BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//jEvents 2.0 for Joomla//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
BEGIN:VTIMEZONE
TZID:Australia/Sydney
BEGIN:STANDARD
DTSTART:20200602T193000
RDATE:20201004T030000
TZOFFSETFROM:+1100
TZOFFSETTO:+1000
TZNAME:Australia/Sydney AEST
END:STANDARD
BEGIN:STANDARD
DTSTART:20210404T020000
RDATE:20211003T030000
TZOFFSETFROM:+1100
TZOFFSETTO:+1000
TZNAME:Australia/Sydney AEST
END:STANDARD
BEGIN:STANDARD
DTSTART:20220403T020000
RDATE:20221002T030000
TZOFFSETFROM:+1100
TZOFFSETTO:+1000
TZNAME:Australia/Sydney AEST
END:STANDARD
BEGIN:STANDARD
DTSTART:20230402T020000
RDATE:20231001T030000
TZOFFSETFROM:+1100
TZOFFSETTO:+1000
TZNAME:Australia/Sydney AEST
END:STANDARD
BEGIN:STANDARD
DTSTART:20240407T020000
RDATE:20241006T030000
TZOFFSETFROM:+1100
TZOFFSETTO:+1000
TZNAME:Australia/Sydney AEST
END:STANDARD
BEGIN:STANDARD
DTSTART:20250406T020000
RDATE:20251005T030000
TZOFFSETFROM:+1100
TZOFFSETTO:+1000
TZNAME:Australia/Sydney AEST
END:STANDARD
BEGIN:STANDARD
DTSTART:20260405T020000
RDATE:20261004T030000
TZOFFSETFROM:+1100
TZOFFSETTO:+1000
TZNAME:Australia/Sydney AEST
END:STANDARD
BEGIN:STANDARD
DTSTART:20270404T020000
RDATE:20271003T030000
TZOFFSETFROM:+1100
TZOFFSETTO:+1000
TZNAME:Australia/Sydney AEST
END:STANDARD
BEGIN:STANDARD
DTSTART:20280402T020000
RDATE:20281001T030000
TZOFFSETFROM:+1100
TZOFFSETTO:+1000
TZNAME:Australia/Sydney AEST
END:STANDARD
BEGIN:DAYLIGHT
DTSTART:20201004T030000
RDATE:20210404T020000
TZOFFSETFROM:+1000
TZOFFSETTO:+1100
TZNAME:Australia/Sydney AEDT
END:DAYLIGHT
BEGIN:DAYLIGHT
DTSTART:20211003T030000
RDATE:20220403T020000
TZOFFSETFROM:+1000
TZOFFSETTO:+1100
TZNAME:Australia/Sydney AEDT
END:DAYLIGHT
BEGIN:DAYLIGHT
DTSTART:20221002T030000
RDATE:20230402T020000
TZOFFSETFROM:+1000
TZOFFSETTO:+1100
TZNAME:Australia/Sydney AEDT
END:DAYLIGHT
BEGIN:DAYLIGHT
DTSTART:20231001T030000
RDATE:20240407T020000
TZOFFSETFROM:+1000
TZOFFSETTO:+1100
TZNAME:Australia/Sydney AEDT
END:DAYLIGHT
BEGIN:DAYLIGHT
DTSTART:20241006T030000
RDATE:20250406T020000
TZOFFSETFROM:+1000
TZOFFSETTO:+1100
TZNAME:Australia/Sydney AEDT
END:DAYLIGHT
BEGIN:DAYLIGHT
DTSTART:20251005T030000
RDATE:20260405T020000
TZOFFSETFROM:+1000
TZOFFSETTO:+1100
TZNAME:Australia/Sydney AEDT
END:DAYLIGHT
BEGIN:DAYLIGHT
DTSTART:20261004T030000
RDATE:20270404T020000
TZOFFSETFROM:+1000
TZOFFSETTO:+1100
TZNAME:Australia/Sydney AEDT
END:DAYLIGHT
BEGIN:DAYLIGHT
DTSTART:20271003T030000
RDATE:20280402T020000
TZOFFSETFROM:+1000
TZOFFSETTO:+1100
TZNAME:Australia/Sydney AEDT
END:DAYLIGHT
BEGIN:DAYLIGHT
DTSTART:20281001T030000
RDATE:20290401T020000
TZOFFSETFROM:+1000
TZOFFSETTO:+1100
TZNAME:Australia/Sydney AEDT
END:DAYLIGHT
END:VTIMEZONE
BEGIN:VEVENT
UID:73868db78cf23e1f84347445eb128fb7
CATEGORIES:Guest Speaker Night
CREATED:20210329T214858
SUMMARY:Guest Speaker - Dr Paul Hancock (Curtin University)
LOCATION:Zoom Meeting - members will be invited
DESCRIPTION:Space Debris and an update on the SKA \nDr Paul HancockI am an Early Career
  Research Fellow currently at Curtin University. I obtained my PhD at the U
 niversity of Sydney, where I worked on the Australia Telescope 20GHz (AT20G
 ) survey. I then continued to work as a Super Science Fellow in radio trans
 ients at USYD where I helped to create the Variable And Slow Transients (VA
 ST) prototype pipeline, including the source finding algorithm Aegean. My i
 nterests are in radio transients including: supernovae, gamma-ray bursts, a
 nd tidal disruption events.\nI lead two projects that use the Murchison Wid
 e-field Array (MWA). The first project uses the scintillation of extragalac
 tic radio sources to trace the turbulent structure of gas within the Milky 
 Way. The second project uses the MWA to search for radio emission from fire
 balls as they burn a path through our atmosphere.\n
X-ALT-DESC;FMTTYPE=text/html:<h2>Space Debris and an update on the SKA</h2><p>&nbsp;</p><h2><img src="ht
 tps://www.sasi.net.au/images/articles/Dr_Paul_Hancock.png" alt="Dr Paul Han
 cock photo" style="margin-right: 10px; float: left;" />Dr Paul Hancock</h2>
 <p>I am an Early Career Research Fellow currently at Curtin University. I o
 btained my PhD at the University of Sydney, where I worked on the Australia
  Telescope 20GHz (AT20G) survey. I then continued to work as a Super Scienc
 e Fellow in radio transients at USYD where I helped to create the Variable 
 And Slow Transients (VAST) prototype pipeline, including the source finding
  algorithm Aegean. My interests are in radio transients including: supernov
 ae, gamma-ray bursts, and tidal disruption events.</p><p>I lead two project
 s that use the Murchison Wide-field Array (MWA). The first project uses the
  scintillation of extragalactic radio sources to trace the turbulent struct
 ure of gas within the Milky Way. The second project uses the MWA to search 
 for radio emission from fireballs as they burn a path through our atmospher
 e.</p>
DTSTAMP:20260620T200609
DTSTART;TZID=Australia/Sydney:20210603T193000
DTEND;TZID=Australia/Sydney:20210603T213000
SEQUENCE:0
TRANSP:OPAQUE
END:VEVENT
END:VCALENDAR