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 …
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 …
High resolution observations with Artemis-IV and the NRH-I. Type IV associated narrow-band bursts
Context. Narrow-band bursts appear on dynamic spectra from microwave to decametric
frequencies as fine structures with very small duration and bandwidth. They are believed to …
frequencies as fine structures with very small duration and bandwidth. They are believed to …
The possible effects of the solar and geomagnetic activity on multiple sclerosis
P Papathanasopoulos, P Preka-Papadema… - Clinical Neurology and …, 2016 - Elsevier
Objectives Increasing observational evidence on the biological effects of Space Weather
suggests that geomagnetic disturbances may be an environmental risk factor for multiple …
suggests that geomagnetic disturbances may be an environmental risk factor for multiple …
Fine structure of metric Type IV radio bursts observed with the ARTEMIS-IV radio-spectrograph: association with flares and coronal mass ejections
Fine structures embedded in type IV burst continua may be used as diagnostics of the
magnetic-field restructuring and the corresponding energy release associated with the low …
magnetic-field restructuring and the corresponding energy release associated with the low …
On the onset time of several SPE/GLE events: Indications from high‐energy gamma‐ray and neutron measurements by CORONAS‐F
V Kurt, K Kudela, B Yushkov… - Advances in Astronomy, 2013 - Wiley Online Library
We analyzed the high‐energy gamma and neutron emissions observed by the SONG
instrument onboard the CORONAS‐F satellite during August 25, 2001, October 28, 2003 …
instrument onboard the CORONAS‐F satellite during August 25, 2001, October 28, 2003 …
Protons acceleration in solar flares: the results of the analysis of gamma-emission and neutrons recorded by the SONG instrument onboard the CORONAS-F satellite
SN Kuznetsov, VG Kurt, BY Yushkov… - The Coronas-F Space …, 2014 - Springer
The SONG instrument onboard CORONAS-F satellite was the only experiment which
observed neutral emissions with energies> 20 MeV from solar flares during the 23rd solar …
observed neutral emissions with energies> 20 MeV from solar flares during the 23rd solar …
Statistical Links between Solar Cosmic Rays, Type-II Radio Emission, and Coronal Mass Ejections
GA Bazilevskaya, YI Logachev, EI Daibog… - Geomagnetism and …, 2021 - Springer
Type-II radio emission often accompanies events in solar cosmic rays and is an indicator of
the propagation of a shock wave in the solar corona. Conversely, the shock wave associated …
the propagation of a shock wave in the solar corona. Conversely, the shock wave associated …
[PDF][PDF] Επεξεργασία και ανάλυση φάσματος ηλιακών ραδιοεκπομπών του ηλιακού ραδιοφασματογράφου ΑΡΤΕΜΙΣ IV
Θ Σμάνης - 2019 - ir.lib.uth.gr
The processing and analysis of the solar spectrum for the detection of radio bursts, is of
increased importance for solar astronomy, as it affects many aspects of human activity (eg …
increased importance for solar astronomy, as it affects many aspects of human activity (eg …
[PDF][PDF] The relativistic solar particle event of 2005 January 20: prompt and delayed particle acceleration
KL Klein, S Masson, C Bouratzis… - arXiv preprint arXiv …, 2014 - academia.edu
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 …