Impulsive 30THz continuum bursts have been recently observed in solar flares, utilizing small telescopes with a unique and relatively simple optical setup concept. The most intense burst was observed together with a GOES X2 class event on 27 October 2014, also detected at two subterahertz (sub-THz) frequencies, Reuven Ramaty High Energy Solar Spectroscopic Imager X-rays and Solar Dynamics Observatory/Helioseismic and Magnetic Imager and EUV. It exhibits strikingly good correlation in time and in space with white-light flare emission. It is likely that this association may prove to be very common. All three 30THz events recently observed exhibited intense fluxes in the range of 104 solar flux units, considerably larger than those measured fo...
The GOES X28 flare of 4 November 2003 was the largest ever recorded in its class. It produced the fi...
A new solar burst emission spectral component has been found showing sub-THz fluxes increasing with ...
Recent sub-THz and 30 THz observations revealed an unexpected new spectral component, with fluxes in...
FAPESP - FUNDAÇÃO DE AMPARO À PESQUISA DO ESTADO DE SÃO PAULOCNPQ - CONSELHO NACIONAL DE DESENVOLVIM...
The recent discovery of impulsive solar burst emission in the 30 THz band is raising new interpretat...
Ground- and space-based observations of solar flares from radio wavelengths to gamma-rays have produ...
It has been found that solar bursts exhibit one unexpected spectral component with fluxes increasing...
Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Conselho Nacional de Desenvolvimento Ci...
International audienceWe discuss the implications of the first systematic observations of solar flar...
Previous sub-THz studies were derived from single-event observations. We here analyze for the first ...
Solar flare energy manifestations were believed to be the result of the same kind of particle accele...
Context. Since the installation of submillimeter solar radio telescopes, a new spectral burst compo...
The presence of a solar burst spectral component with flux density increasing with frequency in the ...
Itapetinga measurements at 48 GHz with the multibeam technique are used to determine the relative po...
Recent solar flare observations have shown the existence of a spectral component exhibiting fluxes i...
The GOES X28 flare of 4 November 2003 was the largest ever recorded in its class. It produced the fi...
A new solar burst emission spectral component has been found showing sub-THz fluxes increasing with ...
Recent sub-THz and 30 THz observations revealed an unexpected new spectral component, with fluxes in...
FAPESP - FUNDAÇÃO DE AMPARO À PESQUISA DO ESTADO DE SÃO PAULOCNPQ - CONSELHO NACIONAL DE DESENVOLVIM...
The recent discovery of impulsive solar burst emission in the 30 THz band is raising new interpretat...
Ground- and space-based observations of solar flares from radio wavelengths to gamma-rays have produ...
It has been found that solar bursts exhibit one unexpected spectral component with fluxes increasing...
Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Conselho Nacional de Desenvolvimento Ci...
International audienceWe discuss the implications of the first systematic observations of solar flar...
Previous sub-THz studies were derived from single-event observations. We here analyze for the first ...
Solar flare energy manifestations were believed to be the result of the same kind of particle accele...
Context. Since the installation of submillimeter solar radio telescopes, a new spectral burst compo...
The presence of a solar burst spectral component with flux density increasing with frequency in the ...
Itapetinga measurements at 48 GHz with the multibeam technique are used to determine the relative po...
Recent solar flare observations have shown the existence of a spectral component exhibiting fluxes i...
The GOES X28 flare of 4 November 2003 was the largest ever recorded in its class. It produced the fi...
A new solar burst emission spectral component has been found showing sub-THz fluxes increasing with ...
Recent sub-THz and 30 THz observations revealed an unexpected new spectral component, with fluxes in...