BEGIN:VCALENDAR VERSION:2.0 PRODID:-//jEvents 2.0 for Joomla//EN CALSCALE:GREGORIAN METHOD:PUBLISH BEGIN:VTIMEZONE TZID:Australia/Sydney BEGIN:STANDARD DTSTART:20140701T193000 RDATE:20141005T030000 TZOFFSETFROM:+1100 TZOFFSETTO:+1000 TZNAME:Australia/Sydney AEST END:STANDARD BEGIN:STANDARD DTSTART:20150405T020000 RDATE:20151004T030000 TZOFFSETFROM:+1100 TZOFFSETTO:+1000 TZNAME:Australia/Sydney AEST END:STANDARD BEGIN:STANDARD DTSTART:20160403T020000 RDATE:20161002T030000 TZOFFSETFROM:+1100 TZOFFSETTO:+1000 TZNAME:Australia/Sydney AEST END:STANDARD BEGIN:STANDARD DTSTART:20170402T020000 RDATE:20171001T030000 TZOFFSETFROM:+1100 TZOFFSETTO:+1000 TZNAME:Australia/Sydney AEST END:STANDARD BEGIN:STANDARD DTSTART:20180401T020000 RDATE:20181007T030000 TZOFFSETFROM:+1100 TZOFFSETTO:+1000 TZNAME:Australia/Sydney AEST END:STANDARD BEGIN:STANDARD DTSTART:20190407T020000 RDATE:20191006T030000 TZOFFSETFROM:+1100 TZOFFSETTO:+1000 TZNAME:Australia/Sydney AEST END:STANDARD BEGIN:STANDARD DTSTART:20200405T020000 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:20141005T030000 RDATE:20150405T020000 TZOFFSETFROM:+1000 TZOFFSETTO:+1100 TZNAME:Australia/Sydney AEDT END:DAYLIGHT BEGIN:DAYLIGHT DTSTART:20151004T030000 RDATE:20160403T020000 TZOFFSETFROM:+1000 TZOFFSETTO:+1100 TZNAME:Australia/Sydney AEDT END:DAYLIGHT BEGIN:DAYLIGHT DTSTART:20161002T030000 RDATE:20170402T020000 TZOFFSETFROM:+1000 TZOFFSETTO:+1100 TZNAME:Australia/Sydney AEDT END:DAYLIGHT BEGIN:DAYLIGHT DTSTART:20171001T030000 RDATE:20180401T020000 TZOFFSETFROM:+1000 TZOFFSETTO:+1100 TZNAME:Australia/Sydney AEDT END:DAYLIGHT BEGIN:DAYLIGHT DTSTART:20181007T030000 RDATE:20190407T020000 TZOFFSETFROM:+1000 TZOFFSETTO:+1100 TZNAME:Australia/Sydney AEDT END:DAYLIGHT BEGIN:DAYLIGHT DTSTART:20191006T030000 RDATE:20200405T020000 TZOFFSETFROM:+1000 TZOFFSETTO:+1100 TZNAME:Australia/Sydney AEDT END:DAYLIGHT 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:b702e3502e1f555e716cd646db1c8adb CATEGORIES:Guest Speaker Night CREATED:20150531T070158 SUMMARY:Guest Speaker - Dr Gail Iles - Bragg Institute, ANSTO DESCRIPTION:

Science in Space: Reality vs Fiction

Here I share my own experie nces of conducting science in microgravity, training the next generation of astronauts, and the similarities to every-day life onboard the Internation al Space Station with those depicted in film.  I shall also describe some t ypical scientific experiments conducted in space, and the process followed to fly your experiment in reduced gravity conditions. 

Using the Fren ch Zero-G airbus, we have performed condensed matter experiments in 2G and microgravity to investigate the agglomeration of intermetallic melts.  We d iscovered that without the earth-based forces of gravity and convective hea t flows we were able to grow unique nanoparticulate structures, impossible to fabricate in earth-based laboratories.

Recently, Hollywood has tre ated us to two modern-day blockbuster movies set in space: Gravity, starrin g Sandra Bullock and Interstellar starring Matthew McConaughey.  The films are exciting and tackle Newtonian physics in the special effects, but are t he orbital mechanics and relativity accurate?  After this seminar – y ou can decide!

About Dr Iles

Dr Gail IlesRole at ANSTO

Dr Gail Iles is an instrument scientist responsible for EMU, the co ld neutron backscattering spectrometer, in the Bragg Institute.  Her ex pertise in neutron scattering has been demonstrated through characterisatio n measurements at neutron sources around the world, and in neutron instrume ntation.

Gail was instrument scientist of FALCON, the neutron Laue diffractometer at HZB in Berlin, Germany, re sponsible for the design, construction and commissioning of this new instru ment.  Previously, Gail also spent a short time as instrument scientist on the high-flux powder diffractometer, D20 at the ILL i n Grenoble, France. Gail’s research interests are in the field of rar e earth magnetism.  The very high resolution of EMU will be ideal for inves tigating hyperfine energy fields which typically occur at just a few µeV.   A number of rare earth atoms have been shown to undergo hyperfine splitting which can be observed as the interaction between the spins of the incoming neutron and the sample nuclei.  Studies of nuclear magnetism will help us better understand the mechanisms of high-temperature superconductivity, for example.

Qualifications and Achievements

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Science in Space: Reality vs Fiction

Here I share my own experie nces of conducting science in microgravity, training the next generation of astronauts, and the similarities to every-day life onboard the Internation al Space Station with those depicted in film.  I shall also describe some t ypical scientific experiments conducted in space, and the process followed to fly your experiment in reduced gravity conditions. 

Using the Fren ch Zero-G airbus, we have performed condensed matter experiments in 2G and microgravity to investigate the agglomeration of intermetallic melts.  We d iscovered that without the earth-based forces of gravity and convective hea t flows we were able to grow unique nanoparticulate structures, impossible to fabricate in earth-based laboratories.

Recently, Hollywood has tre ated us to two modern-day blockbuster movies set in space: Gravity, starrin g Sandra Bullock and Interstellar starring Matthew McConaughey.  The films are exciting and tackle Newtonian physics in the special effects, but are t he orbital mechanics and relativity accurate?  After this seminar – y ou can decide!

About Dr Iles

Dr Gail IlesRole at ANSTO

Dr Gail Iles is an instrument scientist responsible for EMU, the cold neutron backscattering spectrometer, in the Bragg Institute.  Her expertise in neutron scattering has been demonstrated through characterisation measurements at neutron sources around the world, and in neutron instrumentation.

Gail was instrument scientist of FALCON, the neutron Laue diffractometer at HZ B in Berlin, Germany, responsible for the design, construction and commissi oning of this new instrument.  Previously, Gail also spent a short time as instrument scientist on the high-flux powder diffractomet er, D20 at the ILL in Grenoble, France. Gail’s research interests are in the field of rare earth magnetism.  The very high resolution of EMU will be ideal for investigating hyperfine energy fields which typically oc cur at just a few µeV.  A number of rare earth atoms have been shown to und ergo hyperfine splitting which can be observed as the interaction between t he spins of the incoming neutron and the sample nuclei.  Studies of nuclear magnetism will help us better understand the mechanisms of high-temperatur e superconductivity, for example.

Qualifications and Achievements DTSTAMP:20260906T193344 DTSTART;TZID=Australia/Sydney:20150702T193000 DTEND;TZID=Australia/Sydney:20150702T213000 SEQUENCE:0 TRANSP:OPAQUE END:VEVENT END:VCALENDAR