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DTSTART:16011028T020000
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BEGIN:VEVENT
ATTENDEE;CN="ESC F51 Meeting Room (max 8) RESTRICTED";CUTYPE=RESOURCE;ROLE=
	NON-PARTICIPANT;RSVP=TRUE:mailto:ESCF51MEETINGROOM@stfc.ac.uk
ATTENDEE;CN=tomographic.imaging@gmail.com;RSVP=TRUE:mailto:tomographic.imag
	ing@gmail.com
CLASS:PUBLIC
CREATED:20260724T085619Z
DESCRIPTION:3-4pm BST:\n\n               gVXR Release v2.1.0 - Prof. Franck
	 Vidal\n\n \n\nCheck: https://ccpi.ac.uk/events/ccpi-show-tell-and-user-su
	pport-drop-in/ for the upcoming schedule.\n\n \n\n4-4:30pm BST user suppor
	t drop in\n\n \n\n \n\nFranck’s talk will be covering what’s new in th
	e latest release of gVXR:\n\nThis release builds on 2.0.10 with improvemen
	ts in performance\, usability\, and simulation fidelity.\n\n🔧 Key Upd
	ates\n\n⚡ Mixed-Precision Support\n\n*	Introduction and refinement of mi
	xed‑precision computation\n*	Enables faster simulations by combining hal
	f (16 bits) and single (32 bits) precision on GPU where appropriate\n*	Mai
	ntains numerical accuracy while improving GPU performance\n\n✅ Enhanced 
	Python Integration\n\n*	Improved PyPI packaging and cross-platform distrib
	ution\n*	New digital twin framework to simplify setting up scans for speci
	fic devices\n*	Integration with Numpy to speed up the computeXRayImage and
	 makeIsoSurface functions\n\n🧪 Feature Refinements\n\n*	Flux can now 
	be set as a number of photons per cm2 at one metre\, seamlessly applying t
	he inverse square law when the source-detector distance is changes\n*	Avai
	lability of an OpenMP backend on CPU when a GPU is not available\n*	Comput
	ation of the peak signal-noise ratio (PSNR) when noise is enabled\n*	Gener
	ation of iso-surfaces using the Marching Cubes algorithm to create meshes 
	from 2D images or 3D volumes\n*	Integration of XrayPhysics to generate X-r
	ay tube spectra without any Python dependency\n*	Possibility to automatica
	lly maximise the magnification\n*	More consistent behaviour across API fun
	ctions\n*	Continued maturation of the simulation engine\n\n🐞 Bug Fixe
	s\n\n*	Resolution of issues from previous 2.0.x releases\n*	Improved cross
	-platform compatibility\n*	Fixes for edge cases affecting reproducibility 
	and stability\n\n👉 Full changelog:\nhttps://sourceforge.net/p/gvirtua
	lxray/gitroot/ci/master/tree/CHANGELOG\n\n \n\n \n\n
DTEND;TZID="GMT Standard Time":20260728T163000
DTSTAMP:20260724T085351Z
DTSTART;TZID="GMT Standard Time":20260728T150000
LAST-MODIFIED:20260724T085619Z
LOCATION:ESC F51 Meeting Room (max 8) RESTRICTED\; https://teams.microsoft.
	com/l/meetup-join/19%3ameeting_MWQ5YjRmODItN2Y5YS00N2JiLWJhOTMtZDMwODQxOTM
	zYmEx%40thread.v2/0?context=%7b%22Tid%22%3a%223f66361c-a87e-4158-8f61-99e8
	2db3cac8%22%2c%22Oid%22%3a%2276e00762-ea1c
ORGANIZER;CN="Murgatroyd, Laura (STFC,RAL,SC)":mailto:laura.murgatroyd@stfc
	.ac.uk
PRIORITY:5
SEQUENCE:0
SUMMARY;LANGUAGE=en-gb:CCPi Show & Tell: gVXR Release v2.1.0 - Prof. Franck
	 Vidal\, followed by User Support Drop-in at 4pm
TRANSP:OPAQUE
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	rd-wrap:break-word'><div class=WordSection1><p class=MsoNormal>3-4pm BST:<
	o:p></o:p></p><p class=MsoNormal>               gVXR Release
	 v2.1.0 - Prof. Franck Vidal<o:p></o:p></p><p style='margin:0cm'><span sty
	le='font-family:"Aptos Display"\,sans-serif\;color:black'><o:p>&nbsp\;</o:
	p></span></p><p style='margin:0cm'><span style='font-family:"Aptos Display
	"\,sans-serif\;color:black'>Check: </span><u><span style='font-family:"Apt
	os Display"\,sans-serif\;color:#467886'><a href="https://ccpi.ac.uk/events
	/ccpi-show-tell-and-user-support-drop-in/" target="_blank">https://ccpi.ac
	.uk/events/ccpi-show-tell-and-user-support-drop-in/</a></span></u><span st
	yle='font-family:"Aptos Display"\,sans-serif\;color:black'>&nbsp\;for the 
	upcoming schedule.</span><span style='font-family:"Gulim"\,sans-serif'><o:
	p></o:p></span></p><p style='margin:0cm'><span style='font-family:"Aptos D
