activity
20092022
most citedOn-disk counterparts of type II spicules in the Ca II 854.2 nm and Halpha lines

196 citations · 1.8k across the 25 of their papers we have counts for

collaborators

25 papers

astro-ph.SR2022★ 22 cited

Heating of the solar chromosphere through current dissipation

J. M. da Silva Santos, S. Danilovic, J. Leenaarts +5

The solar chromosphere is heated to temperatures higher than predicted by radiative equilibrium. This excess heating is greater in active regions where the magnetic field is strong…

astro-ph.IM2021★ 9 cited

COCOPLOT: COlor COllapsed PLOTting software : Using color to view 3D data as a 2D image

Malcolm K. Druett, Alexander G. M. Pietrow, Gregal J. M. Vissers +2

Most modern solar observatories deliver data products formatted as 3D spatio-temporal data cubes, that contain additional, higher dimensions with spectral and/or polarimetric infor…

astro-ph.SR2021★ 23 cited

Active region chromospheric magnetic fields

G. J. M. Vissers, S. Danilovic, X. Zhu +5

Context. A proper estimate of the chromospheric magnetic fields is believed to improve modelling of both active region and coronal mass ejection evolution. Aims. We investigate the…

astro-ph.SR2020★ 25 cited

Non-LTE inversions of a confined X2.2 flare: I. Vector magnetic field in the photosphere and chromosphere

G. J. M. Vissers, S. Danilovic, J. de la Cruz Rodriguez +7

Obtaining the magnetic field vector accurately in the solar atmosphere is essential for studying changes in field topology during flares and to reliably model space weather. We tac…

astro-ph.SR2020★ 18 cited

ALMA observations of transient heating in a solar active region

J. M. da Silva Santos, J. de la Cruz Rodríguez, S. M. White +3

We aim to investigate the temperature enhancements and formation heights of impulsive heating phenomena in solar active-regions such as Ellerman bombs (EBs), ultraviolet bursts (UV…

astro-ph.SR2020★ 5 cited

Stratification of canopy magnetic fields in a plage region. Constraints from a spatially-regularized weak-field approximation method

R. Morosin, J. de la Cruz Rodriguez, G. J. M. Vissers +1

The role of magnetic fields in the chromospheric heating problem remains greatly unconstrained. Most theoretical predictions from numerical models rely on a magnetic configuration,…

astro-ph.SR2020★ 22 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.SR2019★ 42 cited

Dissecting bombs and bursts: non-LTE inversions of low-atmosphere reconnection in SST and IRIS observations

G. J. M. Vissers, J. de la Cruz Rodriguez, T. Libbrecht +3

Ellerman bombs and UV bursts are transient brightenings that are ubiquitously observed in the lower atmospheres of active and emerging flux regions. Here we present inversion resul…

astro-ph.SR2019★ 21 cited

Automating Ellerman bomb detection in ultraviolet continua

Gregal J. M. Vissers, Luc H. M. Rouppe van der Voort, Robert J. Rutten

Ellerman bombs are transient brightenings in the wings of H-alpha 6563 Å that pinpoint photospheric sites of magnetic reconnection in solar active regions. Their partial visibility…

astro-ph.SR2018★ 121 cited

Solar ultraviolet bursts

Peter R. Young, Hui Tian, Hardi Peter +16

The term "ultraviolet (UV) burst" is introduced to describe small, intense, transient brightenings in ultraviolet images of solar active regions. We inventorize their properties an…

astro-ph.IM2018★ 86 cited

SSTRED: Data- and metadata-processing pipeline for CHROMIS and CRISP

M. G. Löfdahl, T. Hillberg, J. de la Cruz Rodriguez +5

Context: Data from ground-based, high-resolution solar telescopes can only be used for science with calibrations and processing, which requires detailed knowledge about the instrum…

astro-ph.SR2017★ 91 cited

Intermittent reconnection and plasmoids in UV bursts in the low solar atmosphere

L. Rouppe van der Voort, B. De Pontieu, G. B. Scharmer +9

Magnetic reconnection is thought to drive a wide variety of dynamic phenomena in the solar atmosphere. Yet the detailed physical mechanisms driving reconnection are difficult to di…

