Search results for "PLASMA"

showing 10 items of 4043 documents

Spatial transcriptome of a germinal center plasmablastic burst hints at MYD88/CD79B mutants-enriched diffuse large B-cell lymphomas

2022

The GC reaction results in the selection of B cells acquiring effector Ig secreting ability by progressing toward plasmablastic differentiation. This transition is associated with exclusion from the GC microenvironment. The aberrant expansion of plasmablastic elements within the GC fringes configures an atypical condition, the biological characteristics of which have not been defined yet. We investigated the in situ immunophenotypical and transcriptional characteristics of a nonclonal germinotropic expansion of plasmablastic elements (GEx) occurring in the tonsil of a young patient. Compared to neighboring GC and perifollicular regions, the GEx showed a distinctive signature featuring key r…

Plasma CellsImmunologyGerminal centerDiffuse large B-cell lymphomaDigital spatial profilingSettore MED/08 - Anatomia PatologicaPlasmablastDiffuse large B-cell lymphoma; Digital spatial profiling; Germinal center; Plasmablastdigital spatial profiling; germinal center; plasmablast; diffuse large b-cell lymphomaMyeloid Differentiation Factor 88Tumor MicroenvironmentHumansSettore MED/05 - Patologia ClinicaImmunology and AllergyLymphoma Large B-Cell DiffuseTranscriptomeCD79 AntigensDiffuse large B-cell lymphoma ⋅ Digital spatial profiling ⋅ Germinal center ⋅ Plasmablast
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Influencia del movimiento de vórtices de plasma en concentraciones magnéticas finas en la fotósfera solar

2016

High-resolution observations from ground-based (Solar Swedish Telescope) and space-borne (Hinode) solar telescopes acquired data with various filters, obtaining images of a quiet Sun region populated with small-scale magnetic elements. The region is also characterized by the presence of photospheric swirl convective plasma structures. This work abridges the results of different analysis applied over time series of images to follow the evolution of magnetic features aiming to establish the influence of the plasma vortices on their motions. Observaciones solares en alta resolución desde telescopios en tierra (SST) y en el espacio (Hinode) registraron datos con diferentes filtros, obteniendo i…

Plasma FotosféricoMagnetic FieldFísica SolarSolar PhysicsCampo MagnéticoPhotospheric Plasma
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The role of rf-scattering in high-energy electron losses from minimum-B ECR ion source

2019

The measurement of the axially lost electron energy distribution escaping from a minimum-B electron cyclotron resonance ion source in the range of 4-800 keV is reported. The experiments have revealed the existence of a hump at 150-300 keV energy, containing up to 15% of the lost electrons and carrying up to 30% of the measured energy losses. The mean energy of the hump is independent of the microwave power, frequency and neutral gas pressure but increases with the magnetic field strength, most importantly with the value of the minimum-B field. Experiments in pulsed operation mode have indicated the presence of the hump only when microwave power is applied, confirming that the origin of the …

Plasma Physics (physics.plasm-ph)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesPhysics - Plasma Physics
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Nanoscale subsurface dynamics of solids upon high-intensity laser irradiation observed by femtosecond grazing-incidence x-ray scattering

2020

Observing ultrafast laser-induced structural changes in nanoscale systems is essential for understanding the dynamics of intense light-matter interactions. For laser intensities on the order of $10^{14} \, \rm W/cm^2$, highly-collisional plasmas are generated at and below the surface. Subsequent transport processes such as heat conduction, electron-ion thermalization, surface ablation and resolidification occur at picosecond and nanosecond time scales. Imaging methods, e.g. using x-ray free-electron lasers (XFEL), were hitherto unable to measure the depth-resolved subsurface dynamics of laser-solid interactions with appropriate temporal and spatial resolution. Here we demonstrate picosecond…

Plasma Physics (physics.plasm-ph)Condensed Matter - Mesoscale and Nanoscale PhysicsMesoscale and Nanoscale Physics (cond-mat.mes-hall)FOS: Physical sciencesPhysics - Plasma Physics
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Method for estimating charge breeder ECR ion source plasma parameters with short pulse 1+ injection

2021

A new method for determining plasma parameters from beam current transients resulting from short pulse 1+ injection into a Charge Breeder Electron Cyclotron Resonance Ion Source (CB-ECRIS) has been developed. The proposed method relies on few assumptions, and yields the ionisation times $1/n_e\left\langle\sigma v\right\rangle^{\text{inz}}_{q\to q+1}$, charge exchange times $1/n_0\left\langle\sigma v\right\rangle^{\text{cx}}_{q\to q-1}$, the ion confinement times $\tau^q$, as well as the plasma energy contents $n_e\left\langle E_e\right\rangle$ and the plasma triple products $n_e \left\langle E_e\right\rangle \tau^q$. The method is based on fitting the current balance equation on the extract…

