{"id":290,"date":"2020-02-29T01:03:47","date_gmt":"2020-02-28T23:03:47","guid":{"rendered":"http:\/\/cosmicrays.oulu.fi\/espera\/?p=290"},"modified":"2020-03-05T19:37:52","modified_gmt":"2020-03-05T17:37:52","slug":"a-kick-off-ruka-meeting-agenda-is-available","status":"publish","type":"post","link":"https:\/\/cosmicrays.oulu.fi\/espera\/index.php\/2020\/02\/29\/a-kick-off-ruka-meeting-agenda-is-available\/","title":{"rendered":"The program of the kick-off meeting is available"},"content":{"rendered":"\n<p>The program of the kick-off meeting is <a href=\"https:\/\/drive.google.com\/file\/d\/1NTWxzfdjUxA7cGgBvcaX0jg_I22yF5H9\/view?usp=sharing\">available<\/a>.<\/p>\n\n\n\n<p>Our plan: a three-day productive teamwork and discussion.<\/p>\n\n\n\n<p><\/p>\n\n\n\n<p class=\"has-text-align-center\">The first day (<strong>30th March<\/strong>) will start <strong>at 4 p.m.<\/strong><\/p>\n\n\n\n<div class=\"wp-container-6a8ae14cedfb1 wp-block-group\"><div class=\"wp-block-group__inner-container\">\n<p>16:00 &#8211; 16:15 <em>Introduction<\/em> by Ilya Usoskin<\/p>\n\n\n\n<p>16:15 &#8211; 17:00 <em>New method of SEP integral fluence reconstruction for GLE   events: description and results<\/em> by Sergey Koldobskiy <\/p>\n\n\n\n<p>17:00 &#8211; 17:30 <em>Modelled production of cosmogenic nuclides in the   atmosphere&nbsp;<\/em><\/p>\n\n\n\n<p>17:30 &#8211; 18:00 <em>Cleaned DB of NM data<\/em> by Pauli V\u00e4is\u00e4nen<\/p>\n\n\n\n<p><\/p>\n\n\n\n<p><\/p>\n\n\n\n<p><\/p>\n<\/div><\/div>\n\n\n\n<p class=\"has-text-align-center\">The second day (<strong>31th March<\/strong>) will start <strong>at 9 a.m.<\/strong> It long day, which will be end with <a href=\"http:\/\/cosmicrays.oulu.fi\/espera\/index.php\/2020\/02\/19\/welcome-dinner\/\">welcome dinner<\/a>.<\/p>\n\n\n\n<div class=\"wp-container-6a8ae14cee279 wp-block-group\"><div class=\"wp-block-group__inner-container\">\n<p>9:00 &#8211; 9:45 <em>Measurements of 14C in trees,  process of 14C uptake, tree growth, late\/early wood<\/em> by Joonas Uusitalo<\/p>\n\n\n\n<p>9:45 &#8211; 10:15 <em>Modelling of cosmogenic-isotope transport in the atmosphere<\/em> by Eugene Rozanov <\/p>\n\n\n\n<p>10:15 &#8211; 10:45 <em>Status of SOCOL modeling<\/em> by Kseniia Golubenko<\/p>\n\n\n\n<p>10:45 &#8211; 12:45 Lunch break <\/p>\n\n\n\n<p>12:45 &#8211; 15:30 Brainstorming<\/p>\n\n\n\n<p>15:30 &#8211; 18:00 free time<\/p>\n\n\n\n<p>18:00 &#8211; 21:00 Conference Dinner<\/p>\n<\/div><\/div>\n\n\n\n<p><\/p>\n\n\n\n<p><\/p>\n\n\n\n<p class=\"has-text-align-center\">The last <em>working<\/em> day (<strong>1st April<\/strong>) will start <strong>at 9 a.m.