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DTSTAMP:20260720T095710Z
UID:992BD671-C1B2-4371-9035-4101730DD29E
DTSTART;TZID=Australia/Canberra:20260804T190000
DTEND;TZID=Australia/Canberra:20260804T200000
DESCRIPTION:Title: Measuring the Behaviour of Planetary Entry Wake Flows\n\
 nWhen: Tue 04-Aug-26 7:00 PM - 8:00 PM\n\nWhere: https://teams.microsoft.c
 om/l/meetup-join/19%3ameeting_MzkxOTlkYjItNmQzZC00MmM4LTkzMGYtZjFkNmE0OTVh
 YTU0%40thread.v2/0?context=%7b%22Tid%22%3a%223ff6cfa4-e715-48db-b8e1-0867b
 9f9fba3%22%2c%22Oid%22%3a%2254161dc0-27a7-4593-b943-bf35a0e00257%22%7d\n\n
 Speaker: Prof. Sean O’Byrne from ANU\n\nAbstract:\n\nThe flow behind a v
 ehicle entering a planetary atmosphere is very challenging to model\, beca
 use the density is very low\, allowing the flow to slide along surfaces an
 d because counter-rotating vortices are set up that can produce a range of
  possible flow configurations\, as seen in the recent Artemis re-entry fli
 ghts. These conditions can\, however\, be investigated in the controlled c
 onditions achieveable in hypersonic ground test facilities using laser-bas
 ed measurement techniques. This talk will summarise some of the measuremen
 t techniques that have been developed to investigate these fascinating flo
 ws.\n\nBio: []Sean O&#39;Byrne is the Professor of Aerospace Engineering at th
 e Australian National University. Prior to his ANU appointment in 2023\, h
 e worked at NASA Langly Research Centre in Virginia and for 20 years teach
 ing engineers and doing research at the Australian Defence Force Academy. 
 His research interests have mostly been associated with the design of lase
 r-based fluid sensing systems for high-speed flight\, but he has also been
  involved with experiments on supersonic combustion ramjet engines and pla
 netary entry physics\, as well as the dynamics of short-duration plasmas.\
 n\nVirtual: https://events.vtools.ieee.org/m/568767
LOCATION:Virtual: https://events.vtools.ieee.org/m/568767
ORGANIZER:l.qiao@unsw.edu.au
SEQUENCE:18
SUMMARY:IEEE AESS ACT Seminar Measuring the Behaviour of Planetary Entry Wa
 ke Flows
URL;VALUE=URI:https://events.vtools.ieee.org/m/568767
X-ALT-DESC:Description: &lt;br /&gt;&lt;p&gt;&lt;strong&gt;&lt;span style=&quot;color: black\; mso-co
 lor-alt: windowtext\; background: white\;&quot;&gt;Title: &lt;/span&gt;&lt;/strong&gt;&lt;span st
 yle=&quot;mso-fareast-font-family: Calibri\; color: black\; mso-themecolor: tex
 t1\;&quot;&gt;Measuring the Behaviour of Planetary Entry Wake Flows&lt;/span&gt;&lt;/p&gt;\n&lt;p
 &gt;&lt;strong&gt;&lt;span style=&quot;color: black\; mso-color-alt: windowtext\; backgroun
 d: white\;&quot;&gt;When: &lt;/span&gt;&lt;/strong&gt;&lt;span style=&quot;font-size: 10.5pt\; font-fa
 mily: &#39;Segoe UI&#39;\,sans-serif\; color: #424242\; background: white\;&quot;&gt;Tue 0
 4-Aug-26 7:00 PM - 8:00 PM&lt;/span&gt;&lt;/p&gt;\n&lt;p&gt;&lt;strong&gt;&lt;span style=&quot;color: blac
 k\; mso-color-alt: windowtext\; background: white\;&quot;&gt;Where: &lt;a href=&quot;https
 ://teams.microsoft.com/l/meetup-join/19%3ameeting_MzkxOTlkYjItNmQzZC00MmM4
 LTkzMGYtZjFkNmE0OTVhYTU0%40thread.v2/0?context=%7b%22Tid%22%3a%223ff6cfa4-
 e715-48db-b8e1-0867b9f9fba3%22%2c%22Oid%22%3a%2254161dc0-27a7-4593-b943-bf
 35a0e00257%22%7d&quot;&gt;https://teams.microsoft.com/l/meetup-join/19%3ameeting_M
 zkxOTlkYjItNmQzZC00MmM4LTkzMGYtZjFkNmE0OTVhYTU0%40thread.v2/0?context=%7b%
 22Tid%22%3a%223ff6cfa4-e715-48db-b8e1-0867b9f9fba3%22%2c%22Oid%22%3a%22541
 61dc0-27a7-4593-b943-bf35a0e00257%22%7d&lt;/a&gt; &lt;/span&gt;&lt;/strong&gt;&lt;/p&gt;\n&lt;p&gt;&lt;stro
 ng&gt;&lt;span style=&quot;color: black\; mso-color-alt: windowtext\; background: whi
 te\;&quot;&gt;Speaker: Prof. Sean O&amp;rsquo\;Byrne from ANU&lt;/span&gt;&lt;/strong&gt;&lt;/p&gt;\n&lt;p&gt;
 &lt;strong&gt;&lt;span style=&quot;color: black\; mso-color-alt: windowtext\; background
 : white\;&quot;&gt;Abstract: &lt;/span&gt;&lt;/strong&gt;&lt;/p&gt;\n&lt;p&gt;The flow behind a vehicle en
 tering a planetary atmosphere is very challenging to model\, because the d
 ensity is very low\, allowing the flow to slide along surfaces and because
  counter-rotating vortices are set up that can produce a range of possible
  flow configurations\, as seen in the recent Artemis re-entry flights.&lt;spa
 n style=&quot;mso-spacerun: yes\;&quot;&gt;&amp;nbsp\; &lt;/span&gt;These conditions can\, howeve
 r\, be investigated in the controlled conditions achieveable in hypersonic
  ground test facilities using laser-based measurement techniques.&lt;span sty
 le=&quot;mso-spacerun: yes\;&quot;&gt;&amp;nbsp\; &lt;/span&gt;This talk will summarise some of t
 he measurement techniques that have been developed to investigate these fa
 scinating flows.&lt;/p&gt;\n&lt;p&gt;&lt;strong&gt;&lt;span style=&quot;color: black\; mso-color-alt
 : windowtext\; background: white\;&quot;&gt;Bio: &lt;/span&gt;&lt;/strong&gt;&lt;a name=&quot;OLE_LINK
 3&quot;&gt;&lt;/a&gt;&lt;span style=&quot;mso-fareast-font-family: Aptos\; color: black\; mso-th
 emecolor: text1\;&quot;&gt;Sean O&#39;Byrne is the Professor of Aerospace Engineering 
 at the Australian National University.&lt;span style=&quot;mso-spacerun: yes\;&quot;&gt;&amp;n
 bsp\; &lt;/span&gt;Prior to his ANU appointment in 2023\, he worked at NASA Lang
 ly Research Centre in Virginia and for 20 years teaching engineers and doi
 ng research at the Australian Defence Force Academy.&lt;span style=&quot;mso-space
 run: yes\;&quot;&gt;&amp;nbsp\; &lt;/span&gt;His research interests have mostly been associa
 ted with the design of laser-based fluid sensing systems for high-speed fl
 ight\, but he has also been involved with experiments on supersonic combus
 tion ramjet engines and planetary entry physics\, as well as the dynamics 
 of short-duration plasmas.&lt;/span&gt;&lt;/p&gt;
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