{"id":229,"date":"2019-07-18T02:59:52","date_gmt":"2019-07-18T02:59:52","guid":{"rendered":"https:\/\/gonewithsolarwind.com\/?page_id=229"},"modified":"2019-07-18T03:21:41","modified_gmt":"2019-07-18T03:21:41","slug":"second-working-meeting-on-use-of-vector-synoptic-maps-for-modeling","status":"publish","type":"page","link":"https:\/\/gonewithsolarwind.com\/index.php\/second-working-meeting-on-use-of-vector-synoptic-maps-for-modeling\/","title":{"rendered":"Second working meeting on Use of Vector Synoptic Maps for Modeling"},"content":{"rendered":"\n<ul><li><a href=\"http:\/\/spd.stanford.edu\/\/SolarNews\/2017\/20170701.html#section_pevtsov\">First announcement<\/a><\/li><li>Dates: 6-10 November, 2017\u00a0 (6 November &#8211; travel day), 7- 10 November (3 full and one half days)<\/li><li>Location: <a href=\"https:\/\/www.google.com\/maps\/place\/Space+Science,+3665+Discovery+Dr,+Boulder,+CO+80303\/@40.0117958,-105.2479205,17z\/data=!3m1!4b1!4m5!3m4!1s0x876bedc3b5625603:0x725ff0c791cb1ebc!8m2!3d40.0118841!4d-105.2458178\">National Solar Observatory, 3665 Discovery Drive, 3rd Floor, Boulder, CO 80303<\/a><\/li><li><a href=\"https:\/\/www-dev.nso.edu\/node\/1606\">Lodging and travel info<\/a><\/li><li><a href=\"https:\/\/gonewithsolarwind.com\/index.php\/vector-synoptic-maps-meeting-2-agenda\/\">Meeting agenda<\/a> (including presentation slides)<\/li><li>List of major topics that meeting discussions concentrated on:<\/li><\/ul>\n\n\n\n<ol><li>Utility of vector synoptic maps:\n&nbsp;a). what improvements in modeling we see from using&nbsp; true radial vs.\n pseudo-radial field maps, are horizontal fields important for modeling,\n synoptic maps of pseudo-radial derived from other functional dependency\n (not cosine of heliocentric position)<br>&nbsp;b). what are limitations of \nvector synoptic data as compared with &#8220;traditional&#8221; LOS data and how to \nmitigate\/address these limitations (e.g., the effect of noise, ambiguity\n resolution).<br>&nbsp;c). specifics for integer and near-real-time synoptic maps (noise, uncertainties).<br>&nbsp;d). what is the best way to represent uncertainties in vector synoptic maps\n<\/li><li>How to deal with polar fields in vector synoptic maps\n&nbsp;a). what are the (best) approaches to fill poles in vector data and what are the effects on model outcomes<br>&nbsp;b).\n how important is to &#8220;fill poles&#8221; at low spatial resolution (more \nuniformed, less structured) or high\/moderate resolution (highly \nstructured).\n<\/li><li>Magnetic flux calibration of vector magnetograms and synergy with \nhigh-resolution &#8220;synoptic&#8221; observations from DKIST (and other high-res \ninstruments).\na). new approaches in calibrating the magnetic field data \n(combination of MHD\/radiative transfer\/instrument models for end-to-end \ncalibration).<br>b). new approaches in comparing\/cross-calibrating magnetic data from different instruments (e.g., using spherical harmonics).\n<\/li><\/ol>\n\n\n\n<ul><li>Meeting Organizers:\n<ul><li>Alexei Pevtsov (NSO, USA)<\/li><li>Luca Bertello (NSO, USA)<\/li><li>Gordon Petrie (NSO, USA)<\/li><li>Ilpo Virtanen (Un. of Oulu, Finland)<\/li><\/ul><\/li><\/ul>\n","protected":false},"excerpt":{"rendered":"<p>First announcement Dates: 6-10 November, 2017\u00a0 (6 November &#8211; travel day), 7- 10 November (3 full and one half days) Location: National Solar Observatory, 3665 Discovery Drive, 3rd Floor, Boulder, CO 80303 Lodging and travel info Meeting agenda (including presentation slides) List of major topics that meeting discussions concentrated on: Utility of vector synoptic maps: &hellip; <\/p>\n<p class=\"link-more\"><a href=\"https:\/\/gonewithsolarwind.com\/index.php\/second-working-meeting-on-use-of-vector-synoptic-maps-for-modeling\/\" class=\"more-link\">Continue reading<span class=\"screen-reader-text\"> &#8220;Second working meeting on Use of Vector Synoptic Maps for Modeling&#8221;<\/span><\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"_links":{"self":[{"href":"https:\/\/gonewithsolarwind.com\/index.php\/wp-json\/wp\/v2\/pages\/229"}],"collection":[{"href":"https:\/\/gonewithsolarwind.com\/index.php\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/gonewithsolarwind.com\/index.php\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/gonewithsolarwind.com\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/gonewithsolarwind.com\/index.php\/wp-json\/wp\/v2\/comments?post=229"}],"version-history":[{"count":2,"href":"https:\/\/gonewithsolarwind.com\/index.php\/wp-json\/wp\/v2\/pages\/229\/revisions"}],"predecessor-version":[{"id":238,"href":"https:\/\/gonewithsolarwind.com\/index.php\/wp-json\/wp\/v2\/pages\/229\/revisions\/238"}],"wp:attachment":[{"href":"https:\/\/gonewithsolarwind.com\/index.php\/wp-json\/wp\/v2\/media?parent=229"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}