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View article: Gowers norms for linearly recurrent numeration systems
Gowers norms for linearly recurrent numeration systems Open
Gowers norms have been a key component in the proofs of many breakthrough results in connection to the sum of digits function. Spiegelhofer has used them to show that the Thue-Morse sequence has level of distribution 1 and also that it is …
View article: Formation of Jet-driven Forced Reconnection Region and Associated Plasma Blobs in a Prominence Segment
Formation of Jet-driven Forced Reconnection Region and Associated Plasma Blobs in a Prominence Segment Open
We use data from the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory to study the most likely formation of a forced reconnection region and associated plasma blobs, triggered by jetlike structures in a prominence segme…
View article: Formation of Jet-driven Forced Reconnection Region and Associated Plasma Blobs in a Prominence Segment
Formation of Jet-driven Forced Reconnection Region and Associated Plasma Blobs in a Prominence Segment Open
We use data from the Atmospheric Imaging Assembly (AIA) onboard the Solar Dynamics Observatory (SDO) to study the most likely formation of a forced reconnection region and associated plasma blobs, triggered by jet-like structures in a prom…
View article: Binary-ternary collisions and the last significant digit of $n!$ in base 12
Binary-ternary collisions and the last significant digit of $n!$ in base 12 Open
The third-named author recently proved [Israel J. of Math. 258 (2023), 475--502] that there are infinitely many \textit{collisions} of the base-2 and base-3 sum-of-digits functions. In other words, the equation \[ s_2(n)=s_3(n) \] admits i…
View article: Turbulent plasma flow, its energies, and structures: Velocity vortices, magnetic field cocoons, and plasmoids
Turbulent plasma flow, its energies, and structures: Velocity vortices, magnetic field cocoons, and plasmoids Open
Context. Turbulent flows are believed to be present in the solar corona, especially in connection with solar flares and coronal mass ejections. They are supposed to be very effective processes in energy transportation and can contribute to…
View article: Spectroscopic Diagnostic of the Footpoints of the Cool loops
Spectroscopic Diagnostic of the Footpoints of the Cool loops Open
Statistically, the cool loop's footpoints are diagnosed using Si~{\sc iv} resonance lines observations provided by Interface Region Imaging Spectrograph (IRIS). The intensity and Full Width at Half Maximum (FWHM) of the loop's footpoints i…
View article: Origin of Quasi-periodic Pulsation at the Base of a Kink-unstable Jet
Origin of Quasi-periodic Pulsation at the Base of a Kink-unstable Jet Open
We studied a blowout jet that occurred at the west limb of the Sun on 2014 August 29 using high-resolution imaging/spectroscopic observations provided by the Solar Dynamics Observatory/Atmospheric Imaging Assembly and the Interface Region …
View article: Origin of Quasi-Periodic Pulsation at the Base of Kink Unstable Jet
Origin of Quasi-Periodic Pulsation at the Base of Kink Unstable Jet Open
We study a blowout jet that occurs at the west limb of the Sun on August 29$^{th}$, 2014 using high-resolution imaging/spectroscopic observations provided by SDO/AIA and IRIS. An inverse $γ$-shape flux-rope appears before the jet{--} morph…
View article: Numerical Simulations of Oscillations in Solar Corona Excited by Vortex Shedding
Numerical Simulations of Oscillations in Solar Corona Excited by Vortex Shedding Open
We study transverse oscillations of plasma structures in the solar corona excited by vortex shedding solving the full set of the 3D ideal time-dependent magnetohydrodynamic equations. To present how the creation of vortices and excited osc…
View article: Transverse oscillations of a quiescent solar filament observed at the 304 Å EUV passband
Transverse oscillations of a quiescent solar filament observed at the 304 Å EUV passband Open
Quasi-periodic transverse oscillations of a quiescent solar filament based on the Hα and the 304 Å EUV intensity maps have been studied. Time-distance diagrams of filament intensity variations were produced. The method of the identificatio…
View article: The Prominence Driven Forced Reconnection in the Solar Corona and Associated Plasma Dynamics
The Prominence Driven Forced Reconnection in the Solar Corona and Associated Plasma Dynamics Open
Using the multitemperature observations from SDO/AIA on 2019 December 30, we provide a signature of prominence driven forced magnetic reconnection in the corona and associated plasma dynamics from 09:20 UT to 10:38 UT. A hot prominence seg…
