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Science (American Association for the Advancement of Science), ISSN 1095-9203, 2007, Volume 317, Issue 5842, pp. 1192 - 1196
Alfvén waves, transverse incompressible magnetic oscillations, have been proposed as a possible mechanism to heat the Sun's corona to millions of degrees by transporting convective energy... 
Speed | Solar corona | Wave propagation | Wavelengths | Emission spectra | Linear polarization | Reports | Wave velocity | Magnetic fields | Waves | Pixels | MAGNETOHYDRODYNAMIC WAVES | CHROMOSPHERE | MULTIDISCIPLINARY SCIENCES | TRANSITION-REGION | FREQUENCY | SUN | DYNAMIC FIBRILS | LINES | LOOP OSCILLATIONS | Polarization | Corona | Research | Magnetohydrodynamic waves | Sun | Electromagnetic waves | Astrophysics | Estimates
Journal Article
Science (American Association for the Advancement of Science), ISSN 1095-9203, 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... 
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
The Astrophysical journal, ISSN 1538-4357, 2012, Volume 761, Issue 2, pp. 138 - 8
Journal Article
Nature (London), ISSN 0028-0836, 01/2019, Volume 565, Issue 7738, pp. 198 - 201
The geometry of the accretion flow around stellar-mass black holes can change on timescales of days to months1,2,3. When a black hole emerges from quiescence... 
VARIABILITY | OUTBURSTS | REFLECTION | EVOLUTION | MULTIDISCIPLINARY SCIENCES | TIME-LAGS | X-RAY REVERBERATION | IRON K | ACCRETION | MODEL | EMISSION | Observations | Black holes (Astronomy) | Neutron stars | Accretion | Black holes | Space telescopes | Iron | Stellar coronas | X-ray spectrum | Accretion disks | Reverberation time | Emissions | Reduction | Corona | Gravity | Physics - High Energy Astrophysical Phenomena
Journal Article
Space Science Reviews, ISSN 0038-6308, 11/2012, Volume 172, Issue 1, pp. 169 - 185
Determining how the heliospheric magnetic field and plasma connect to the Sun’s corona and photosphere is, perhaps, the central problem in solar and heliospheric physics... 
Extraterrestrial Physics, Space Sciences | Sun: solar wind | Astrophysics and Astroparticles | Planetology | Sun: corona | Aerospace Technology and Astronautics | Physics | MASS EJECTIONS | DISCONNECTION | RECONNECTION | FLUX | SUN | FLOW | ACCELERATION | MODELS | ASTRONOMY & ASTROPHYSICS | MAGNETIC-FIELD | SLOW SOLAR-WIND | Plasma | Corona | Magnetic fields | Sun | Heliosphere | Photosphere | Coronas | Computer simulation | Dynamics | Mathematical models | Joints
Journal Article
Journal of geophysical research. Planets, ISSN 2169-9097, 05/2014, Volume 119, Issue 5, pp. 905 - 924
Journal Article
The Astrophysical journal, ISSN 1538-4357, 2009, Volume 697, Issue 2, pp. 1384 - 1391
...) instrument to perform time-distance seismology of the solar corona. We construct the first k-omega diagrams of the region... 
Sun: corona