activity
20062023
most citedTwisting solar coronal jet launched at the boundary of an active region

107 citations · 286 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2023★ 3 cited

Exploring magnetic field properties at the boundary of solar pores: A comparative study based on SDO-HMI observations

J. I. Campos Rozo, S. Vargas Domínguez, D. Utz +2

The Sun's magnetic fields play an important role in various solar phenomena. Solar pores are regions of intensified magnetic field strength compared to the surrounding photospheric…

physics.plasm-ph2022★ 10 cited

Energy transport during 3D small-scale reconnection driven by anisotropic plasma turbulence

Jeffersson A. Agudelo Rueda, Daniel Verscharen, Robert T. Wicks +6

Energy dissipation in collisionless plasmas is a longstanding fundamental physics problem. Although it is well known that magnetic reconnection and turbulence are coupled and trans…

astro-ph.SR2016★ 16 cited

Relationship between chromospheric evaporation and magnetic field topology in M-class solar flare

V. M. Sadykov, A. G. Kosovichev, I. N. Sharykin +2

Chromospheric evaporation is observed as Doppler blueshift during solar flares. It plays one of key roles in dynamics and energetics of solar flares, however, its mechanism is stil…

astro-ph.SR2014★ 44 cited

Properties of chromospheric evaporation and plasma dynamics of a solar flare from IRIS observations

Viacheslav M. Sadykov, Santiago Vargas Dominguez, Alexander G. Kosovichev +3

Dynamics of hot chromospheric plasma of solar flares is a key to understanding of mechanisms of flare energy release and particle acceleration. A moderate M1.0 class flare of 12 Ju…

astro-ph.SR2013★ 107 cited

Twisting solar coronal jet launched at the boundary of an active region

B. Schmieder, Y. Guo, F. Moreno-Insertis +7

A broad jet was observed in a weak magnetic field area at the edge of active region NOAA 11106. The peculiar shape and magnetic environment of the broad jet raised the question of…

astro-ph.SR2012★ 12 cited

Magnetic topology of a naked sunspot: Is it really naked?

A. Sainz Dalda, S. Vargas Dominguez, T. D. Tarbell

The high spatial, temporal and spectral resolution achieved by Hinode instruments give much better understanding of the behavior of some elusive solar features, such as pores and n…

astro-ph.IM2011★ 31 cited

LEMUR: Large European Module for solar Ultraviolet Research. European contribution to JAXA's Solar-C mission

Luca Teriaca, Vincenzo Andretta, Frédéric Auchère +39

Understanding the solar outer atmosphere requires concerted, simultaneous solar observations from the visible to the vacuum ultraviolet (VUV) and soft X-rays, at high spatial resol…

astro-ph.SR2011★ 29 cited

Spatial distribution and statistical properties of small-scale convective vortex-like motions in a quiet Sun region

S. Vargas Dominguez, J. Palacios, L. Balmaceda +2

High-resolution observations of a quiet Sun internetwork region taken with the Solar 1-m Swedish Telescope in La Palma are analyzed. We determine the location of small-scale vortex…

astro-ph.SR2010★ 31 cited

Characterization of horizontal flows around solar pores from high-resolution time series of images

S. Vargas Dominguez, A. de Vicente, J. A. Bonet +1

Though there is increasing evidence linking the moat flow and the Evershed flow along the penumbral filaments, there is not a clear consensus regarding the existence of a moat flow…

astro-ph.SR2009★ 2 cited

Study of horizontal flows in solar active regions based on high-resolution image reconstruction techniques

S. Vargas Dominguez

This thesis can be framed in a more general concept designated as "High resolution in solar physics". The first part of the thesis is dedicated to the topic of high-resolution obse…

astro-ph2006★ 1 cited

Simulation and analysis of VIM measurements: feedback on design parameters

D. Orozco Suarez, L. R. Bellot Rubio, S. Vargas Dominguez +3

The Visible-light Imager and Magnetograph (VIM) proposed for the ESA Solar Orbiter mission will observe a photospheric spectral line at high spatial resolution. Here we simulate an…