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Nicolas Scepi
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Nicolas Scepi
Nicolas Scepi
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<div class="contentLayout2"> <div class="columnLayout two-right-sidebar" data-layout="two-right-sidebar"> <div class="cell normal" data-type="normal"> <div class="innerCell"> <h2 style="text-align: center;"><strong>Welcome to my personal page!</strong></h2><p>You can find my <span>CV</span> <a class="confluence-link" href="/download/attachments/43617216/CV2.pdf?version=1&modificationDate=1544691015455&api=v2" data-linked-resource-container-id="43617216" data-linked-resource-container-version="25" data-linked-resource-content-type="application/pdf" data-linked-resource-id="43617478" data-linked-resource-version="1" data-linked-resource-type="attachment" data-linked-resource-default-alias="CV2.pdf" data-base-url="https://ipag-wiki.osug.fr">here</a><strong>.<br /></strong></p><p style="text-align: left;">I am <strong>currently a PhD student at IPAG in Grenoble in the high energy and accretion disk group</strong> (SHERPAS team). I <strong>work from a theoretical and numerical point of view on accretion disks around compact binaries</strong>. My research interest are centered on astrophysical plasmas processes. This includes MHD turbulence, formation of winds/jets, dynamo and all type of plasma instabilities. Also, I am particularly into accretion disks as they have such a rich physics with a strong interplay between plasma physics, hydrodynamics, radiative transfer and thermodynamics.</p><p><br /></p><p style="text-align: left;">During my PhD thesis, I have been focusing mainly on one particular object : the dwarf novae (a compact binary system with an accreting white dwarf; see Figure below) as we have great observational constraints from these objects. However, the accretion processes that we study are quite similar in all types of accretion disks and I would like to extend my research to X-ray binaries, Active Galactic Nuclei and protoplanetary disks.</p><p style="text-align: left;"><br /></p><p><img class="confluence-embedded-image image-center" draggable="false" height="250" src="/download/attachments/43617216/image.png?version=1&modificationDate=1544631830367&api=v2" data-image-src="/download/attachments/43617216/image.png?version=1&modificationDate=1544631830367&api=v2" data-unresolved-comment-count="0" data-linked-resource-id="43617229" data-linked-resource-version="1" data-linked-resource-type="attachment" data-linked-resource-default-alias="image.png" data-base-url="https://ipag-wiki.osug.fr" data-linked-resource-content-type="image/png" data-linked-resource-container-id="43617216" data-linked-resource-container-version="25" title="Nicolas Scepi > Nicolas Scepi > image.png" data-location="Nicolas Scepi > Nicolas Scepi > image.png" data-image-height="524" data-image-width="1313"></p><p><br /></p><p>My day to day work implies <strong>heavy 3D MHD local (and soon global!) simulations of accretion disks with radiative transfer with the PLUTO code</strong>. I also use a lighter 1D+1D (radial and vertical directions decoupled) code solving the temporal evolution of an accretion disk (see video below from Scepi et al 2018c submitted to A&A) and allowing us to compute the light curves in a very short amount of time (see figure below from Scepi et al 2018c submitted to A&A). Additionally, I perform analytical calculations to complement numerical simulations in our understanding of the physics inside accretion disks.</p><p><br /></p><p style="text-align: center;"><img class="editor-inline-macro" height="250" src="/plugins/servlet/view-file-macro/placeholder?type=Multimedia&name=disk.mp4&attachmentId=43617437&version=1&mimeType=video%2Fmp4&height=250" data-macro-name="view-file" data-macro-id="4288e923-f0d9-4790-8232-167781fcbecc" role="button" tabindex="0" aria-haspopup="true" aria-label="view-file macro" data-macro-parameters="height=250|name=disk.mp4" data-macro-schema-version="1"></p><p style="text-align: center;"><img class="editor-inline-macro" height="400" src="/rest/documentConversion/latest/conversion/thumbnail/43617439/1?attachmentId=43617439&version=1&mimeType=application%2Fpdf&height=400&thumbnailStatus=200" data-macro-name="view-file" data-macro-id="0345e4fe-dece-49c1-b776-0a57ccbd28ee" role="button" tabindex="0" aria-haspopup="true" aria-label="view-file macro" data-macro-parameters="height=400|name=dipole_lc-eps-converted-to.pdf" data-macro-schema-version="1"></p><p><br /></p><p class="auto-cursor-target"><br /></p></div> </div> <div class="cell aside" data-type="aside"> <div class="innerCell"> <p><img class="confluence-embedded-image image-right" draggable="false" width="200" src="/download/attachments/43617216/Capture%20d%E2%80%99e%CC%81cran%202018-12-13%20a%CC%80%2009.40.49.png?version=1&modificationDate=1544690472424&api=v2" data-image-src="/download/attachments/43617216/Capture%20d%E2%80%99e%CC%81cran%202018-12-13%20a%CC%80%2009.40.49.png?version=1&modificationDate=1544690472424&api=v2" data-unresolved-comment-count="0" data-linked-resource-id="43617474" data-linked-resource-version="1" data-linked-resource-type="attachment" data-linked-resource-default-alias="Capture d’écran 2018-12-13 à 09.40.49.png" data-base-url="https://ipag-wiki.osug.fr" data-linked-resource-content-type="image/png" data-linked-resource-container-id="43617216" data-linked-resource-container-version="25" title="Nicolas Scepi > Nicolas Scepi > Capture d’écran 2018-12-13 à 09.40.49.png" data-location="Nicolas Scepi > Nicolas Scepi > Capture d’écran 2018-12-13 à 09.40.49.png" data-image-height="679" data-image-width="285"></p></div> </div> </div> </div>
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