Radio measurements of the magnetic field in the solar chromosphere and the corona
CE Alissandrakis, DE Gary - Frontiers in Astronomy and Space …, 2021 - frontiersin.org
The structure of the upper solar atmosphere, on all observable scales, is intimately governed
by the magnetic field. The same holds for a variety of solar phenomena that constitute solar …
by the magnetic field. The same holds for a variety of solar phenomena that constitute solar …
The first SEPServer event catalogue~ 68-MeV solar proton events observed at 1 AU in 1996–2010
SEPServer is a three-year collaborative project funded by the seventh framework
programme (FP7-SPACE) of the European Union. The objective of the project is to provide …
programme (FP7-SPACE) of the European Union. The objective of the project is to provide …
Fine Structure of Solar Metric Radio bursts: ARTEMIS-IV/JLS and NRH Observations
Radio bursts provide important diagnostics of energetic phenomena of the Sun. In particular,
bursts in decimetric and metric wavelengths probe the physical conditions and the energy …
bursts in decimetric and metric wavelengths probe the physical conditions and the energy …
Properties of solar energetic particle events inferred from their associated radio emission
A Kouloumvakos, A Nindos, E Valtonen… - Astronomy & …, 2015 - aanda.org
Aims. We study selected properties of solar energetic particle (SEP) events as inferred from
their associated radio emissions. Methods. We used a catalogue of 115 SEP events, which …
their associated radio emissions. Methods. We used a catalogue of 115 SEP events, which …
Variable emission mechanism of a Type IV radio burst
DE Morosan, EKJ Kilpua, EP Carley… - Astronomy & …, 2019 - aanda.org
Context. The Sun is an active star and the source of the largest explosions in the solar
system, such as flares and coronal mass ejections (CMEs). Flares and CMEs are powerful …
system, such as flares and coronal mass ejections (CMEs). Flares and CMEs are powerful …
IPRT/AMATERAS: A new metric spectrum observation system for solar radio bursts
K Iwai, F Tsuchiya, A Morioka, H Misawa - Solar Physics, 2012 - Springer
A new radio spectropolarimeter for solar radio observation has been developed at Tohoku
University and installed on the Iitate Planetary Radio Telescope (IPRT) at the Iitate …
University and installed on the Iitate Planetary Radio Telescope (IPRT) at the Iitate …
CME expansion as the driver of metric type II shock emission as revealed by self-consistent analysis of high-cadence EUV images and radio spectrograms
A Kouloumvakos, S Patsourakos, A Hillaris… - Solar Physics, 2014 - Springer
On 13 June 2010, an eruptive event occurred near the solar limb. It included a small filament
eruption and the onset of a relatively narrow coronal mass ejection (CME) surrounded by an …
eruption and the onset of a relatively narrow coronal mass ejection (CME) surrounded by an …
Observations of low frequency solar radio bursts from the Rosse solar-terrestrial observatory
Abstract The Rosse Solar-Terrestrial Observatory (RSTO; www. rosseobservatory. ie) was
established at Birr Castle, Co. Offaly, Ireland (53° 05′ 38.9 ″, 7° 55′ 12.7 ″) in 2010 to …
established at Birr Castle, Co. Offaly, Ireland (53° 05′ 38.9 ″, 7° 55′ 12.7 ″) in 2010 to …
An eruptive hot-channel structure observed at metric wavelength as a moving Type-IV solar radio burst
ABSTRACT Hot-channel (HC) structure, observed in the high-temperature passbands of the
Atmospheric Imaging Assembly/Solar Dynamic Observatory, is regarded as one candidate …
Atmospheric Imaging Assembly/Solar Dynamic Observatory, is regarded as one candidate …
The relativistic solar particle event of 2005 January 20: origin of delayed particle acceleration
KL Klein, S Masson, C Bouratzis, V Grechnev… - Astronomy & …, 2014 - aanda.org
Context. The highest energies of solar energetic nucleons detected in space or through
gamma-ray emission in the solar atmosphere are in the GeV range. Where and how the …
gamma-ray emission in the solar atmosphere are in the GeV range. Where and how the …