activity
20072018
most citedOrigin of the 30 THz emission detected during the 2012 March 13 solar flare at 17:20 UT

35 citations · 192 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2018★ 10 cited

Physical processes involved in the EUV "Surge" Event of 09 May 2012

Marcelo López Fuentes, Cristina H. Mandrini, Mariano Poisson +4

We study an EUV confined ejection observed on 09 May 2012 in active region (AR) NOAA 11476. For the analysis we use observations in multiple wavelengths (EUV, X-rays, H, and mag…

astro-ph.SR2017★ 21 cited

Moreton and EUV Waves Associated with an X1.0 Flare and CME Ejection

Carlos Francile, Fernando M. López, Hebe Cremades +3

A Moreton wave was detected in active region (AR) 12017 on 29 March 2014 with very high cadence with the Halpha Solar Telescope for Argentina (HASTA) in association with an X1.0 fl…

astro-ph.SR2015★ 6 cited

Comparison of 30 THz impulsive burst time development to microwaves, H-alpha, EUV, and GOES soft X-rays

R. Miteva, P. Kaufmann, D. P. Cabezas +11

The recent discovery of impulsive solar burst emission in the 30 THz band is raising new interpretation challenges. One event associated with a GOES M2 class flare has been observe…

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.SR2015★ 25 cited

Bright 30 THz Impulsive Solar Bursts

P. Kaufmann, S. M. White, R. Marcon +10

Impulsive 30 THz continuum bursts have been recently observed in solar flares, utilizing small telescopes with a unique and relatively simple optical setup concept. The most intens…

astro-ph.SR2012★ 1 cited

12 Years of Stellar Activity Observations in Argentina

Pablo J. D. Mauas, A. Buccino, R. Diaz +6

We present an observational program we started in 1999, to systematically obtain mid-resolution spectra of late-type stars, to study in particular chromospheric activity. In partic…