Automatic detection of limb prominences in 304 A EUV images [PDF]
A new algorithm for automatic detection of prominences on the solar limb in 304 A EUV images is presented, and results of its application to SOHO/EIT data discussed.
C. Cortes +22 more
core +2 more sources
Electron acceleration sites in a large-scale coronal structure [PDF]
Radio observations and interplanetary particle measurements have shown that even in the absence of conspicuous violent processes in the low atmosphere (such as Hα flares) electrons are accelerated in the corona, most likely at higher altitudes than ...
Aurass, H. +3 more
core
Features of correlation curves of the Siberian Radioheliograph
Correlation curves of the multi-frequency Siberian Radioheliograph (SRH) provide a sensitive indication and demonstrative representation of monitoring the microwave life of the active Sun.
Uralov Arkadiy +3 more
doaj +1 more source
Space storm measurements of the July 2005 solar extreme events from the low corona to the Earth
The Athens Neutron Monitor Data Processing (ANMODAP) Center recorded an unusual Forbush decrease with a sharp enhancement of cosmic ray intensity right after the main phase of the Forbush decrease on 16 July 2005, followed by a second decrease within ...
A. Hillaris +18 more
core +1 more source
Electron acceleration and transport in the 2023-03-06 solar flare
We investigated in detail the M5.8 class solar flare that occurred on 2023-03-06. This flare was one of the first strong flares observed by the Siberian Radioheliograph in the microwave range and the Advanced Space-based Solar Observatory in the X-ray ...
Alexey Kuznetsov +8 more
doaj +1 more source
Do solar decimetric spikes originate in coronal X-ray sources?
In the standard solar flare scenario, a large number of particles are accelerated in the corona. Nonthermal electrons emit both X-rays and radio waves. Thus, correlated signatures of the acceleration process are predicted at both wavelengths, coinciding ...
A. O. Benz +31 more
core +1 more source
Synoptic study of the corona at meter wavelength [PDF]
The Mark III Nancay Radioheliograph is used to observe the Sun at 169 MHz with a time resolution of 25 East-West and North-South images per second. When the brightness distribution of the Sun is stable during the eight hours of daily observation, a two ...
Alissandrakis, C. E., Lantos, P.
core +1 more source
Multiwavelength Observations of an Eruptive Flare: Evidence for Blast Waves and Break-out
Images of an east-limb flare on 3 November 2010 taken in the 131 \AA\ channel of the Atmospheric Imaging Assembly onboard the Solar Dynamics Observatory provide a convincing example of a long current sheet below an erupting plasmoid, as predicted by the ...
Innes, D. E., Kumar, Pankaj
core +1 more source
Interferometric Imaging, and Beam-Formed Study of a Moving Type-IV Radio Burst with LOFAR. [PDF]
Liu H +8 more
europepmc +1 more source
Observations of Low Frequency Solar Radio Bursts from the Rosse Solar-Terrestrial Observatory
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 study solar radio bursts and the response of the Earth's ionosphere and geomagnetic field. To
A. Kontogeorgos +27 more
core +1 more source