<\/strong> <\/p>\n\n\n\n<div class=\"wp-container-6a8ae14cee586 wp-block-group\"><div class=\"wp-block-group__inner-container\">\n<p>9:00 &#8211; 10:00 <em>Revised open solar flux model, and   irradiance variability during superflares<\/em> by Natalia Krivova<\/p>\n\n\n\n<p>10:00 &#8211; 11:00 <em>Constancy of GCR in VLISM and GRB<\/em> by Igor Moskalenko<\/p>\n\n\n\n<p>11:00 &#8211; 13:00 LUNCH<\/p>\n\n\n\n<p>13:00 &#8211; 15:30 Brainstorming<\/p>\n\n\n\n<p>15:30 &#8211; 16:00 Coffee-break<\/p>\n\n\n\n<p>16:00 &#8211; 16:30 <em>Climate effects of extreme solar events<\/em> by Eugene Rozanov<\/p>\n\n\n\n<p>16:30 &#8211; 17:30 <em>Strong solar particle events and related radiation space   weather effects<\/em> by Alexander Mishev<\/p>\n\n\n\n<p>17:30 &#8211; 18:00 <em>Reconstruction of mean GCR and SEP fluxes from lunar Al-26\u00a0<\/em>by Stepan Poluianov<\/p>\n\n\n\n<p>18:00 &#8211; 18:30 Wrap-up<\/p>\n\n\n\n<p><\/p>\n\n\n\n<p><\/p>\n\n\n\n<p><\/p>\n\n\n\n<p class=\"has-text-align-center\">The last <em>meeting<\/em> day (<strong>2nd April<\/strong>). <\/p>\n\n\n\n<p><\/p>\n\n\n\n<p><\/p>\n<\/div><\/div>\n\n\n\n<p class=\"has-text-align-center\">Looking forward to the meeting!<\/p>\n","protected":false},"excerpt":{"rendered":"<p>The program of the kick-off meeting is available. Our plan: a three-day productive teamwork and discussion. The first day (30th March) will start at 4 p.m. 16:00 &#8211; 16:15 Introduction by Ilya Usoskin 16:15 &#8211; 17:00 New method of SEP integral fluence reconstruction for GLE events: description and results by Sergey Koldobskiy 17:00 &#8211; 17:30 <span class=\"ellipsis\">&hellip;<\/span> <span class=\"more-link-wrap\"><a href=\"https:\/\/cosmicrays.oulu.fi\/espera\/index.php\/2020\/02\/29\/a-kick-off-ruka-meeting-agenda-is-available\/\" class=\"more-link\"><span>Read More &rarr;<\/span><\/a><\/span><\/p>\n","protected":false},"author":2,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":[],"categories":[5],"tags":[],"_links":{"self":[{"href":"https:\/\/cosmicrays.oulu.fi\/espera\/index.php\/wp-json\/wp\/v2\/posts\/290"}],"collection":[{"href":"https:\/\/cosmicrays.oulu.fi\/espera\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/cosmicrays.oulu.fi\/espera\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/cosmicrays.oulu.fi\/espera\/index.php\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/cosmicrays.oulu.fi\/espera\/index.php\/wp-json\/wp\/v2\/comments?post=290"}],"version-history":[{"count":17,"href":"https:\/\/cosmicrays.oulu.fi\/espera\/index.php\/wp-json\/wp\/v2\/posts\/290\/revisions"}],"predecessor-version":[{"id":318,"href":"https:\/\/cosmicrays.oulu.fi\/espera\/index.php\/wp-json\/wp\/v2\/posts\/290\/revisions\/318"}],"wp:attachment":[{"href":"https:\/\/cosmicrays.oulu.fi\/espera\/index.php\/wp-json\/wp\/v2\/media?parent=290"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/cosmicrays.oulu.fi\/espera\/index.php\/wp-json\/wp\/v2\/categories?post=290"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/cosmicrays.oulu.fi\/espera\/index.php\/wp-json\/wp\/v2\/tags?post=290"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}