{"id":41,"date":"2019-09-13T13:59:49","date_gmt":"2019-09-13T11:59:49","guid":{"rendered":"http:\/\/spreadfast.astro.bas.bg\/?page_id=41"},"modified":"2019-09-13T13:59:49","modified_gmt":"2019-09-13T11:59:49","slug":"psi-models","status":"publish","type":"page","link":"https:\/\/spreadfast.astro.bas.bg\/index.php\/about\/psi-models\/","title":{"rendered":"PSI MODELS"},"content":{"rendered":"<p align=\"JUSTIFY\"><span style=\"color: #000000;\"><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">For the events, which do not lie close to the limb, we will gather the necessary coronal plasma parameters from the synoptic MHD model<\/span><\/span><\/span><\/span><a class=\"sdfootnoteanc\" href=\"#sdfootnote1sym\" name=\"sdfootnote1anc\"><sup>1<\/sup><\/a><span style=\"color: #000000;\"><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\"> of Predictive Sciences, Inc. (PSI). Their MHD Around a Sphere (MAS) model has been extensively validated<\/span><\/span><\/span><\/span><a class=\"sdfootnoteanc\" href=\"#sdfootnote2sym\" name=\"sdfootnote2anc\"><sup>2<\/sup><\/a><span style=\"color: #000000;\"><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">, and its results are freely available for download (in Hierarchical Data Format), for both the coronal and heliospheric domains<\/span><\/span><\/span><\/span><a class=\"sdfootnoteanc\" href=\"#sdfootnote3sym\" name=\"sdfootnote3anc\"><sup>3<\/sup><\/a><span style=\"color: #000000;\"><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">. Figure 1F shows as an example an equatorial cut of radial velocity out to 30 R<\/span><\/span><\/span><\/span><span style=\"color: #000000;\"><sub><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\">\u0298<\/span><\/span><\/sub><\/span><span style=\"color: #000000;\"><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">, for a particular Carrington rotation<\/span><\/span><\/span><\/span><span style=\"color: #000000;\"><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\">. Similar 3D maps of heliospheric plasma model properties are also readily available, extending beyond 2 AU. We will develop an interface for reading and interpolating the coronal PSI maps in Work Package 2. An interface for the heliospheric maps is already available in EPREM.<\/span><\/span><\/span><\/p>\n<div id=\"sdfootnote1\">\n<p lang=\"it-IT\"><a class=\"sdfootnotesym\" href=\"#sdfootnote1anc\" name=\"sdfootnote1sym\">1<\/a><sup><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\">\u0002<\/span><\/span><\/sup> <span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">Lionello<\/span><\/span><\/span><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">, <\/span><\/span><\/span><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">R<\/span><\/span><\/span><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">. <\/span><\/span><\/span><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">et<\/span><\/span><\/span> <span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">al<\/span><\/span><\/span><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">., 2009, <\/span><\/span><\/span><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">ApJ<\/span><\/span><\/span><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">, <\/span><\/span><\/span><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">https<\/span><\/span><\/span><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">:\/\/<\/span><\/span><\/span><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">doi<\/span><\/span><\/span><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">.<\/span><\/span><\/span><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">org<\/span><\/span><\/span><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">\/10.1088\/0004-637<\/span><\/span><\/span><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">X<\/span><\/span><\/span><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">\/690\/1\/902<\/span><\/span><\/span><\/p>\n<\/div>\n<div id=\"sdfootnote2\">\n<p><a class=\"sdfootnotesym\" href=\"#sdfootnote2anc\" name=\"sdfootnote2sym\">2<\/a><sup><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\">\u0002<\/span><\/span><\/sup><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"> Riley, P. et al., 2011, SolPhys, <\/span><\/span><span style=\"color: #333333;\"><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">https<\/span><\/span><\/span><\/span><span style=\"color: #333333;\"><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">:\/\/<\/span><\/span><\/span><\/span><span style=\"color: #333333;\"><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">doi<\/span><\/span><\/span><\/span><span style=\"color: #333333;\"><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">.<\/span><\/span><\/span><\/span><span style=\"color: #333333;\"><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">org<\/span><\/span><\/span><\/span><span style=\"color: #333333;\"><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">\/10.1007\/<\/span><\/span><\/span><\/span><span style=\"color: #333333;\"><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">s<\/span><\/span><\/span><\/span><span style=\"color: #333333;\"><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">11207-010-9698-<\/span><\/span><\/span><\/span><span style=\"color: #333333;\"><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"><span lang=\"en-US\">x<\/span><\/span><\/span><\/span><\/p>\n<\/div>\n<div id=\"sdfootnote3\">\n<p lang=\"it-IT\"><a class=\"sdfootnotesym\" href=\"#sdfootnote3anc\" name=\"sdfootnote3sym\">3<\/a><sup><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\">\u0002<\/span><\/span><\/sup><span style=\"font-family: Arial, serif;\"><span style=\"font-size: small;\"> http:\/\/www.predsci.com\/mhdweb\/<\/span><\/span><\/p>\n<\/div>\n","protected":false},"excerpt":{"rendered":"<p>For the events, which do not lie close to the limb, we will gather the necessary coronal plasma parameters from the synoptic MHD model1 of Predictive Sciences, Inc. (PSI). Their MHD Around a Sphere (MAS) model has been extensively validated2, and its results are freely available for download (in Hierarchical Data Format), for both the coronal and heliospheric domains3. Figure<\/p>\n<p><a class=\"more-link\" href=\"https:\/\/spreadfast.astro.bas.bg\/index.php\/about\/psi-models\/\">Read More<\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"parent":21,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"_links":{"self":[{"href":"https:\/\/spreadfast.astro.bas.bg\/index.php\/wp-json\/wp\/v2\/pages\/41"}],"collection":[{"href":"https:\/\/spreadfast.astro.bas.bg\/index.php\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/spreadfast.astro.bas.bg\/index.php\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/spreadfast.astro.bas.bg\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/spreadfast.astro.bas.bg\/index.php\/wp-json\/wp\/v2\/comments?post=41"}],"version-history":[{"count":1,"href":"https:\/\/spreadfast.astro.bas.bg\/index.php\/wp-json\/wp\/v2\/pages\/41\/revisions"}],"predecessor-version":[{"id":42,"href":"https:\/\/spreadfast.astro.bas.bg\/index.php\/wp-json\/wp\/v2\/pages\/41\/revisions\/42"}],"up":[{"embeddable":true,"href":"https:\/\/spreadfast.astro.bas.bg\/index.php\/wp-json\/wp\/v2\/pages\/21"}],"wp:attachment":[{"href":"https:\/\/spreadfast.astro.bas.bg\/index.php\/wp-json\/wp\/v2\/media?parent=41"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}