Results 61 to 70 of about 1,286 (129)
Spatially resolved microwave pulsations of a flare loop [PDF]
A microwave burst with quasi-periodic pulsations was studied with high spatial resolution using observations with the Nobeyama Radioheliograph (NoRH).
Asai +31 more
core +1 more source
A Subsystem Test Bed for Chinese Spectral Radioheliograph [PDF]
AbstractThe Chinese Spectral Radioheliograph is a solar dedicated radio interferometric array that will produce high spatial resolution, high temporal resolution, and high spectral resolution images of the Sun simultaneously in decimetre and centimetre wave range.
An Zhao, Yihua Yan, Wei Wang
openaire +1 more source
Relationship of type III radio bursts with quasi-periodic pulsations in a solar flare [PDF]
We studied a solar flare with pronounced quasi-periodic pulsations detected in the microwave, X-ray, and radio bands. We used correlation, Fourier, and wavelet analyses methods to examine the temporal fine structures and relationships between the time ...
Kashapova, L.K. +3 more
core +2 more sources
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
On the relationship of shock waves to flares and coronal mass ejections
Context: Metric type II bursts are the most direct diagnostic of shock waves in the solar corona. Aims: There are two main competing views about the origin of coronal shocks: that they originate in either blast waves ignited by the pressure pulse of a ...
A. Hillaris +66 more
core +1 more source
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
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
Survey on solar X-ray flares and associated coherent radio emissions
The radio emission during 201 X-ray selected solar flares was surveyed from 100 MHz to 4 GHz with the Phoenix-2 spectrometer of ETH Zurich. The selection includes all RHESSI flares larger than C5.0 jointly observed from launch until June 30, 2003 ...
A. O. Benz +39 more
core +1 more source
Ten Years of the Solar Radiospectrograph ARTEMIS-IV
The Solar Radiospectrograph of the University of Athens (ARTEMIS-IV) is in operation at the Thermopylae Satellite Communication Station since 1996. The observations extend from the base of the Solar Corona (650 MHz) to about 2 Solar Radii (20 MHz) with ...
Alissandrakis, C. E. +12 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

