{"id":4621,"date":"2017-06-19T17:10:04","date_gmt":"2017-06-19T17:10:04","guid":{"rendered":"http:\/\/www.astro.gla.ac.uk\/?p=4621"},"modified":"2022-02-03T18:59:00","modified_gmt":"2022-02-03T18:59:00","slug":"nicolina-chrysaphi","status":"publish","type":"post","link":"https:\/\/www.astro.gla.ac.uk\/?p=4621","title":{"rendered":"Nicolina Chrysaphi"},"content":{"rendered":"<p><a href=\"http:\/\/www.astro.gla.ac.uk\/wp-content\/uploads\/chrysaphi.jpg\"><img decoding=\"async\" loading=\"lazy\" class=\"alignright  wp-image-4651\" src=\"http:\/\/www.astro.gla.ac.uk\/wp-content\/uploads\/chrysaphi-233x300.jpg\" alt=\"chrysaphi\" width=\"174\" height=\"221\" \/><\/a><strong>PhD Student<\/strong><\/p>\n<p>I conduct research focused on the observation and analysis of radio emissions from the Sun, under the supervision of <span style=\"color: #0000ff;\"><a style=\"color: #0000ff;\" href=\"https:\/\/www.astro.gla.ac.uk\/?p=168\" target=\"_blank\" rel=\"noopener\">Professor Eduard P. Kontar<\/a><\/span>.\u00a0 I am particularly interested in the physical mechanisms defining the morphological characteristics of Type II radio bursts which are excited by shock waves associated with Coronal Mass Ejections (CMEs).\u00a0 I also study the radio-wave scattering effects in the solar corona to better understand the observed radio emissions.\u00a0 I have utilised data from several instruments including <em>SDO<\/em>\/AIA, <em>SOHO<\/em>\/LASCO, GOES\/XRS, and LOFAR.<\/p>\n<p><strong>Refereed Publications:<\/strong><\/p>\n<ol>\n<li><strong>Chrysaphi, N.<\/strong>, Kontar, E. P., Holman, G. D., and Temmer, M. (2018). <span style=\"color: #0000ff;\"><a style=\"color: #0000ff;\" href=\"http:\/\/adsabs.harvard.edu\/abs\/2018ApJ...868...79C\" target=\"_blank\" rel=\"noopener\">CME-driven Shock and Type II Solar Radio Burst Band Splitting<\/a><\/span>. ApJ, 868, 79. DOI: <span style=\"color: #0000ff;\"><a style=\"color: #0000ff;\" href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/1538-4357\/aae9e5\/meta\" target=\"_blank\" rel=\"noopener\">10.3847\/1538-4357\/aae9e5<\/a><\/span>. [<span style=\"color: #0000ff;\"><a style=\"color: #0000ff;\" href=\"https:\/\/arxiv.org\/abs\/1810.08026\" target=\"_blank\" rel=\"noopener\">arXiv<\/a><\/span>]<\/li>\n<li>Kontar, E. P., Chen, X., <strong>Chrysaphi, N.<\/strong>, Jeffrey, N. L. S., et al. (2019). <span style=\"color: #0000ff;\"><a style=\"color: #0000ff;\" href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2019ApJ...884..122K\/abstract\" target=\"_blank\" rel=\"noopener\">Anisotropic Radio-wave Scattering and the Interpretation of Solar Radio Emission Observations<\/a><\/span>. ApJ, 884, 112. DOI: <span style=\"color: #0000ff;\"><a style=\"color: #0000ff;\" href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/1538-4357\/ab40bb\" target=\"_blank\" rel=\"noopener\">10.3847\/1538-4357\/ab40bb<\/a><\/span>. [<span style=\"color: #0000ff;\"><a style=\"color: #0000ff;\" href=\"https:\/\/arxiv.org\/abs\/1909.00340\" target=\"_blank\" rel=\"noopener\">arXiv<\/a><\/span>]<\/li>\n<li><strong>Chrysaphi, N.<\/strong>, Reid, H. A. S., and Kontar, E. P. (2020). <span style=\"color: #0000ff;\"><a style=\"color: #0000ff;\" href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020ApJ...893..115C\/abstract\" target=\"_blank\" rel=\"noopener\">First Observation of a Type II Solar Radio Burst Transitioning Between a Stationary and Drifting State<\/a><\/span>. ApJ, 893, 115. DOI: <span style=\"color: #0000ff;\"><a style=\"color: #0000ff;\" href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/1538-4357\/ab80c1\" target=\"_blank\" rel=\"noopener\">10.3847\/1538-4357\/ab80c1<\/a><\/span>. [<span style=\"color: #0000ff;\"><a style=\"color: #0000ff;\" href=\"https:\/\/arxiv.org\/abs\/2003.11101\" target=\"_blank\" rel=\"noopener\">arXiv<\/a><\/span>]<\/li>\n<li>Kuznetsov, A. A., <strong>Chrysaphi, N.