{"version":"1.0","provider_name":"AGN Driven Winds","provider_url":"https:\/\/phsites.technion.ac.il\/agn-2017","author_name":"Adi","author_url":"https:\/\/phsites.technion.ac.il\/agn-2017\/author\/adile\/","title":"S. Davis - Simulations of accretion flows with grey opacities - AGN Driven Winds","type":"rich","width":600,"height":338,"html":"<blockquote class=\"wp-embedded-content\" data-secret=\"0bTk26PoOv\"><a href=\"https:\/\/phsites.technion.ac.il\/agn-2017\/s-davis-simulations-accretion-flows-grey-opacities\/\">S. Davis &#8211; Simulations of accretion flows with grey opacities<\/a><\/blockquote><iframe sandbox=\"allow-scripts\" security=\"restricted\" src=\"https:\/\/phsites.technion.ac.il\/agn-2017\/s-davis-simulations-accretion-flows-grey-opacities\/embed\/#?secret=0bTk26PoOv\" width=\"600\" height=\"338\" title=\"&#8220;S. Davis &#8211; Simulations of accretion flows with grey opacities&#8221; &#8212; AGN Driven Winds\" data-secret=\"0bTk26PoOv\" frameborder=\"0\" marginwidth=\"0\" marginheight=\"0\" scrolling=\"no\" class=\"wp-embedded-content\"><\/iframe><script type=\"text\/javascript\">\n\/* <![CDATA[ *\/\n\/*! This file is auto-generated *\/\n!function(d,l){\"use strict\";l.querySelector&&d.addEventListener&&\"undefined\"!=typeof URL&&(d.wp=d.wp||{},d.wp.receiveEmbedMessage||(d.wp.receiveEmbedMessage=function(e){var t=e.data;if((t||t.secret||t.message||t.value)&&!\/[^a-zA-Z0-9]\/.test(t.secret)){for(var s,r,n,a=l.querySelectorAll('iframe[data-secret=\"'+t.secret+'\"]'),o=l.querySelectorAll('blockquote[data-secret=\"'+t.secret+'\"]'),c=new RegExp(\"^https?:$\",\"i\"),i=0;i<o.length;i++)o[i].style.display=\"none\";for(i=0;i<a.length;i++)s=a[i],e.source===s.contentWindow&&(s.removeAttribute(\"style\"),\"height\"===t.message?(1e3<(r=parseInt(t.value,10))?r=1e3:~~r<200&&(r=200),s.height=r):\"link\"===t.message&&(r=new URL(s.getAttribute(\"src\")),n=new URL(t.value),c.test(n.protocol))&&n.host===r.host&&l.activeElement===s&&(d.top.location.href=t.value))}},d.addEventListener(\"message\",d.wp.receiveEmbedMessage,!1),l.addEventListener(\"DOMContentLoaded\",function(){for(var e,t,s=l.querySelectorAll(\"iframe.wp-embedded-content\"),r=0;r<s.length;r++)(t=(e=s[r]).getAttribute(\"data-secret\"))||(t=Math.random().toString(36).substring(2,12),e.src+=\"#?secret=\"+t,e.setAttribute(\"data-secret\",t)),e.contentWindow.postMessage({message:\"ready\",secret:t},\"*\")},!1)))}(window,document);\n\/\/# sourceURL=https:\/\/phsites.technion.ac.il\/agn-2017\/wp-includes\/js\/wp-embed.min.js\n\/* ]]> *\/\n<\/script>\n","description":"See Presentation What role does UV opacity play in the structure and evolution of accretion disks? \u00a0What can simulations tell us about how winds are launched by radiation and, in particular, how that launching feeds back on the disk structure? \u00a0Given the limits of numerical simulations, how can we best design the simulations that address &hellip;"}