Search results for "QC Physics"

showing 6 items of 56 documents

On nature of mathematics. On mathematics and reality Par matemātikas dabu. Par matemātiku un realitāti

2007

Idea that mathematics should be considered as creative order in nature is considered.

T Technology (General)QC PhysicsBD Speculative PhilosophyQH301 BiologyMathematicsofComputing_GENERALQA Mathematics (General)Computer Science::General LiteratureBL Religion
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Contribution of mode coupling and phase-mixing of Alfv\'en waves to coronal heating

2017

This research has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No. 647214) and from the UK Science and Technology Facilities Council. This work used the DiRAC Data Centric system at Durham University, operated by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility (www.dirac.ac.uk. This equipment was funded by a BIS National E-infrastructure capital grant ST/K00042X/1, STFC capital grant ST/K00087X/1, DiRAC Operations grant ST/K003267/1 and Durham University. Context. Phase-mixing of Alfvén waves in the solar corona has been identified as one possible candid…

Work (thermodynamics)Magnetohydrodynamics (MHD)corona [Sun]010504 meteorology & atmospheric sciencesNDASSun: Magnetic fieldsContext (language use)Astrophysics7. Clean energy01 natural sciences0103 physical sciencesThermalQB AstronomyAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsQCQB0105 earth and related environmental sciencesPhysicsSun: Coronabusiness.industrySun: Oscillationsoscillations [Sun]Astronomy and AstrophysicsCoronal loopMechanicsBoundary layerQC Physicsmagnetic fields [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceMode couplingPhysics::Space PhysicsWavesMagnetohydrodynamicsbusinessThermal energy
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The magnetosphere of the close accreting PMS binary V4046 Sgr

2013

V4046 Sagittarii AB is a close short-period classical T Tauri binary. It is a circularised and synchronised system accreting from a circumbinary disk. In 2009 it was observed as part of a coordinated program involving near-simultaneous spectropolarimetric observations with ESPaDOnS at the Canada-France-Hawai'i Telescope and high-resolution X-ray observations with XMM-Newton. Magnetic maps of each star were derived from Zeeman-Doppler imaging. After briefly highlighting the most significant observational findings, we present a preliminary 3D model of the binary magnetosphere constructed from the magnetic maps using a newly developed binary magnetic field extrapolation code. The large-scale f…

accretion young starsQC1-999Astrophysics::High Energy Astrophysical PhenomenaMagnetosphereBinary numberFOS: Physical sciencesAstrophysics01 natural scienceslaw.inventionTelescopeSettore FIS/05 - Astronomia E Astrofisicalaw0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsQCAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Physics010308 nuclear & particles physicsPhysicsMagnetic fieldDipoleStarsT Tauri starQC PhysicsAstrophysics - Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsCircumbinary planet
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Propagating Alfvén waves in open structures with random structuring

2022

Funding: The research leading to these results has received funding from the UK Science and Technology Facilities Council (consolidated grant ST/N000609/1), the European Union Horizon 2020 research and innovation programme (grant agreement No. 647214). IDM received funding from the Research Council of Norway through its Centres of Excellence scheme, project number 262622. We consider the behaviour of Alfvén waves propagating in a medium with random density perturbations. The imposed density perturbations have a broadband spectrum and their characteristic spatial scale may be defined according to the peak in the spectrum. The interaction of the boundary driven Alfvén waves with the medium ge…

atmosphere [Sun]MCCcorona [Sun]MHDoscillations [Sun]NDASAstronomy and AstrophysicsMHD – Sun: atmosphere – Sun: corona – Sun: oscillationsQC PhysicsSpace and Planetary ScienceQB AstronomySettore FIS/06 - Fisica Per Il Sistema Terra E Il Mezzo CircumterrestreQCQB
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Contribution of observed multi frequency spectrum of Alfvén waves to coronal heating

2019

Context. Whilst there are observational indications that transverse magnetohydrodynamic (MHD) waves carry enough energy to maintain the thermal structure of the solar corona, it is not clear whether such energy can be efficiently and effectively converted into heating. Phase-mixing of Alfvén waves is considered a candidate mechanism, as it can develop transverse gradient where magnetic energy can be converted into thermal energy. However, phase-mixing is a process that crucially depends on the amplitude and period of the transverse oscillations, and only recently have we obtained a complete measurement of the power spectrum for transverse oscillations in the corona. Aims. We aim to investig…

atmosphere [Sun]Magnetohydrodynamics (MHD)corona [Sun]T-NDASContext (language use)Astrophysics01 natural sciences03 medical and health sciences0103 physical sciencesQB AstronomyAstrophysics::Solar and Stellar AstrophysicsQA MathematicsSun: oscillationsQASun: magnetic fields010303 astronomy & astrophysicsQCQB030304 developmental biologyPhysics0303 health sciencesMagnetic energySun: coronaoscillations [Sun]Spectral densityAstronomy and AstrophysicsTransverse waveCoronal loopComputational physicsTransverse planeQC PhysicsAmplitudemagnetic fields [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsWavesMagnetohydrodynamicsSun: atmosphereAstronomy & Astrophysics
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Constraining the pass-band of future space-based coronagraphs for observations of solar eruptions in the FeXIV 530.3 nm “green line”

2017

This research has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No 647214) and from the UK Science and Technology Facilities Council. Observations of the solar corona in the FeXIV 530.3 nm “green line” have been very important in the past, and are planned for future coronagraphs on-board forthcoming space missions such as PROBA-3 and Aditya. For these instruments, a very important parameter to be optimized is the spectral width of the band-pass filter to be centred over the “green line”. Focusing on solar eruptions, motions occurring along the line of sight will Doppler shift the line prof…

coronal mass ejections [Sun]corona [Sun]media_common.quotation_subjectAstrophysics01 natural sciences010309 opticssymbols.namesakeSuperposition principle0103 physical sciencesSpectral widthQB AstronomySun: Coronal mass ejections010303 astronomy & astrophysicsQCmedia_commonLine (formation)Spectral purityQBPhysicsLine-of-sightnumerical [Methods]Sun: CoronaAstronomyInstrumentation: CoronagraphsAstronomy and AstrophysicsDASQC Physics13. Climate actionSkySpace and Planetary Sciencecoronagraphs [Instrumentation]Methods: NumericalsymbolsMagnetohydrodynamicsDoppler effectExperimental Astronomy
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