	isplay"\,sans-serif\;color:black'>&nbsp\;</span><span style='font-family:"
	Gulim"\,sans-serif'><o:p></o:p></span></p><p style='margin:0cm'><span styl
	e='font-family:"Aptos Display"\,sans-serif\;color:black'>4-4:30pm BST user
	 support drop in<o:p></o:p></span></p><p style='margin:0cm'><span style='f
	ont-family:"Aptos Display"\,sans-serif\;color:black'><o:p>&nbsp\;</o:p></s
	pan></p><p style='margin:0cm'><span style='color:black'><o:p>&nbsp\;</o:p>
	</span></p><p style='margin:0cm'>Franck’s talk will be covering what’s
	 new in the latest release of gVXR:<o:p></o:p></p><p>This release builds o
	n <b>2.0.10</b> with improvements in performance\, usability\, and simulat
	ion fidelity.<o:p></o:p></p><p><b><span style='font-family:"Segoe UI Emoji
	"\,sans-serif'>&#128295\;</span></b><b> Key Updates<o:p></o:p></b></p><p><
	b><span style='font-family:"Segoe UI Emoji"\,sans-serif'>⚡</span></b><b>
	 Mixed-Precision Support<o:p></o:p></b></p><ul type=disc><li style='mso-li
	st:l2 level1 lfo1'>Introduction and refinement of <b>mixed‑precision com
	putation</b><o:p></o:p></li><li style='mso-list:l2 level1 lfo1'>Enables fa
	ster simulations by combining half (16 bits) and single (32 bits) precisio
	n on GPU where appropriate<o:p></o:p></li><li style='mso-list:l2 level1 lf
	o1'>Maintains numerical accuracy while improving GPU performance<o:p></o:p
	></li></ul><p><b><span style='font-family:"Segoe UI Emoji"\,sans-serif'>
	✅</span></b><b> Enhanced Python Integration<o:p></o:p></b></p><ul type=d
	isc><li style='mso-list:l1 level1 lfo2'>Improved PyPI packaging and cross-
	platform distribution<o:p></o:p></li><li style='mso-list:l1 level1 lfo2'>N
	ew digital twin framework to simplify setting up scans for specific device
	s<o:p></o:p></li><li style='mso-list:l1 level1 lfo2'>Integration with Nump
	y to speed up the computeXRayImage and makeIsoSurface functions<o:p></o:p>
	</li></ul><p><b><span style='font-family:"Segoe UI Emoji"\,sans-serif'>&#1
	29514\;</span></b><b> Feature Refinements<o:p></o:p></b></p><ul type=disc>
	<li style='mso-list:l3 level1 lfo3'>Flux can now be set as a number of pho
	tons per cm<sup>2</sup> at one metre\, seamlessly applying the inverse squ
	are law when the source-detector distance is changes<o:p></o:p></li><li st
	yle='mso-list:l3 level1 lfo3'>Availability of an OpenMP backend on CPU whe
	n a GPU is not available<o:p></o:p></li><li style='mso-list:l3 level1 lfo3
	'>Computation of the peak signal-noise ratio (PSNR) when noise is enabled<
	o:p></o:p></li><li style='mso-list:l3 level1 lfo3'>Generation of iso-surfa
	ces using the Marching Cubes algorithm to create meshes from 2D images or 
	3D volumes<o:p></o:p></li><li style='mso-list:l3 level1 lfo3'>Integration 
	of XrayPhysics to generate X-ray tube spectra without any Python dependenc
	y<o:p></o:p></li><li style='mso-list:l3 level1 lfo3'>Possibility to automa
	tically maximise the magnification<o:p></o:p></li><li style='mso-list:l3 l
	evel1 lfo3'>More consistent behaviour across API functions<o:p></o:p></li>
	<li style='mso-list:l3 level1 lfo3'>Continued maturation of the simulation
	 engine<o:p></o:p></li></ul><p><b><span style='font-family:"Segoe UI Emoji
	"\,sans-serif'>&#128030\;</span></b><b> Bug Fixes<o:p></o:p></b></p><ul ty
	pe=disc><li style='mso-list:l0 level1 lfo4'>Resolution of issues from prev
	ious 2.0.x releases<o:p></o:p></li><li style='mso-list:l0 level1 lfo4'>Imp
	roved cross-platform compatibility<o:p></o:p></li><li style='mso-list:l0 l
	evel1 lfo4'>Fixes for edge cases affecting reproducibility and stability<o
	:p></o:p></li></ul><p><span style='font-family:"Segoe UI Emoji"\,sans-seri
	f'>&#128073\;</span> Full changelog:<br><a href="https://sourceforge.net/p
	/gvirtualxray/gitroot/ci/master/tree/CHANGELOG">https://sourceforge.net/p/
	gvirtualxray/gitroot/ci/master/tree/CHANGELOG</a><o:p></o:p></p><p style='
	margin:0cm'><o:p>&nbsp\;</o:p></p><p class=MsoNormal><o:p>&nbsp\;</o:p></p
	></div></body></html>
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