activity
20052022
most citedThe Magnetic Structure of Coronal Loops Observed by TRACE

88 citations · 323 across the 8 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2022

Scaling Laws of Quiet-Sun Coronal Loops

C. Mac Cormack, M. López Fuentes, C. H. Mandrini +3

We study a series of relations between physical parameters in coronal loops of the quiet Sun reconstructed by combining tomographic techniques and modeling of the coronal magnetic…

astro-ph.HE2022★ 53 cited

The Optical Two and Three-Dimensional Fundamental Plane Correlations for Nearly 180 Gamma-Ray Burst Afterglows with Swift/UVOT, RATIR, and the SUBARU Telescope

Maria Giovanna Dainotti, Sam Young, L. Li +21

Gamma-ray bursts (GRBs) are fascinating events due to their panchromatic nature. We study optical plateaus in GRB afterglows via an extended search into archival data. We comprehen…

astro-ph.SR2019★ 8 cited

Correcting the effect of magnetic tongues on the tilt angle of bipolar active regions

M. Poisson, M. C. López Fuentes, C. H. Mandrini +2

The magnetic polarities of bipolar active regions (ARs) exhibit elongations in line-of-sight magnetograms during their emergence. These elongations are referred to as magnetic tong…

astro-ph.SR2016★ 16 cited

A nanoflare based cellular automaton model and the observed properties of the coronal plasma

Marcelo López Fuentes, James A. Klimchuk

We use the cellular automaton model described in López Fuentes \& Klimchuk (2015, ApJ, 799, 128) to study the evolution of coronal loop plasmas. The model, based on the idea of a c…

astro-ph2007★ 35 cited

Are constant loop widths an artifact of the background and the spatial resolution?

M. C. Lopez Fuentes, P. Demoulin, J. A. Klimchuk

We study the effect of the coronal background in the determination of the diameter of EUV loops, and we analyze the suitability of the procedure followed in a previous paper (López…

astro-ph2005★ 88 cited

The Magnetic Structure of Coronal Loops Observed by TRACE

M. C. Lopez Fuentes, J. A. Klimchuk, P. Demoulin

Previous studies have found that coronal loops have a nearly uniform thickness, which seems to disagree with the characteristic expansion of active region magnetic fields. This is…