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X-ORIGINAL-URL:https://www.atnf.csiro.au
X-WR-CALDESC:Events for Australia Telescope National Facility
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DTSTART;TZID=Australia/Sydney:20251121T080000
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DTSTAMP:20260607T191130
CREATED:20251203T010158Z
LAST-MODIFIED:20251203T010415Z
UID:16319-1763712000-1765904400@www.atnf.csiro.au
SUMMARY:Apply for the 2026APR semester
DESCRIPTION:Overview\n\nWe’re pleased to announce that proposals for ATNF observing time are now open for the 2026APR semester. Grab your chance to use some of our new receivers and facilities. \n\nApply now for: \n\n\nOur ASKAP radio telescope (including CRACO)\n\n\n\nOur Australia Telescope Compact Array\n\n\n\nMurriyang\, our 64-m Parkes radio telescope\n\n\n\nThe Tidbinbilla radio antennas: the 70-m antenna Ballima (DSS-43) \, and the 34-m (DSS-34) antenna;\n\n\n\nThe Long Baseline Array\n\n\nMark your calendars: the deadline for all proposals is 06:00 UT (17:00 Sydney local time) on Tuesday\, 16 December 2025. \n\nTo submit your proposal\, visit our online proposal application system\, OPAL. \nMore information\nOrganiser\n\nEvent details\nDownload iCal\nCategory\nColloquia
URL:https://www.atnf.csiro.au/event/apply-for-the-2026apr-semester/
LOCATION:NSW
ATTACH;FMTTYPE=image/jpeg:https://www.atnf.csiro.au/wp-content/uploads/2024/09/E9A915740-OBERSVERS-6-scaled.jpg
ORGANIZER;CN="George Hobbs":MAILTO:george.hobbs@csiro.au
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DTSTART;TZID=Australia/Sydney:20251126T150000
DTEND;TZID=Australia/Sydney:20251126T160000
DTSTAMP:20260607T191130
CREATED:20251123T222415Z
LAST-MODIFIED:20251123T222416Z
UID:16208-1764169200-1764172800@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Jennifer West (Dominion Radio Astrophysical Observatory)
DESCRIPTION:Is the heliopause seen in radio synchrotron emission?\n\nAbstract: \n\nDiffuse radio synchrotron emission originating in the Milky Way fills the entire sky\, even at high Galactic latitudes. The emission is highly linearly polarised\, and comes from high energy CRs moving in the Galaxy’s magnetic field. Planck has measured the orientation of this emission and has mapped the magnetic field pattern across the sky\, however\, we do not know if the origin of the pattern is distant (tracing the large-scale magnetic field) or nearby (tracing the Local Bubble\, a massive superbubble where our Sun now resides). The reality is the emission must originate at a wide range of distances. In this talk\, I will present evidence that some of this emission has its origin in the interaction between the heliopause and the very local interstellar magnetic field. The emission is polarised\, and traces the local interstellar magnetic field as it wraps around the heliosphere at the heliopause boundary\, which is related to the Sun’s motion through space\, and which has previously been revealed through a bright ribbon of emission detected by NASA’s Interstellar Boundary Explorer (IBEX). \n\nPlease note that the event timezone is AEDT (UTC+11 hrs) \n\n \nJoin Event on Microsoft Teams\nLocation\n\nOrganiser\n\nEvent details\nDownload iCal\nCategory\nColloquia
URL:https://www.atnf.csiro.au/event/sa-colloquium-jennifer-west-dominion-radio-astrophysical-observatory/
LOCATION:Marsfield Lecture Theatre\, 26 Pembroke Road\, Marsfield\, NSW\, 2122\, Australia
CATEGORIES:Colloquia
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ORGANIZER;CN="Jishnu Thekkeppattu":MAILTO:Jishnunambissan.Thekkeppattu@csiro.au
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