View article: The prominence driven forced reconnection in the solar corona and\n associated plasma dynamics
The prominence driven forced reconnection in the solar corona and\n associated plasma dynamics Open
Using the multi-temperature observations from SDO/AIA on 30th December 2019,\nwe provide a signature of prominence driven forced magnetic reconnection in the\ncorona and associated plasma dynamics during 09:20 UT to 10:38 UT. A hot\npromin…
View article: Transverse oscillations of a double-structured solar filament
Transverse oscillations of a double-structured solar filament Open
Aims. We study the transverse oscillations of a double-structured solar filament. Methods. We modelled the filament numerically via a 2D magnetohydrodynamic (MHD) model, in which we solved a full set of time-dependent MHD equations by mean…
View article: On the rapid forced reconnection in the Sun's corona for its localized heating
On the rapid forced reconnection in the Sun's corona for its localized heating Open
The million-degree hot solar corona maintains its high temperature and compensates for its radiative losses by continuously acquiring an energy flux of $\approx$10$^{3}$ W m$^{-2,}$. Recent studies suggest that energy transport in the sola…
View article: First Evidence of the Frequency Filtering of Magnetoacoustic Waves in the Flaring Star EK Dra
First Evidence of the Frequency Filtering of Magnetoacoustic Waves in the Flaring Star EK Dra Open
Using the data obtained from XMM-Newton, we show the gradual evolution of two periodicities of ~4500 s and ~2200 s in the decay phase of the flare observed in a solar analog EK Dra. The longer period evolves firstly for first 14 ks, while …
View article: On the plasma deposition of vancomycin‐containing nano‐capsules for drug‐delivery applications
On the plasma deposition of vancomycin‐containing nano‐capsules for drug‐delivery applications Open
Aerosol‐assisted atmospheric pressure plasma allows for a one‐step synthesis of vancomycin‐containing nano‐capsules. Morphological and chemical analyses are carried out to estimate how different discharge parameters affect the plasma depos…
View article: Magnetic swirls and associated fast magnetoacoustic kink waves in a solar chromospheric flux tube
Magnetic swirls and associated fast magnetoacoustic kink waves in a solar chromospheric flux tube Open
We perform numerical simulations of impulsively generated magnetic swirls in an isolated flux tube which is rooted in the solar photosphere. These swirls are triggered by an initial pulse in a horizontal component of the velocity. The init…
View article: Quasi-periodic processes in the flare loop generated by sudden temperature enhancements at loop footpoints
Quasi-periodic processes in the flare loop generated by sudden temperature enhancements at loop footpoints Open
\n Aims. During the impulsive flare phase, the plasma at the flare loop footpoints is rapidly heated by particle beams. In the present paper, we study processes that occur after this sudden heating in a two-dimensional magnetic loop.\n Met…
View article: Magnetohydrodynamic Oscillations in the Solar Corona and Earth’s Magnetosphere: Towards Consolidated Understanding
Magnetohydrodynamic Oscillations in the Solar Corona and Earth’s Magnetosphere: Towards Consolidated Understanding Open
View article: Environmental Aspects of Renovations – Case Studies
Environmental Aspects of Renovations – Case Studies Open
In this paper we would like to show the readers two case studies of energy-, environmentally- and cost-efficient renovations of contemporary buildings in Czech Republic that were assessed according to the IEA ECBS Annex 56 methodology - el…
View article: ELECTRIC CURRENT FILAMENTATION AT A NON-POTENTIAL MAGNETIC NULL-POINT DUE TO PRESSURE PERTURBATION
ELECTRIC CURRENT FILAMENTATION AT A NON-POTENTIAL MAGNETIC NULL-POINT DUE TO PRESSURE PERTURBATION Open
An increase of electric current densities due to filamentation is an important process in any flare. We show that the pressure perturbation, followed by an entropy wave, triggers such a filamentation in the non-potential magnetic null-poin…
View article: Spectroscopic observations and modelling of impulsive Alfvén waves along a polar coronal jet
Spectroscopic observations and modelling of impulsive Alfvén waves along a polar coronal jet Open
\n Context. The magnetic reconnection in the solar corona results in impulsively generated Alfvén waves, which drive a polar jet.\n Aims. Using the Hinode/EIS 2′′ spectroscopic observations, we study the intensity, velocity, and full width…