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Astronomy and Astrophysics, ISSN 0004-6361, 2012, Volume 548, p. A62
Context. We study the magnetic properties of small-scale transients in coronal holes and a few in the quiet Sun identified in X-ray observations and... 
Methods: observational | Magnetic fields | Sun: corona | Sun: chromosphere | Sun: evolution | methods: observational | magnetic fields | X-RAY JETS | FLUX | SOLAR OPTICAL TELESCOPE | REGION | EVOLUTION | QUIET-SUN | ASTRONOMY & ASTROPHYSICS | DYNAMICS-OBSERVATORY SDO | HINODE MISSION | POINTS | TEMPORAL VARIATIONS | Physics - Solar and Stellar Astrophysics
Journal Article
Astrophysical Journal, ISSN 0004-637X, 04/2018, Volume 857, Issue 2, p. 130
We used our newly developed magnetohydrodynamic (MHD) code to perform 2.5D simulations of a fast-mode MHD wave interacting with coronal holes (CHs) of varying... 
waves | Sun: corona | magnetohydrodynamics (MHD) | Sun: evolution | MECHANISM | CMES | QUADRATURE OBSERVATIONS | SHOCK-WAVES | SOLAR CORONA | SOHO MISSION | ASTRONOMY & ASTROPHYSICS | ULTRAVIOLET IMAGING TELESCOPE | MASS EJECTION | STEREO | EIT WAVES
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 04/2007, Volume 658, Issue 2 I, pp. 1340 - 1348
In a recent study of the 2006 solar eclipse, we noted that there are two kinds of coronal streamers: "helmet streamers,'' which separate coronal holes of... 
Sun: corona | Solar wind | Sun: magnetic fields | POLAR PLUMES | WHITE-LIGHT | HOLES | STREAMERS | solar wind | 3-DIMENSIONAL STRUCTURE | Sun : corona | INTERPLANETARY MAGNETIC-FIELD | EVOLUTION | Sun : magnetic fields | ASTRONOMY & ASTROPHYSICS | SOLAR-WIND | JETS | HELIOSPHERIC CURRENT SHEET
Journal Article
Solar Physics, ISSN 0038-0938, 2010, Volume 264, Issue 1, pp. 189 - 237
Journal Article
Solar Physics, ISSN 0038-0938, 12/2008, Volume 253, Issue 1, pp. 215 - 235
Journal Article
The Astrophysical Journal Letters, ISSN 1538-4357, 08/2009, Volume 701, Issue 1, pp. L1 - L6
The Sun's corona is millions of degrees hotter than its 5000 K photosphere. This heating enigma is typically addressed by invoking the deposition at coronal... 
Sun: transition region | Sun: atmospheric motions | Sun: corona | Sun: magnetic fields | Sun: chromosphere | TRACE | SPICULES | SUMER | HINODE | MISSION | RESOLUTION | TRANSITION REGION MOSS | ATMOSPHERE | MODELS | ASTRONOMY & ASTROPHYSICS | DYNAMIC FIBRILS | Physics - Solar and Stellar Astrophysics
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 06/2019, Volume 626, p. A67
Context. Solar photospheric magnetic fields have been observed since the 1950s and calibrated digital data are available from the 1970s onwards. Synoptic maps... 
SOURCE SURFACE | Sun: corona | Sun: magnetic fields | ASTRONOMY & ASTROPHYSICS | SOLAR | INTERPLANETARY | FLUX | Sun: photosphere | MODEL | Sun: activity
Journal Article
Astrophysical Journal, ISSN 0004-637X, 11/2017, Volume 850, Issue 1, p. 88
We have developed a new numerical code that is able to perform 2.5D simulations of a magnetohydrodynamic (MHD) wave propagation in the corona, and its... 
waves | Sun: corona | magnetohydrodynamics (MHD) | Sun: evolution | SOHO/EIT OBSERVATIONS | QUADRATURE OBSERVATIONS | SHOCK-WAVES | SOLAR CORONA | PROPAGATING DISTURBANCE | MHD WAVES | ASTRONOMY & ASTROPHYSICS | ULTRAVIOLET IMAGING TELESCOPE | MASS EJECTION | MORETON WAVES | EIT WAVES | Physics - Solar and Stellar Astrophysics
Journal Article
Science, ISSN 0036-8075, 8/1999, Volume 285, Issue 5429, pp. 862 - 864
The imaging telescope on board the Transition Region and Coronal Explorer (TRACE) spacecraft observed the decaying transversal oscillations of a long [(130 ±... 
Viscosity | Solar corona | Power laws | Coronal loops | Solar flares | Classical mechanics | Spacecraft | Reports | Magnetic fields | Coefficients | Sunspots | RESONANT ABSORPTION | ALFVEN WAVES | DRIVEN | MULTIDISCIPLINARY SCIENCES | SOLAR CORONA | SCALING LAWS | Space vehicles | Corona | Research | Observations | Sun | Solar wind | Temperature | Atmosphere
Journal Article
Astrophysical Journal, ISSN 0004-637X, 04/2012, Volume 749, Issue 1, pp. 40 - 14
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 09/2017, Volume 605, p. A8
We proposed that the use of an approximate "jump condition" at the solar transition region permits fast and accurate numerical solutions of the one dimensional... 
Magnetohydrodynamics (MHD) | Sun: Chromosphere | Sun: Magnetic fields | Sun: Corona | PLASMA | Sun: corona | Sun: magnetic fields | ASTRONOMY & ASTROPHYSICS | SIMULATIONS | LOOPS | magnetohydrodynamics (MHD) | Sun: chromosphere | Physics - Solar and Stellar Astrophysics
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2017, Volume 598, p. A3
Context. Coronal dimmings are regions of decreased extreme-ultravoilet (EUV) and/or X-ray (originally Skylab, then Yohkoh/SXT) intensities, which are often... 
Sun: flares | Sun: corona | Sun: coronal mass ejections (CMEs) | SOLAR-FLARES | CHROMOSPHERIC EVAPORATION | SLIPPING MAGNETIC RECONNECTION | EIT | EXTREME-ULTRAVIOLET WAVE | ASTRONOMY & ASTROPHYSICS | FILAMENT | MASS EJECTION | DYNAMICS | FLUX ROPES | ONSET | Physics - Solar and Stellar Astrophysics
Journal Article