astro-ph.SR2016★ 46 cited

Observing the formation of flare-driven coronal rain

E. Scullion, L. Rouppe Van Der Voort, P. Antolin +4

Flare-driven coronal rain can manifest from rapidly cooled plasma condensations near coronal loop-tops in thermally unstable post-flare arcades. We detect 5 phases that characteris…

astro-ph.SR2016★ 66 cited

Reconnection brightenings in the quiet solar photosphere

Luc H. M. Rouppe van der Voort, Robert J. Rutten, Gregal J. M. Vissers

We describe a new quiet-Sun phenomenon which we call "Quiet-Sun Ellerman-like Brightenings" (QSEB). QSEBs are similar to Ellerman bombs (EB) in some respects but differ significant…

astro-ph.SR2015★ 45 cited

Evidence for a Transition Region response to penumbral microjets in sunspots

Gregal J. M. Vissers, Luc H. M. Rouppe van der Voort, Mats Carlsson

Penumbral microjets are short-lived, fine-structured and bright jets that are generally observed in chromospheric imaging of the penumbra of sunspots. Here we investigate their pot…

astro-ph.SR2015★ 129 cited

Ellerman bombs at high resolution III. Simultaneous observations with IRIS and SST

Gregal J. M. Vissers, Luc H. M. Rouppe van der Voort, Robert J. Rutten +2

Ellerman bombs are transient brightenings of the extended wings of the solar Balmer lines in emerging active regions. We describe their properties in the ultraviolet lines sampled…

astro-ph.SR2015★ 28 cited

Ellerman bombs at high resolution. IV. Visibility in Na I and Mg I

R. J. Rutten, L. H. M. Rouppe van der Voort, G. J. M. Vissers

Ellerman bombs are transient brightenings of the wings of the solar Balmer lines that mark reconnection in the photosphere. Ellerman noted in 1917 that he did not observe such brig…

astro-ph.SR2015★ 115 cited

The multi-thermal and multi-stranded nature of coronal rain

P. Antolin, G. Vissers, T. M. D. Pereira +2

In this work, we analyse coordinated observations spanning chromospheric, TR and coronal temperatures at very high resolution which reveal essential characteristics of thermally un…

astro-ph.SR2013★ 103 cited

Ellerman Bombs at high resolution: II. Visibility, triggering and effect on upper atmosphere

Gregal J. M. Vissers, Luc H. M. Rouppe van der Voort, Robert J. Rutten

We use high-resolution imaging spectroscopy with the Swedish 1-m Solar Telescope (SST) to study the transient brightenings of the wings of the Balmer Halpha line in emerging active…

astro-ph.SR2013★ 101 cited

Ellerman bombs: fallacies, fads, usage

Robert J. Rutten, Gregal J. M. Vissers, Luc H. M. Rouppe van der Voort +2

Ellerman bombs are short-lived brightenings of the outer wings of Halpha that occur in active regions with much flux emergence. We point out fads and fallacies in the extensive Ell…

astro-ph.SR2012★ 138 cited

Flocculent flows in the chromospheric canopy of a sunspot

Gregal Vissers, Luc Rouppe van der Voort

High-quality imaging spectroscopy in the Hα line, obtained with the CRisp Imaging SpectroPolarimeter (CRISP) at the Swedish 1-m Solar Telescope (SST) at La Palma and covering a sma…

astro-ph.SR2012

A Sharp Look at Coronal Rain with Hinode/SOT and SST/CRISP

P. Antolin, M. Carlsson, L. Rouppe van der Voort +2

The tropical wisdom that when it is hot and dense we can expect rain might also apply to the Sun. Indeed, observations and numerical simulations have shown that strong heating at f…

astro-ph.SR2011★ 148 cited

Ellerman Bombs at high resolution: I. Morphological evidence for photospheric reconnection

Hiroko Watanabe, Gregal Vissers, Reizaburo Kitai +2

High-resolution imaging-spectroscopy movies of solar active region NOAA 10998 obtained with the CRisp Imaging SpectroPolarimeter (CRISP) at the Swedish 1-m Solar Telescope show ver…

astro-ph.SR2009★ 152 cited

Coronal rain as a marker for coronal heating mechanisms

P. Antolin, K. Shibata

Reported observations in H-alpha, Ca II H and K or or other chromospheric lines of coronal rain trace back to the days of the Skylab mission. Offering a high contrast in intensity…