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Astronomy and Astrophysics, ISSN 0004-6361, 11/2018, Volume 619, p. L6
Journal Article
Astrophysical Journal, ISSN 0004-637X, 07/2015, Volume 808, Issue 1
Journal Article
Astrophysical Journal, ISSN 0004-637X, 01/2018, Volume 852, Issue 2, p. 69
The recent availability of fine-grained high-sensitivity data from the new generation of low radio frequency instruments such as the Murchison Widefield Array... 
Sun: flares | Sun: activity | Sun: corona | Sun: radio radiation | NANOFLARES | ASTRONOMY & ASTROPHYSICS | BRIGHTNESS TEMPERATURE | BURSTS | MICROFLARES | QUIET SUN
Journal Article
Publications of the Astronomical Society of Japan, ISSN 0004-6264, 12/2013, Volume 65, Issue sp1, p. S18
The Chinese Spectral Radioheliograph (CSRH) is a solar-dedicated interferometric array with a frequency range from 400MHz to 15 GHz. There are 40 4.5m antennas... 
Methods: observational | Sun: radio radiation
Journal Article
Astrophysical Journal, ISSN 0004-637X, 07/2012, Volume 753, Issue 1
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2019, Volume 622, p. A150
Solar observations with the Atacama Large Millimeter/submillimeter Array (ALMA) provide us with direct measurements of the brightness temperature in the solar... 
Sun: transition region | Sun: UV radiation | Sun: chromosphere | Sun: radio radiation | WAVES | TRANSITION REGION | ASTRONOMY & ASTROPHYSICS | DYNAMICS | MODEL | EMISSION | Physics - Solar and Stellar Astrophysics
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2015, Volume 575, p. A15
Aims. We use advanced 3D non-local thermodynamic equilibrium radiative magnetohydrodynamic simulations of the solar atmosphere to carry out detailed tests of... 
Sun: atmosphere | Sun: magnetic fields | Sun: chromosphere | Sun: radio radiation | Chromosphere | Wavelengths | Brightness | Radio telescopes | Solar atmosphere | Formations | Diagnostic systems | Arrays | Physics - Solar and Stellar Astrophysics
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 0004-6361, 03/2015, Volume 575
Aims. We use advanced 3D non-local thermodynamic equilibrium radiative magnetohydrodynamic simulations of the solar atmosphere to carry out detailed tests of... 
HYDROGEN IONIZATION | Sun: chromosphere | REGION | Sun: atmosphere | IRIS | K LINES | Sun: magnetic fields | CHROMOSPHERE | ASTRONOMY & ASTROPHYSICS | DYNAMICS | MG II | SIMULATIONS | EMISSION | Sun: radio radiation
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 05/2017, Volume 601, p. 1DUMMY
Aims. We use state-of-the-art, three-dimensional non-local thermodynamic equilibrium (non-LTE) radiative magnetohydrodynamic simulations of the quiet solar... 
Sun: Chromosphere | Sun: Atmosphere | Sun: Magnetic fields | Sun: Radio radiation | RADIO OBSERVATIONS | ACTIVE REGIONS | C II | Sun: chromosphere | ALPHA LINE | Sun: atmosphere | IRIS | K LINES | Sun: magnetic fields | ASTRONOMY & ASTROPHYSICS | 133.5 NM | GENERAL FORMATION PROPERTIES | MG II | EMISSION | Sun: radio radiation | Physics - Solar and Stellar Astrophysics
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 10/2018, Volume 618, p. A60
Aims. The zebra structures observed in radio waves during solar flares are some of the most important structures used as diagnostics of solar flare plasmas. We... 
Sun: flares | Sun: radio radiation | INSTABILITY | FINE-STRUCTURE | BURSTS | CORONA | PATTERNS | MODEL | RADIATION | REGION | ASTRONOMY & ASTROPHYSICS | MAGNETIC-FIELD | SPECTRA
Journal Article
Astrophysical Journal, ISSN 0004-637X, 09/2018, Volume 864, Issue 2, p. 122
The source regions of solar type III radio bursts are regions of very intense Langmuir wave packets excited by the bump-on-tail distributions of energetic... 
Sun: flares | Sun: radio radiation | WIND | ELECTRONS | STABILITY | INTERPLANETARY PLASMA | RADIATION | SPATIAL COLLAPSE | ASTRONOMY & ASTROPHYSICS | MAGNETIC-FIELD | TURBULENCE | WAVE COLLAPSE | CONTINUOUS MEDIA
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 04/2019, Volume 875, Issue 2, p. 98
At the site of their origin, solar meter-wave radio bursts contain pristine information about the local coronal magnetic field and plasma parameters. On its... 
Sun: flares | Sun: oscillations | Sun: corona | CORONA | ACCELERATION | SPACE | POSITION | Sun: fundamental parameters | PLASMA | ASTRONOMY & ASTROPHYSICS | FREQUENCY | EMISSION | PULSATIONS | Sun: radio radiation | techniques: interferometric | SCATTERING | PROPAGATION
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 04/2019, Volume 624, p. A119
Context. Radio bursts with fine structures are used in diagnostics of solar flare plasmas, of which zebra structures are the most important. However, there is... 
Sun: flares | INSTABILITY | FINE-STRUCTURE | FIELD | ASTRONOMY & ASTROPHYSICS | CORONA | PATTERNS | EMISSION | Sun: radio radiation | REGION
Journal Article
Journal Article
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