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Journal Article
The Astrophysical Journal Letters, ISSN 2041-8205, 08/2011, Volume 736, Issue 2, p. L24
Journal Article
ASTROPHYSICAL JOURNAL LETTERS, ISSN 2041-8205, 06/2012, Volume 752, Issue 1
Spicules are long, thin, highly dynamic features that jut out ubiquitously from the solar limb. They dominate the interface between the chromosphere and corona... 
Sun: oscillations | HIGH-RESOLUTION OBSERVATIONS | Sun: corona | CORONA | SOLAR SPICULES | Sun: chromosphere | ATMOSPHERE | ALFVEN WAVES | Sun: magnetic topology | CHROMOSPHERE | COUNTERPARTS | ASTRONOMY & ASTROPHYSICS | MAGNETOACOUSTIC SHOCKS | DYNAMIC FIBRILS | VELOCITIES
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 06/2012, Volume 752, Issue 1, pp. L12 - 6
Journal Article
Astrophysical Journal, ISSN 0004-637X, 06/2016, Volume 824, Issue 2, p. 65
Solar spicules are chromospheric fibrils that appear everywhere on the Sun, yet their origin is not understood. Using high resolution observations of spicules... 
Sun: atmosphere | Sun: chromosphere | FINE-STRUCTURE | MAGNETIC-FIELDS | TEMPORAL EVOLUTION | TRANSITION REGION MODELS | DOWNFLOW | ATMOSPHERE | DISK COUNTERPART | ASTRONOMY & ASTROPHYSICS | DYNAMICS | SOLAR CHROMOSPHERE | QUIET SUN | Physics - Solar and Stellar Astrophysics
Journal Article
Astrophysical Journal, ISSN 0004-637X, 03/2018, Volume 856, Issue 1, p. 44
In addition to their jet-like dynamic behavior, spicules usually exhibit strong transverse speeds, multi-stranded structure, and heating from chromospheric to... 
Sun: oscillations | Sun: activity | Sun: corona | instabilities | magnetohydrodynamics (MHD) | Sun: chromosphere | INSTABILITY | INTERFACE-REGION | ALFVENIC WAVES | HINODE | MISSION | KINK OSCILLATIONS | CORONA | SOLAR OPTICAL TELESCOPE | SMALL-SCALE | CHROMOSPHERE | ASTRONOMY & ASTROPHYSICS | Physics - Solar and Stellar Astrophysics
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 01/2015, Volume 573, p. A4
Context. For investigating spicules from the photosphere to coronal heights, the new Hinode/SOT long series of high-resolution observations from space taken in... 
Sun chromosphere | Sun: transition region | MACROSPICULES | MOTIONS | Sun: chromosphere | LIMB | SURGES | MODELS | H-ALPHA SPICULES | ASTRONOMY & ASTROPHYSICS | SOT | OSCILLATIONS | DISK | SOLAR CHROMOSPHERE | Photosphere | Wave propagation | Fuelling | Emission | Helical | Polar regions | Astronomy | Spicules | Physics - Solar and Stellar Astrophysics
Journal Article
Journal Article
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 09/2014, Volume 792, Issue 1, pp. 1 - 6
Journal Article
Astrophysical Journal, ISSN 0004-637X, 01/2018, Volume 853, Issue 1, p. 61
Ubiquitous transverse oscillations observed in spicular waveguides, identified as the kink wave-mode had previously been reported along with periodic... 
Sun: oscillations | magnetohydrodynamics (MHD) | Sun: chromosphere | MAGNETIC TUBES | TRANSVERSE PERTURBATIONS | ALFVENIC WAVES | CHROMOSPHERE | ASTRONOMY & ASTROPHYSICS | DYNAMICAL RESPONSE | FLUX TUBES | SOLAR SPICULES | KINK WAVES
Journal Article
Journal Article
SCIENCE, ISSN 0036-8075, 11/2019, Volume 366, Issue 6467, pp. 890 - 890
Spicules are rapidly evolving fine-scale jets of magnetized plasma in the solar chromosphere. It remains unclear how these prevalent jets originate from the... 
ORIGIN | SCALE MAGNETIC LOOPS | FLUX EMERGENCE | QUIET-SUN | MULTIDISCIPLINARY SCIENCES | JETS | ACTIVE-REGION | MODEL | Magnetic flux | Solar corona | Chromosphere | Solar physics | Spicules | Solar activity | Observatories | Atmospheric heating | Solar surface | Atmosphere | Polarity | Jets | Solar atmosphere | Magnetic fields | Solar magnetic field | Solar observatories
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 09/2016, Volume 828, Issue 1, pp. L9 - L9
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 11/2009, Volume 705, Issue 1, pp. 272 - 284
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 07/2019, Volume 627, p. L5
A solar filament is a dense cool condensation that is supported and thermally insulated by magnetic fields in the rarefied hot corona. Its evolution and... 
waves | Sun: atmosphere | ENERGY | Sun: corona | THREADS | Sun: magnetic fields | CHROMOSPHERE | ASTRONOMY & ASTROPHYSICS | prominences | CORONA | turbulence | Sun: filaments | Physics - Solar and Stellar Astrophysics
Journal Article