Search results for " Fisica solare"

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Post-flare evolution of AR 10923 with Hinode/XRT

2010

Flares are dynamic events which involve rapid changes in coronal magnetic topology end energy release. Even if they may be localized phenomena, the magnetic disturbance at their origin may propagate and be effective in a larger part of the active region. We investigate the temporal evolution of a flaring active region with respect to the loops morphology, the temperature, and emission measure distributions. We consider $Hinode/XRT$ data of a the 2006 November 12th C1.1 flare. We inspect the evolution of the morphology of the flaring region also with the aid of TRACE data. XRT filter ratios are used to derive temperature and emission measure maps and evolution. The analyzed flare includes se…

PhysicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsMeasure (mathematics)law.inventionSettore FIS/05 - Astronomia E AstrofisicaMagnetic disturbanceastrofisica Fisica solare Sun: activity Sun: flares Sun: corona Sun: X-rays gamma raysAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencelawThermalPhysics::Space PhysicsAstrophysics::Solar and Stellar AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Flare
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On the importance of background subtraction in the analysis of coronal loops observed with TRACE

2010

In the framework of TRACE coronal observations, we compare the analysis and diagnostics of a loop after subtracting the background with two different and independent methods. The dataset includes sequences of images in the 171 A, 195 A filter bands of TRACE. One background subtraction method consists in taking as background values those obtained from interpolation between concentric strips around the analyzed loop. The other method is a pixel-to-pixel subtraction of the final image when the loop had completely faded out, already used by Reale & Ciaravella 2006. We compare the emission distributions along the loop obtained with the two methods and find that they are considerably differen…

PhysicsBackground subtractionTrace (linear algebra)Subtractionastrofisica Fisica solare Sun: corona Sun: X-rays gamma rays method: data analysisFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsSTRIPSCoronal loopFilter (signal processing)law.inventionComputational physicsLoop (topology)Settore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencelawSolar and Stellar Astrophysics (astro-ph.SR)Interpolation
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