Plasma Physics (physics.plasm-ph)FOS: Physical sciencesPhysics - Plasma Physics[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]
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Connecting Solar Orbiter remote-sensing observations and Parker Solar Probe in situ measurements with a numerical MHD reconstruction of the Parker sp…

2022

As a key feature, NASA's Parker Solar Probe (PSP) and ESA-NASA's Solar Orbiter (SO) missions cooperate to trace solar wind and transients from their sources on the Sun to the inner interplanetary space. The goal of this work is to accurately reconstruct the interplanetary Parker spiral and the connection between coronal features observed remotely by the Metis coronagraph on-board SO and those detected in situ by PSP at the time of the first PSP-SO quadrature of January 2021. We use the Reverse In-situ and MHD Approach (RIMAP), a hybrid analytical-numerical method performing data-driven reconstructions of the Parker spiral. RIMAP solves the MHD equations on the equatorial plane with the PLUT…

Plasma Physics (physics.plasm-ph)Settore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsPhysics - Space PhysicsSpace and Planetary ScienceFOS: Physical sciencesAstronomy and Astrophysicsmagnetohydrodynamics (MHD) – methods: numerical – solar wind – Sun: heliosphere – Sun: coronamagnetohydrodynamics(MHD)methods:numericalsolar windSun:heliosphereSun:coronaPhysics - Plasma PhysicsSolar and Stellar Astrophysics (astro-ph.SR)Space Physics (physics.space-ph)
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Particle energization in colliding subcritical collisionless shocks investigated in the laboratory

2022

Context. Colliding collisionless shocks appear across a broad variety of astrophysical phenomena and are thought to be possible sources of particle acceleration in the Universe. Aims. The main goal of our experimental and computational work is to understand the effect of the interpenetration between two subcritical collisionless shocks on particle energization. Methods. To investigate the detailed dynamics of this phenomenon, we performed a dedicated laboratory experiment. We generated two counter-streaming subcritical collisionless magnetized shocks by irradiating two Teflon (C2F4) targets with 100 J, 1 ns laser beams on the LULI2000 laser facility. The interaction region between the plasm…

Plasma Physics (physics.plasm-ph)Settore FIS/05 - Astronomia E Astrofisica[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU]Sciences of the Universe [physics]Space and Planetary ScienceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and Astrophysicsshock wavesinterplanetary mediumPhysics - Plasma Physicsacceleration of particles
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Investigating particle acceleration dynamics in interpenetrating magnetized collisionless super-critical shocks

2023

Colliding collisionless shocks appear in a great variety of astrophysical phenomena and are thought to be possible sources of particle acceleration in the Universe. We have previously investigated particle acceleration induced by single super-critical shocks (whose magnetosonic Mach number is higher than the critical value of 2.7) (Yao et al., Nat. Phys., vol. 17, issue 10, 2021, pp. 1177–1182; Yao et al., Matter Radiat. Extrem., vol. 7, issue 1, 2022, 014402), as well as the collision of two sub-critical shocks (Fazzini et al., Astron. Astrophys., vol. 665, 2022, A87). Here, we propose to make measurements of accelerated particles from interpenetrating super-critical shocks to observe the …

Plasma Physics (physics.plasm-ph)Settore FIS/05 - Astronomia E Astrofisicaplasma simulationFOS: Physical sciencesCondensed Matter Physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]plasma nonlinear phenomenaPhysics - Plasma Physics[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]
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Importance and Unpredictability of Self-organization Processes in Fusion Burning Plasmas

Self-organization processes are considered to have an important role in well confined plasmas produced by present day experiments where the heating source is externally applied. The observation of ``Profile Consistency'' [1] is viewed as a manifestation of the presence of these processes. In the case of fusion burning plasmas close to self-sustainment (ignition) most of the heating due to fusion products is strongly dependent on the evolution of both the plasma temperature and density profiles. Therefore, self-organization is expected to be of considerably greater importance than in the case of non-reacting plasmas. This fact involves a significant degree of unpredictability on the outcome …

Plasma Physics fusionSettore MAT/07 - Fisica Matematica
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Relationship between plasma endothelin-1 and aortic stiffness in hypertensive patients with chronic kidney disease

2012

Plasma endothelin aortic stiffnes chronic kidney disease arterial hypertension
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