Volume 623, p. A95
During solar minimum activity, the coronal structure is dominated by a tilted streamer belt, associated with the sources of the slow solar wind. It is known... 
Magnetohydrodynamics (MHD) | Sun: UV radiation | Sun: corona | Solar wind | MINIMUM | ASTRONOMY & ASTROPHYSICS | IONS | magnetohydrodynamics (MHD) | MULTI-FLUID MODEL | solar wind | SLOW SOLAR-WIND
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 02/2007, Volume 655, Issue 2 I, pp. 1134 - 1141
MHD wave activity associated with a flare was observed in coronal active region AR 8270 in the extreme ultraviolet (EUV) by the Transition Region and Coronal... 
Sun: flares | MHD | Sun: corona | Waves | Sun: magnetic fields | waves | RESONANT ABSORPTION | VERTICAL OSCILLATIONS | TRANSITION-REGION | Sun : flares | LOOP OSCILLATIONS | Sun : corona | ALFVEN WAVES | Sun : magnetic fields | SOLAR-FLARE | ASTRONOMY & ASTROPHYSICS | BRAGG CRYSTAL SPECTROMETER | TRANSVERSE OSCILLATIONS | NUMERICAL SIMULATIONS | DOPPLER-SHIFT OSCILLATIONS
Journal Article
Journal of Geophysical Research - Space Physics, ISSN 0148-0227, 07/2004, Volume 109, Issue A7, pp. A07102 - n/a
Journal Article
by Ofman, L and Sui, L
The Astrophysical Journal Letters, ISSN 1538-4357, 06/2006, Volume 644, Issue 2, pp. L149 - L152
Journal Article
The Astrophysical Journal Letters, ISSN 1538-4357, 11/2002, Volume 580, Issue 1, pp. L85 - L88
Journal Article
Journal of Geophysical Research: Space Physics, ISSN 2169-9380, 05/2013, Volume 118, Issue 5, pp. 1828 - 1836
Quasi‐perpendicular collisionless shocks undergo structural changes with the increase of the Mach number. These changes are related to the increasing role of... 
Collisionless shocks | 2.5D hybrid models | Ion velocity distributions | BOW SHOCK | WAVES | THERMALIZATION | ASTRONOMY & ASTROPHYSICS | MAGNETIC-FIELD | MACH-NUMBER | 5D hybrid models | NONSTATIONARITY | BETA | Aerodynamics | Ions | Geophysics | Ramps | Simulation | Shock fronts | Oscillations | Two dimensional | Ion distribution | Gyration | Mach number
Journal Article