{"id":2,"date":"2023-10-11T08:53:39","date_gmt":"2023-10-11T08:53:39","guid":{"rendered":"https:\/\/cosmicrays.oulu.fi\/geraclis2024\/?page_id=2"},"modified":"2024-03-01T08:41:37","modified_gmt":"2024-03-01T08:41:37","slug":"sample-page","status":"publish","type":"page","link":"https:\/\/cosmicrays.oulu.fi\/geraclis2024\/?page_id=2","title":{"rendered":"Agenda"},"content":{"rendered":"\n<p><strong>5 March 2024: <\/strong><em>providing a theoretical overview of the main processes affected by changes in the geomagnetic field and their potential atmospheric impact<\/em>\u00a0<\/p>\n\n\n\n<p>11:00-11:30 short Introduction by Ilya\u00a0Usoskin\u00a0<\/p>\n\n\n\n<p>11:30-12:00 Ilya Usoskin \u201cPossible effect of a GE\/R on the magnetosphere and radiation field\u201d.\u00a0<\/p>\n\n\n\n<p>12:00-13:00&nbsp;Lunch&nbsp;<\/p>\n\n\n\n<p>13:00-13:30 Nick Larsen\u00a0\u201cUsing OTSO to compute geomagnetic cut-offs during non-standard geomagnetic conditions\u201d\u00a0<\/p>\n\n\n\n<p>13:30 \u2013 14:00 Sergey Koldobskiy \u201cExtreme solar particle events registered in cosmogenic isotopes and their spectra\u201d.\u00a0<\/p>\n\n\n\n<p>14.00 &#8211; 14.30 Sanja Panovska \u201cGlobal reconstructions of the geomagnetic field in transitional states\u201d.\u00a0<\/p>\n\n\n\n<p>14.30 &#8211; 15.00 Aleksandar Mishev \u201cApplication of the global NM network for study of SEP induced terrestrial effects\u00a0\u201d.\u00a0<\/p>\n\n\n\n<p>15.00 &#8211; 15.30 Coffee&nbsp;<\/p>\n\n\n\n<p>15.30&nbsp;&#8211; 16.30 Discussions&nbsp;<\/p>\n\n\n\n<p><em><strong>6 March 2024: <\/strong>climate model day: set up and expectation<\/em> \u00a0<\/p>\n\n\n\n<p>10:30-11:00 Eija Tanskanen \u201cMagnetic disturbances in the Sun-Earth coupling\u201d.\u00a0<\/p>\n\n\n\n<p>WACCM&nbsp;<\/p>\n\n\n\n<p>11:00-11:30 Monika Szelag \u201cWACCM at FMI &#8211; Overview\u201d\u00a0<\/p>\n\n\n\n<p>11:30-12:00 Niilo Kalakoski \u201cOzone loss from extreme solar proton events in WACCM-D\u201d\u00a0<\/p>\n\n\n\n<p>12:00-13:00 Lunch&nbsp;<\/p>\n\n\n\n<p>SOCOL&nbsp;<\/p>\n\n\n\n<p>13:00 \u2013 13:30 Kseniia Golubenko\u00a0\u201cWhat to expect from GE\/R and how to model it using the SOCOLv4. Part I\u201d\u00a0<\/p>\n\n\n\n<p>13:30 \u2013 14:00 Eugene Rozanov \u201cWhat to expect from GE\/R and how to model it using the SOCOLv4. Part II\u201d\u00a0<\/p>\n\n\n\n<p>14:00 &#8211; 14:30 Timofei Sukhodolov \u201cAdjacent ongoing and upcoming projects involving SOCOLv4\u201d\u00a0<\/p>\n\n\n\n<p>14:30 &#8211; 15:00 Coffee&nbsp;<\/p>\n\n\n\n<p>15:00 &#8211; 17:00 Discussions&nbsp;<\/p>\n\n\n\n<p>18:00 &#8211; dinner at Ravintola Marani (<a rel=\"noreferrer noopener\" href=\"https:\/\/www.google.ru\/maps\/place\/\/data=!4m2!3m1!1s0x4680332f81c99601:0x70b0e151a1084a04?sa=X&amp;ved=2ahUKEwittaSri5mEAxWjFBAIHcv7C2MQ4kB6BAggEAA\" target=\"_blank\">Pakkahuoneenkatu 8, 90100 Oulu<\/a>).<\/p>\n\n\n\n<p><em><strong>7 March 2024: <\/strong>introducing high-performance computing resources for possible simulations <\/em>\u00a0<\/p>\n\n\n\n<p>10:30-10:45 Juhani Kataja \u201cThe LUMI system\u201d\u00a0<\/p>\n\n\n\n<p>10:45-11:00 Cristian-Vasile Achim \u201cThe Mahti system\u201d\u00a0\u00a0<\/p>\n\n\n\n<p>11:00-11:20 Timofei Sukhodolov (implementation of SOCOL)\u00a0<\/p>\n\n\n\n<p>11:20-11:45 Monika Szelag (implementation of WACCM)\u00a0<\/p>\n\n\n\n<p>11:45-12:30 Lunch&nbsp;<\/p>\n\n\n\n<p>12:30 \u2013 14:30 Brainstorming&nbsp;<\/p>\n\n\n\n<p>14:30 &#8211; 15:00 coffee break&nbsp;<\/p>\n\n\n\n<p>15:00 Future plans and conclusions&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>5 March 2024: providing a theoretical overview of the main processes affected by changes in the geomagnetic field and their potential atmospheric impact\u00a0 11:00-11:30 short Introduction by Ilya\u00a0Usoskin\u00a0 11:30-12:00 Ilya Usoskin \u201cPossible effect of a GE\/R on the magnetosphere and radiation field\u201d.\u00a0 12:00-13:00&nbsp;Lunch&nbsp; 13:00-13:30 Nick Larsen\u00a0\u201cUsing OTSO to compute geomagnetic cut-offs during non-standard geomagnetic conditions\u201d\u00a0 [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"open","template":"","meta":{"footnotes":""},"_links":{"self":[{"href":"https:\/\/cosmicrays.oulu.fi\/geraclis2024\/index.php?rest_route=\/wp\/v2\/pages\/2"}],"collection":[{"href":"https:\/\/cosmicrays.oulu.fi\/geraclis2024\/index.php?rest_route=\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/cosmicrays.oulu.fi\/geraclis2024\/index.php?rest_route=\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/cosmicrays.oulu.fi\/geraclis2024\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/cosmicrays.oulu.fi\/geraclis2024\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=2"}],"version-history":[{"count":3,"href":"https:\/\/cosmicrays.oulu.fi\/geraclis2024\/index.php?rest_route=\/wp\/v2\/pages\/2\/revisions"}],"predecessor-version":[{"id":46,"href":"https:\/\/cosmicrays.oulu.fi\/geraclis2024\/index.php?rest_route=\/wp\/v2\/pages\/2\/revisions\/46"}],"wp:attachment":[{"href":"https:\/\/cosmicrays.oulu.fi\/geraclis2024\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=2"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}