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1992, Cambridge astrophysics series, ISBN 9780521382618, Volume 23, xiv, 276
Book
Astrophysical Journal, ISSN 0004-637X, 04/2016, Volume 820, Issue 2, p. 124
Rapid blue- and redshifted excursions (RBEs and RREs) are likely to be the on-disk counterparts of Type II spicules. Recently, heating signatures from... 
Sun: general | Sun: transition region | Sun: activity | Sun: corona | Sun: chromosphere | solar wind | DISK COUNTERPARTS | IMAGING-SPECTROGRAPH | FINE-STRUCTURE | BLUESHIFTED EXCURSIONS | II SPICULES | TORSIONAL MOTIONS | SWEDISH SOLAR TELESCOPE | EVOLUTION | CHROMOSPHERE | ASTRONOMY & ASTROPHYSICS | DYNAMICS | Physics - Solar and Stellar Astrophysics
Journal Article
Astrophysical Journal, ISSN 0004-637X, 09/2015, Volume 811, Issue 1, pp. 48 - 8
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 01/2014, Volume 780, Issue 1, pp. 1 - 7
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 12/2018, Volume 620, p. A122
Context. Fully fledged sunspots are known to be surrounded by a radial outflow called the moat flow. Aims. We investigate the evolution of the horizontal flow... 
Sun: Photosphere | Sun: Evolution | Sunspots | ASTRONOMY & ASTROPHYSICS | Sun: evolution | MASS | ENERGY-FLOW | Sun: photosphere | sunspots | MOTIONS | Physics - Solar and Stellar Astrophysics
Journal Article
Science, ISSN 0036-8075, 2014, Volume 346, Issue 6207, pp. 1255711 - 1255711
As the interface between the Sun's photosphere and corona, the chromosphere and transition region play a key role in the formation and acceleration of the... 
WIND | SUMER | ENERGY | ORIGIN | ALFVENIC WAVES | MULTIDISCIPLINARY SCIENCES | CORONA | RECONNECTION | POWER | II SPICULES | Wind | Sun | Spectrum analysis | Solar energy | Photosphere | Chromosphere | Small scale | Imaging | Jets | Lanes | Acceleration | Solar wind | Physics - Solar and Stellar Astrophysics
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2018, Volume 610, p. A67
Context. Transition region (TR) spectra typically show the Si IV 1402.8 angstrom line to be enhanced by a factor of 5 or more compared to the neighboring O IV... 
Sun: UV radiation | Radiation mechanisms: Non-thermal | Sun: Transition region | radiation mechanisms non-thermal | EXCITATION | Sun UV radiation | CORONAL LOOPS | RADIATION | FOKKER-PLANCK | FLARE | ASTRONOMY & ASTROPHYSICS | EXTREME-ULTRAVIOLET | SOLAR | EQUILIBRIUM | DENSITY DIAGNOSTICS | EMISSION | Sun transition region | Physics - Solar and Stellar Astrophysics
Journal Article
Astrophysical Journal, ISSN 0004-637X, 03/2018, Volume 855, Issue 1, p. 15
Element abundance ratios of magnesium to neon (Mg/Ne) and neon to oxygen (Ne/O) in the transition region of the quiet Sun have been derived by re-assessing... 
Sun: photosphere | Sun: transition region | Sun: abundances | Sun: UV radiation | RATE COEFFICIENTS | SOLAR MODEL PROBLEM | EMISSION-LINES | NE/O ABUNDANCE | CORONAL HOLE | ATMOSPHERE | OXYGEN | NEON | TEMPERATURE | ASTRONOMY & ASTROPHYSICS | STARS | Physics - Solar and Stellar Astrophysics
Journal Article
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 09/2014, Volume 569, p. L7
Aims. We present observations from the Interface Region Imaging Spectrograph (IRIS) of absorption features from a multitude of cool atomic and molecular lines... 
Sun: UV radiation | Sun: transition region | Sun: chromosphere | MODELS | TEMPERATURE | CHROMOSPHERE | ASTRONOMY & ASTROPHYSICS | ULTRAVIOLET SOLAR SPECTRUM | EMISSION-LINES | SUN | ATMOSPHERE | Physics - Solar and Stellar Astrophysics
Journal Article