<\/strong>, Kontar, E. P., and Motorina, G. (2020). <span style=\"color: #0000ff;\"><a style=\"color: #0000ff;\" href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020ApJ...898...94K\/abstract\" target=\"_blank\" rel=\"noopener\">Radio Echo in the Turbulen<span style=\"color: #0000ff;\">t Corona and Simulation<\/span>s of Solar Drift-pair Radio Bursts<\/a><\/span>. ApJ, 898, 94. DOI: <span style=\"color: #0000ff;\"><a style=\"color: #0000ff;\" href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/1538-4357\/aba04a\" target=\"_blank\" rel=\"noopener\">10.3847\/1538-4357\/aba04a<\/a><\/span>. [<span style=\"color: #0000ff;\"><a style=\"color: #0000ff;\" href=\"https:\/\/arxiv.org\/abs\/2007.14648\" target=\"_blank\" rel=\"noopener\">arXiv<\/a><\/span>]<\/li>\n<li>Chen, X., Kontar, E. P., <strong>Chrysaphi, N.<\/strong>, Jeffrey, N. L. S., Gordovskyy, M., Yan, Y., and Tan, B. (2020). <span style=\"color: #0000ff;\"><a style=\"color: #0000ff;\" href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020ApJ...905...43C\/abstract\" target=\"_blank\" rel=\"noopener\">Subsecond Time Evolution of Type III Solar Radio Burst Sources at Fundamental and Harmonic Frequencies<\/a><\/span>. ApJ, 905, 43. DOI:\u00a0<span style=\"color: #0000ff;\"><a style=\"color: #0000ff;\" href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/1538-4357\/abc24e\" target=\"_blank\" rel=\"noopener\">10.3847\/1538-4357\/abc24e<\/a><\/span>. [<span style=\"color: #0000ff;\"><a style=\"color: #0000ff;\" href=\"https:\/\/arxiv.org\/abs\/2010.08782\" target=\"_blank\" rel=\"noopener\">arXiv<\/a><\/span>]<\/li>\n<\/ol>\n<p><strong>Authored open-source code:<\/strong><br \/>\n<span style=\"color: #0000ff;\"><span style=\"color: #000000;\">1.<\/span> <a style=\"color: #0000ff;\" href=\"https:\/\/sohowww.nascom.nasa.gov\/solarsoft\/radio\/lofar\/idl\/rays_new\/scattering_shift.pro\" target=\"_blank\" rel=\"noopener\">scattering_shift.pro<\/a><\/span> &#8211; Added to the SolarSoftWare (SSW) library.<\/p>\n<p><em>Room 604<br \/>\nSchool of Physics and Astronomy<br \/>\nKelvin Building<br \/>\nUniversity of Glasgow<br \/>\nG12 8QQ<br \/>\nScotland<br \/>\n<\/em><br \/>\n<strong>Email<\/strong>:\u00a0n.chrysaphi.1@research.gla.ac.uk<br \/>\n<strong>ORCID:<\/strong> <span style=\"color: #0000ff;\"><a style=\"color: #0000ff;\" href=\"http:\/\/orcid.org\/0000-0002-4389-5540\" target=\"_blank\" rel=\"noopener\">0000-0002-4389-5540<\/a><\/span><\/p>\n<p>Tel: +44 141 330 2960<br \/>\nFax: +44 141 330 8600<\/p>\n","protected":false},"excerpt":{"rendered":"<p>PhD Student I conduct research focused on the observation and analysis of radio emissions from the Sun, under the supervision of Professor Eduard P. Kontar.\u00a0 I am particularly interested in the physical mechanisms defining the morphological characteristics of Type II &hellip;<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":[],"categories":[8,5],"tags":[],"_links":{"self":[{"href":"https:\/\/www.astro.gla.ac.uk\/index.php?rest_route=\/wp\/v2\/posts\/4621"}],"collection":[{"href":"https:\/\/www.astro.gla.ac.uk\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.astro.gla.ac.uk\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.astro.gla.ac.uk\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.astro.gla.ac.uk\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=4621"}],"version-history":[{"count":9,"href":"https:\/\/www.astro.gla.ac.uk\/index.php?rest_route=\/wp\/v2\/posts\/4621\/revisions"}],"predecessor-version":[{"id":5326,"href":"https:\/\/www.astro.gla.ac.uk\/index.php?rest_route=\/wp\/v2\/posts\/4621\/revisions\/5326"}],"wp:attachment":[{"href":"https:\/\/www.astro.gla.ac.uk\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=4621"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.astro.gla.ac.uk\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=4621"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.astro.gla.ac.uk\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=4621"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}