activity
20162025
most citedLong-Period Intensity Pulsations in Coronal Loops Explained by Thermal Non-Equilibrium Cycles

58 citations · 66 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2025

Determining the magnetic field of active region plages using the whole CLASP2/2.1 spectral window

David Afonso Delgado, Tanausú del Pino Alemán, Javier Trujillo Bueno +16

The Chromospheric LAyer SpectroPolarimeter missions, CLASP2 and CLASP2.1, demonstrated that the near-UV spectral region between 279.30 and 280.68 nm is suitable for studying the ma…

astro-ph.SR2023★ 8 cited

Evolution of dynamic fibrils from the cooler chromosphere to the hotter corona

Sudip Mandal, Hardi Peter, Lakshmi Pradeep Chitta +17

Dynamic fibrils (DFs) are commonly observed chromospheric features in solar active regions. Recent observations from the Extreme Ultraviolet Imager (EUI) aboard the Solar Orbiter h…

astro-ph.SR2017

Discovery of Scattering Polarization in the Hydrogen Lyman- Line of the Solar Disk Radiation

R. Kano, J. Trujillo Bueno, A. Winebarger +25

There is a thin transition region (TR) in the solar atmosphere where the temperature rises from 10,000 K in the chromosphere to millions of degrees in the corona. Little is known a…

astro-ph.SR2017★ 58 cited

Long-Period Intensity Pulsations in Coronal Loops Explained by Thermal Non-Equilibrium Cycles

Clara Froment, Frédéric Auchère, Guillaume Aulanier +4

In solar coronal loops, thermal non-equilibrium (TNE) is a phenomenon that can occur when the heating is both highly-stratified and quasi-constant. Unambiguous observational identi…

astro-ph.SR2016

Thermal non-equilibriuem revealed by periodic pulses of random amplitudes in solar coronal loops

F. Auchère, C. Froment, K. Bocchialini +2

We recently detected variations in extreme ultraviolet intensity in coronal loops repeating with periods of several hours. Models of loops including stratified and quasi-steady hea…