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Small-scale dynamos: from idealized models to solar and stellar applications
In this article we review small-scale dynamo processes that are responsible for magnetic
field generation on scales comparable to and smaller than the energy carrying scales of …
field generation on scales comparable to and smaller than the energy carrying scales of …
Reconnection-driven energy cascade in magnetohydrodynamic turbulence
Magnetohydrodynamic turbulence regulates the transfer of energy from large to small scales
in many astrophysical systems, including the solar atmosphere. We perform three …
in many astrophysical systems, including the solar atmosphere. We perform three …
Solar jets: SDO and IRIS observations in the perspective of new MHD simulations
B Schmieder - Frontiers in Astronomy and Space Sciences, 2022 - frontiersin.org
Solar jets are observed as collimated plasma beams over a large range of temperatures and
wavelengths. They have been observed in H α and optical lines for more than 50 years and …
wavelengths. They have been observed in H α and optical lines for more than 50 years and …
Transient small-scale brightenings in the quiet solar corona: A model for campfires observed with Solar Orbiter
Context. Recent observations by the Extreme Ultraviolet Imager (EUI) on board Solar Orbiter
have characterized prevalent small-scale transient brightenings in the corona above the …
have characterized prevalent small-scale transient brightenings in the corona above the …
Probing the physics of the solar atmosphere with the Multi-slit Solar Explorer (MUSE). I. Coronal heating
Abstract The Multi-slit Solar Explorer (MUSE) is a proposed mission composed of a multislit
extreme ultraviolet (EUV) spectrograph (in three spectral bands around 171 Å, 284 Å, and …
extreme ultraviolet (EUV) spectrograph (in three spectral bands around 171 Å, 284 Å, and …
Quasi-periodic energy release and jets at the base of solar coronal plumes
Coronal plumes are long, ray-like, open structures that have been considered as possible
sources of the solar wind. Their origin in the largely unipolar coronal holes has long been a …
sources of the solar wind. Their origin in the largely unipolar coronal holes has long been a …
A statistical study of short-period decayless oscillations of coronal loops in an active region
Coronal loop oscillations are common phenomena in the solar corona, which are often
classified as decaying and decayless oscillations. Using the high-resolution observation …
classified as decaying and decayless oscillations. Using the high-resolution observation …
Probing the physics of the solar atmosphere with the multi-slit solar explorer (MUSE). II. flares and eruptions
Current state-of-the-art spectrographs cannot resolve the fundamental spatial
(subarcseconds) and temporal (less than a few tens of seconds) scales of the coronal …
(subarcseconds) and temporal (less than a few tens of seconds) scales of the coronal …
[HTML][HTML] First perihelion of EUI on the Solar Orbiter mission
Context. The Extreme Ultraviolet Imager (EUI) on board Solar Orbiter consists of three
telescopes: the two High Resolution Imagers, in EUV (HRI EUV) and in Lyman-α (HRI Lya) …
telescopes: the two High Resolution Imagers, in EUV (HRI EUV) and in Lyman-α (HRI Lya) …
Solar X-ray and EUV imager on board the FY-3E satellite
B Chen, XX Zhang, LP He, KF Song, SJ Liu… - Light: Science & …, 2022 - nature.com
The solar X-ray and Extreme Ultraviolet Imager (X-EUVI), developed by the Changchun
Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences (CIOMP), is …
Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences (CIOMP), is …