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20112026
most citedOrigin of the 30 THz emission detected during the 2012 March 13 solar flare at 17:20 UT

35 citations · 76 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2026

First Very Long Baseline Interferometry Fringe Detection at 690GHz

Ming-Tang Chen, Geoffrey B. Crew, Dan Bintley +42

We report the first very long baseline interferometry (VLBI) experiment conducted in the 690 GHz atmospheric window. On 2024 November 21, observations with the Atacama Large Millim…

astro-ph.SR2024★ 4 cited

Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Solar and stellar observations

Sven Wedemeyer, Miroslav Barta, Roman Brajsa +35

Observations at (sub-)millimeter wavelengths offer a complementary perspective on our Sun and other stars, offering significant insights into both the thermal and magnetic composit…

astro-ph.IM2023

LLAMA Millimeter and Submillimeter Observatory. Update on its Science Opportunities

M. Fernandez-Lopez, P. Benaglia, S. Cichowolski +11

The Large Latin American Millimeter Array (LLAMA for short) is a joint scientific and technological undertaking of Argentina and Brazil whose goal is to install and to operate an o…

astro-ph.SR2015★ 35 cited

Origin of the 30 THz emission detected during the 2012 March 13 solar flare at 17:20 UT

G. Trottet, J. -P. Raulin, A. MacKinnon +6

Solar observations in the infrared domain can bring important clues on the response of the low solar atmosphere to primary energy released during flares. At present the infrared co…

astro-ph.SR2014★ 12 cited

The Relation between the Radial Temperature Profile in the Chromosphere and the Solar Spectrum at Centimeter, Millimeter, Sub-millimeter, and Infrared Wavelengths

Victor De la Luz, Miguel Chavez, Emanuele Bertone +1

Solar observations from millimeter to ultraviolet wavelengths show that there is a temperature minimum between photosphere and chromosphere. Analysis based on semi-empirical models…

astro-ph.SR2011★ 25 cited

Origin of the submillimeter radio emission during the time-extended phase of a solar flare

G. Trottet, J. -P. Raulin, G. Giménez de Castro +5

Solar flares observed in the 200-400 GHz radio domain may exhibit a slowly varying and time-extended component which follows a short (few minutes) impulsive phase and which lasts f…