activity
20062022
most citedThe temporal evolution of coronal loops observed by GOES-SXI

36 citations · 67 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2022★ 5 cited

Enthalpy-based modeling of tomographically reconstructed quiet-Sun coronal loops

C. Mac Cormack, M. López Fuentes, C. H. Mandrini +2

The structure of the solar corona is made of magnetic flux tubes or loops. Due to the lack of contrast with their environment, observing and studying coronal loops in the quiet Sun…

astro-ph.SR2020★ 10 cited

Active-Region Tilt Angles from White-Light Images and Magnetograms: The Role of Magnetic Tongues

M. Poisson, P. Démoulin, C. H. Mandrini +1

The presence of elongations in active region (AR) polarities, called magnetic tongues, are mostly visible during their emergence phase. AR tilts have been measured thoroughly using…

astro-ph.SR2019★ 6 cited

Analysis of a long-duration AR throughout five solar rotations: Magnetic properties and ejective events

Francisco A. Iglesias, Hebe Cremades, Luciano A. Merenda +4

Coronal mass ejections (CMEs), which are among the most magnificent solar eruptions, are a major driver of space weather and can thus affect diverse human technologies. Different p…

astro-ph.SR2019★ 10 cited

Two successive partial mini-filament confined ejections

M. Poisson, C. Bustos, M. López Fuentes +2

Active region (AR) NOAA 11476 produced a series of confined plasma ejections, mostly accompanied by flares of X-ray class M, from 08 to 10 May 2012. The structure and evolution of…

astro-ph2006★ 36 cited

The temporal evolution of coronal loops observed by GOES-SXI

M. C. Lopez Fuentes, J. A. Klimchuk, C. H. Mandrini

We study the temporal evolution of coronal loops using data from the Solar X-ray Imager (SXI) on board of GOES-12. This instrument allows us to follow in detail the full lifetime o…