Nonthermal hard X-ray flux saturation in solar flares

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dc.contributor.advisorAlexander, David
dc.creatorDaou, Antoun Georges
dc.date.accessioned2009-06-04T06:30:21Z
dc.date.available2009-06-04T06:30:21Z
dc.date.issued2005
dc.description.abstractWe use the unprecedented spectral and spatial resolution of RHESSI to explore the behavior of electrons and their associated currents in solar flares. Spectral images are used to determine an estimate of the effective surface area for the different independent substructures within each event. The incident electron spectra at those flaring footpoints are derived from the RHESSI photon spectra. We find that, over a wide range of flare X-ray magnitudes, the integrated photon flux above 20 keV asymptotically approaches a limiting value, suggesting a saturation of the photon production in flares. The inferred particle fluxes in the beam, together with this saturation limit, are used to determine the energy loss mechanism dominating the energetic particle transport in solar flares.
dc.format.extent80 p.en_US
dc.format.mimetypeapplication/pdf
dc.identifier.callnoTHESIS PHYS. 2005 DAOU
dc.identifier.citationDaou, Antoun Georges. "Nonthermal hard X-ray flux saturation in solar flares." (2005) Master’s Thesis, Rice University. <a href="https://hdl.handle.net/1911/17847">https://hdl.handle.net/1911/17847</a>.
dc.identifier.urihttps://hdl.handle.net/1911/17847
dc.language.isoeng
dc.rightsCopyright is held by the author, unless otherwise indicated. Permission to reuse, publish, or reproduce the work beyond the bounds of fair use or other exemptions to copyright law must be obtained from the copyright holder.
dc.subjectAstronomy
dc.subjectAstrophysics
dc.titleNonthermal hard X-ray flux saturation in solar flares
dc.typeThesis
dc.type.materialText
thesis.degree.departmentPhysics
thesis.degree.disciplineNatural Sciences
thesis.degree.grantorRice University
thesis.degree.levelMasters
thesis.degree.nameMaster of Science
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