BEGIN:VCALENDAR
VERSION:2.0
PRODID:IEEE vTools.Events//EN
CALSCALE:GREGORIAN
BEGIN:VTIMEZONE
TZID:America/New_York
BEGIN:DAYLIGHT
DTSTART:20260308T030000
TZOFFSETFROM:-0500
TZOFFSETTO:-0400
RRULE:FREQ=YEARLY;BYDAY=2SU;BYMONTH=3
TZNAME:EDT
END:DAYLIGHT
BEGIN:STANDARD
DTSTART:20261101T010000
TZOFFSETFROM:-0400
TZOFFSETTO:-0500
RRULE:FREQ=YEARLY;BYDAY=1SU;BYMONTH=11
TZNAME:EST
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTAMP:20260928T170748Z
UID:8F74D37E-9E4E-435D-928E-10E218B4B4D7
DTSTART;TZID=America/New_York:20261007T151000
DTEND;TZID=America/New_York:20261007T163000
DESCRIPTION:Accurate simulations of fusion experiments and astrophysical ob
 jects such as stars require material data including equation of state\, op
 acity\, and particle transport coefficients under extreme conditions. Thes
 e conditions range from approximately 10\,000 to 100\,000\,000 K and densi
 ties from 1 to 1\,000\,000 g/cm³.\nIn these regimes\, atoms are partially
  ionized and significantly overlap\, making conventional low-density plasm
 a physics methods inaccurate. Dr. Charles Starrett will discuss methods de
 veloped by his research group at Los Alamos National Laboratory to accurat
 ely model these plasmas\, review recent progress\, and discuss major outst
 anding challenges in this rapidly developing field.\n\nAgenda: \n3:10 PM 
 – Welcome and introduction\nTechnical presentation – Material Properti
 es Inside Stars and Fusion Plasmas\nQuestions and discussion\nConclusion\n
 \nRoom: 1003 EECS\, Bldg: Electrical Engineering and Computer Science Buil
 ding\, 36 EECS Bldg.\, 1301 Beal Avenue\, Ann Arbor\, Michigan\, United St
 ates\, 48109\, Virtual: https://events.vtools.ieee.org/m/580498
LOCATION:Room: 1003 EECS\, Bldg: Electrical Engineering and Computer Scienc
 e Building\, 36 EECS Bldg.\, 1301 Beal Avenue\, Ann Arbor\, Michigan\, Uni
 ted States\, 48109\, Virtual: https://events.vtools.ieee.org/m/580498
ORGANIZER:jomidoku@umich.edu
SEQUENCE:0
SUMMARY:MIPSE Early Career Award – Material Properties Inside Stars and F
 usion Plasmas
URL;VALUE=URI:https://events.vtools.ieee.org/m/580498
X-ALT-DESC:Description: &lt;br /&gt;&lt;p&gt;Accurate simulations of fusion experiments
  and astrophysical objects such as stars require material data including e
 quation of state\, opacity\, and particle transport coefficients under ext
 reme conditions. These conditions range from approximately 10\,000 to 100\
 ,000\,000 K and densities from 1 to 1\,000\,000 g/cm&amp;sup3\;.&lt;br&gt;In these r
 egimes\, atoms are partially ionized and significantly overlap\, making co
 nventional low-density plasma physics methods inaccurate. Dr. Charles Star
 rett will discuss methods developed by his research group at Los Alamos Na
 tional Laboratory to accurately model these plasmas\, review recent progre
 ss\, and discuss major outstanding challenges in this rapidly developing f
 ield.&lt;/p&gt;&lt;br /&gt;&lt;br /&gt;Agenda: &lt;br /&gt;&lt;p&gt;3:10 PM &amp;ndash\; Welcome and introdu
 ction&lt;br&gt;Technical presentation &amp;ndash\; &lt;em&gt;Material Properties Inside St
 ars and Fusion Plasmas&lt;/em&gt;&lt;br&gt;Questions and discussion&lt;br&gt;Conclusion&lt;/p&gt;
END:VEVENT
END:VCALENDAR