activity
20172020
most citedSwitchbacks in the near-Sun magnetic field: long memory and impact on the turbulence cascade

221 citations · 420 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR202022 cited

High-resolution observations of the solar photosphere, chromosphere and transition region. A database of coordinated IRIS and SST observations

L. H. M. Rouppe van der Voort, B. De Pontieu, M. Carlsson +30

NASA's Interface Region Imaging Spectrograph (IRIS) provides high resolution observations of the solar atmosphere through UV spectroscopy and imaging. Since the launch of IRIS in J…

astro-ph.SR201949 cited

First direct observation of a torsional Alfvén oscillation at coronal heights

P. Kohutova, E. Verwichte, C. Froment

Torsional Alfvén waves are promising candidates for transport of energy across different layers of the solar atmosphere and have been theoretically predicted for decades. Previous…

astro-ph.SR2019221 cited

Switchbacks in the near-Sun magnetic field: long memory and impact on the turbulence cascade

Thierry Dudok de Wit, Vladimir V. Krasnoselskikh, Stuart D. Bale +14

One of the most striking observations made by Parker Solar Probe during its first solar encounter is the omnipresence of rapid polarity reversals in a magnetic field that is otherw…

astro-ph.SR201912 cited

On the spectroscopic detection of periodic plasma flows in loops undergoing thermal non-equilibrium

Gabriel Pelouze, Frédéric Auchère, Karine Bocchialini +3

Context: Long-period intensity pulsations were recently detected in the EUV emission of coronal loops, and have been attributed to cycles of plasma evaporation and condensation dri…

astro-ph.SR201938 cited

Multi-scale observations of thermal non-equilibrium cycles in coronal loops

C. Froment, P. Antolin, V. M. J. Henriques +2

Thermal non-equilibrium (TNE) is a phenomenon that can occur in solar coronal loops when the heating is quasi-constant and highly-stratified. Under such heating conditions, coronal…

astro-ph.SR201920 cited

Formation of coronal rain triggered by impulsive heating associated with magnetic reconnection

P. Kohutova, E. Verwichte, C. Froment

Coronal rain consists of cool plasma condensations formed in coronal loops as a result of thermal instability. The standard models of coronal rain formation assume that the heating…