Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Solar observations at sub-THz frequencies detected a new flare spectral component peaking in the THz range, simultaneously with the well known microwaves component, bringing challenging constraints for interpretation. Higher THz frequencies observations are needed to understand the nature of the mechanisms occurring in flares. A THz photometer system was developed to observe outside the terrestrial atmosphere on stratospheric balloons or satellites, or at exceptionally transparent ground stations. The telescope was designed to observe the whole solar disk detecting small relative changes in input temperature cause...
International audienceWe discuss the implications of the first systematic observations of solar flar...
FAPESP - FUNDAÇÃO DE AMPARO À PESQUISA DO ESTADO DE SÃO PAULOCNPQ - CONSELHO NACIONAL DE DESENVOLVIM...
It has been found that solar bursts exhibit one unexpected spectral component with fluxes increasing...
A new solar flare spectral component has been found with intensities increasing for larger sub-THz f...
FAPESP - FUNDAÇÃO DE AMPARO À PESQUISA DO ESTADO DE SÃO PAULOCNPQ - CONSELHO NACIONAL DE DESENVOLVIM...
O telescópio solar submilimétrico operando nas freqüências de 212 e 405 GHz detectou uma nova compon...
Recent sub-THz and 30 THz observations revealed an unexpected new spectral component, with fluxes in...
A new solar burst emission spectral component has been found showing sub-THz fluxes increasing with ...
Recent solar flare observations have shown the existence of a spectral component exhibiting fluxes i...
The almost unexplored frequency window from submillimeter to mid-infrared (mid-IR) may bring new clu...
The knowledge of THz continuum spectra is essential to investigate the emission mechanisms by high e...
THz continuum spectral photometry has new and unique applications in different civil and military ar...
Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Conselho Nacional de Desenvolvimento Ci...
Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Conselho Nacional de Desenvolvimento Ci...
The presence of a solar burst spectral component with flux density increasing with frequency in the ...
International audienceWe discuss the implications of the first systematic observations of solar flar...
FAPESP - FUNDAÇÃO DE AMPARO À PESQUISA DO ESTADO DE SÃO PAULOCNPQ - CONSELHO NACIONAL DE DESENVOLVIM...
It has been found that solar bursts exhibit one unexpected spectral component with fluxes increasing...
A new solar flare spectral component has been found with intensities increasing for larger sub-THz f...
FAPESP - FUNDAÇÃO DE AMPARO À PESQUISA DO ESTADO DE SÃO PAULOCNPQ - CONSELHO NACIONAL DE DESENVOLVIM...
O telescópio solar submilimétrico operando nas freqüências de 212 e 405 GHz detectou uma nova compon...
Recent sub-THz and 30 THz observations revealed an unexpected new spectral component, with fluxes in...
A new solar burst emission spectral component has been found showing sub-THz fluxes increasing with ...
Recent solar flare observations have shown the existence of a spectral component exhibiting fluxes i...
The almost unexplored frequency window from submillimeter to mid-infrared (mid-IR) may bring new clu...
The knowledge of THz continuum spectra is essential to investigate the emission mechanisms by high e...
THz continuum spectral photometry has new and unique applications in different civil and military ar...
Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Conselho Nacional de Desenvolvimento Ci...
Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Conselho Nacional de Desenvolvimento Ci...
The presence of a solar burst spectral component with flux density increasing with frequency in the ...
International audienceWe discuss the implications of the first systematic observations of solar flar...
FAPESP - FUNDAÇÃO DE AMPARO À PESQUISA DO ESTADO DE SÃO PAULOCNPQ - CONSELHO NACIONAL DE DESENVOLVIM...
It has been found that solar bursts exhibit one unexpected spectral component with fluxes increasing...