BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//Australia Telescope National Facility - ECPv6.16.1//NONSGML v1.0//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
X-WR-CALNAME:Australia Telescope National Facility
X-ORIGINAL-URL:https://www.atnf.csiro.au
X-WR-CALDESC:Events for Australia Telescope National Facility
REFRESH-INTERVAL;VALUE=DURATION:PT1H
X-Robots-Tag:noindex
X-PUBLISHED-TTL:PT1H
BEGIN:VTIMEZONE
TZID:Australia/Sydney
BEGIN:STANDARD
TZOFFSETFROM:+1100
TZOFFSETTO:+1000
TZNAME:AEST
DTSTART:20250405T160000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+1000
TZOFFSETTO:+1100
TZNAME:AEDT
DTSTART:20251004T160000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+1100
TZOFFSETTO:+1000
TZNAME:AEST
DTSTART:20260404T160000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+1000
TZOFFSETTO:+1100
TZNAME:AEDT
DTSTART:20261003T160000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+1100
TZOFFSETTO:+1000
TZNAME:AEST
DTSTART:20270403T160000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+1000
TZOFFSETTO:+1100
TZNAME:AEDT
DTSTART:20271002T160000
END:DAYLIGHT
END:VTIMEZONE
BEGIN:VTIMEZONE
TZID:Australia/Perth
BEGIN:STANDARD
TZOFFSETFROM:+0800
TZOFFSETTO:+0800
TZNAME:AWST
DTSTART:20250101T000000
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20260505T093000
DTEND;TZID=Australia/Sydney:20260507T170000
DTSTAMP:20260513T145302
CREATED:20260217T120640Z
LAST-MODIFIED:20260504T045830Z
UID:17182-1777973400-1778173200@www.atnf.csiro.au
SUMMARY:Australasian "Orange" Pulsar Workshop 2026
DESCRIPTION:Overview\n\nThe Australasian “Orange” Pulsar Meeting is a fortnightly telecon\, supplemented by occasional in‑person workshops\, for the Australasian pulsar and FRB community that fosters collaboration between theorists\, modellers\, and observers. Following the successful 2022 Orange workshop at CSIRO’s Parkes Radio Observatory\, we are excited to host the next  in‑person meeting at the ATNF Marsfield Headquarters in Sydney from 5–7 May 2026. Online participation will be available for those unable to attend in person. \n\nThe workshop will take place at a time of progress and opportunity in pulsar and time‑domain radio astronomy. New instrumentation and facilities\, including the CryoPAF on Murriyang\, the Phase III upgrade of the MWA\, and the ongoing development of the SKA\, are expanding available discovery spaces. In parallel\, the ATNF is exploring potential future Australian radio astronomy facilities for 2030 and beyond. \n\nThis workshop aims to bring the community together to share recent advances in pulsar and time‑domain science\, discuss emerging scientific opportunities\, and to provide input to future (radio) astronomy strategy. \n\nWorkshop schedule\n\nAustralasian_Orange_Workshop_2026_Sched_v2Download\n\nLocation\n\nOrganiser\n\nScience Organising Committee\n\n\nAndrew Zic (CSIRO)\n\n\n\nManisha Caleb (USyd)\n\n\n\nEmma Carli (Swinburne)\n\n\n\nJoscha Jahns-Schindler (Swinburne)\n\n\n\nBradley Meyers (AusSRC)\n\n\n\nNicholas O’Neill (UMelb)\n\n\n\nRyan Shannon (Swinburne)\n\n\n\nChia Min Tanh (Curtin)\n\n\nEvent details\n\n \nDownload iCal\nCategory\nColloquia
URL:https://www.atnf.csiro.au/event/australasian-orange-pulsar-workshop-2026/
LOCATION:Marsfield Lecture Theatre\, 26 Pembroke Road\, Marsfield\, NSW\, 2122\, Australia
CATEGORIES:Meeting
ATTACH;FMTTYPE=image/jpeg:https://www.atnf.csiro.au/wp-content/uploads/2025/05/ParkesOrionPleiades-scaled-1.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Perth:20260506T120000
DTEND;TZID=Australia/Perth:20260506T130000
DTSTAMP:20260513T145302
CREATED:20260430T030155Z
LAST-MODIFIED:20260430T030300Z
UID:18796-1778068800-1778072400@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Prof Yihua Yan (National Astronomical Observatories\, Chinese Academy of Sciences)
DESCRIPTION:Overview on Chinese Meridian Project – Solar and Heliospheric Radio Studies at Mingantu Observing Station\n\nAbstract: \n\nThe Chinese Meridian Project (CMP) is a Ground‐based Space Environment Monitoring Network which includes the Space Environment Monitoring System. The system adopts a well‐designed monitoring architecture\, known as “One Chain\, Three Networks\, and Four Focuses” to achieve stereoscopic and comprehensive monitoring of the entire solar-terrestrial space. The “One‐Chain” component utilizes optical\, radio\, interplanetary scintillation\, and cosmic ray instruments to cover the causal chain of space weather disturbances from the solar surface to near‐Earth space. For the ionosphere\, middle and upper atmosphere\, and geo-magnetic field\, instruments are deployed along longitudes of 120o and 100oE\, and latitudes of 30o and 40oN\, forming the “Three Networks”. Furthermore\, more powerful monitoring facilities or large‐scale instruments have been deployed in four key regions: the high-latitude polar region\, mid‐latitude region in northern China\, low‐latitude region at Hainan Island\, and the Tibet region. These four regions are crucial for disturbances propagation and evolution\, or possess unique geographical and topographical characteristics. \n\nThe Mingantu Observing Station\, which is located about 400km northwest of Beijing with the wide‐band spectral radioheliographs and the interplanetary scintillation telescopes\, constitutes a key component of CMP for tracking and monitoring solar eruptions from the Sun’s atmosphere into interplanetary space. Here we give an overview on CMP and introduce the progress on solar and heliospheric radio studies at Mingantu Observing Station. \n\nPlease note that the event timezone is AWST (UTC+8 hrs) \n\nLocation\n\nOrganiser\n\n\n \n\n\nEvent details\nDownload iCal\nCategory\nColloquia
URL:https://www.atnf.csiro.au/event/sa-colloquium-prof-yihua-yan-national-astronomical-observatories-chinese-academy-of-sciences/
LOCATION:CSIRO – Kensington\, Australian Resources Research Centre (ARRC)\, 26 Dick Perry Ave\, Kensington\, WA\, 6101\, Australia
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/jpeg:https://www.atnf.csiro.au/wp-content/uploads/2026/04/yihua_yan.jpeg
ORGANIZER;CN="Gemma Anderson":MAILTO:gemma.anderson@csiro.au
END:VEVENT
END:VCALENDAR