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Astronomy and Astrophysics, ISSN 0004-6361, 2011, Volume 531, Issue A154
Journal Article
Science, ISSN 0036-8075, 1/2011, Volume 331, Issue 6013, pp. 55 - 58
The Sun's outer atmosphere, or corona, is heated to millions of degrees, considerably hotter than its surface or photosphere. Explanations for this enigma... 
High temperature plasmas | Solar corona | Chromosphere | Plasma jets | Temperature | Solar temperature | Astrophysics | REPORTS | Coronal holes | Plasma temperature | Solar observatories | SPICULES | MODEL | TRANSITION REGION | MISSION | MULTIDISCIPLINARY SCIENCES | Thermal properties | Composition | Corona | Sun | Natural history | Plasma | Solar physics
Journal Article
Solar Physics, ISSN 0038-0938, 7/2014, Volume 289, Issue 7, pp. 2733 - 2779
Journal Article
Science, ISSN 0036-8075, 06/2017, Volume 356, Issue 6344, pp. 1269 - 1272
In the lower solar atmosphere, the chromosphere is permeated by jets known as spicules, in which plasma is propelled at speeds of 50 to 150 kilometers per... 
CORONA | POWER | SIMULATION | MULTIDISCIPLINARY SCIENCES | REGION | Observations | Wave-motion, Theory of | Solar atmosphere | Solar corona | Magnetohydrodynamics | Chromosphere | Fluid dynamics | Fluid flow | Radiation | Waves | Plasma (physics) | Spicules | Physics | Solar phenomena | Atmosphere | Ambipolar diffusion | Tension | Diffusion | Magnetic fields | Solar wind | Magnetic properties | Coronas | Simulation | Jets | Formations
Journal Article
Journal Article
Science, ISSN 0036-8075, 12/2007, Volume 318, Issue 5856, pp. 1574 - 1577
Alfvén waves have been invoked as a possible mechanism for the heating of the Sun's outer atmosphere, or corona, to millions of degrees and for the... 
Amplitude | Observational astronomy | Chromosphere | Monte Carlo methods | Observational research | Spacetime | Reports | Wave velocity | Magnetic fields | Space research | Solar wind | ACCELERATION | SPICULES | MODELS | MULTIDISCIPLINARY SCIENCES | PARAMETRIC DECAY | DRIVEN | ATMOSPHERE | Solar flares | Research | Properties | Magnetohydrodynamic waves | Magnetic properties | Wind | Astrophysics | Sun | Atmosphere
Journal Article
Astrophysical Journal, ISSN 0004-637X, 04/2017, Volume 839, Issue 1, p. 22
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 09/2009, Volume 702, Issue 1, pp. 1 - 18
We present the results of numerical simulations of wave-induced magnetic reconnection in a model of the solar atmosphere. In the magnetic field geometry we... 
MHD | Sun: transition region | Magnetic fields | Sun: chromosphere | SPICULES | magnetic fields | PHOTOSPHERIC MAGNETIC-FIELD | CORONA | 2D ENVIRONMENT | ATMOSPHERE | EVOLUTION | ASTRONOMY & ASTROPHYSICS | EXPLOSIVE EVENTS | JETS | DYNAMIC FIBRILS | QUIET SUN | Physics - Solar and Stellar Astrophysics
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 09/2007, Volume 666, Issue 2 I, pp. 1277 - 1283
We present the results of numerical simulations of shock wave-driven jets in the solar atmosphere. The dependence of observable quantities such as maximum... 
MHD | Shock waves | Magnetic fields | Sun: chromosphere | SPICULES | magnetic fields | FINE-STRUCTURE | CORONA | MOTTLES | EVOLUTION | PHOTOSPHERIC OSCILLATIONS | ASTRONOMY & ASTROPHYSICS | MAGNETOACOUSTIC SHOCKS | Sun : chromosphere | SOLAR CHROMOSPHERE | DYNAMIC FIBRILS | shock waves
Journal Article