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Veronica Bindi (UH Manoa)06/01/2025, 09:00
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Roman Makarevich06/01/2025, 09:10
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Roald Sagdeev (UMD)06/01/2025, 09:20
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Veronica Bindi (UH Manoa)06/01/2025, 09:40
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Nikolay Nikonov (UH Manoa)06/01/2025, 10:10
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James Ryan (UNH)06/01/2025, 10:45
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Paul Evenson (UDEL)06/01/2025, 11:20
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Andrew Kuhlman (UNH)06/01/2025, 11:50
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Thirasak Panyaphirawat (CMU)06/01/2025, 12:10
Chiang Mai University operates the "Chang Van" mobile neutron detector, a twin model
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of the "Thimon" (Thailand-Hawaii Neutron Monitor). Over the years, we have successfully conducted multiple expeditions aboard icebreaker ships, supported by the Polar Research Institute of China and the Korea Polar Research Institute, to both the Arctic and Antarctic regions as part of the Latitude Survey... -
Jania Newton-Bosch (UNAM)06/01/2025, 13:30
An overview of the Mexico City Cosmic Ray Observatory (MX-CRO), located within University City, UNAM (19°19'47.9"N 99°10'41.6"W) is presented. The MX-CRO includes a 6-NM64 neutron monitor, a muon telescope, a weather station and an electric field monitor. The neutron monitor, its design and electronics, are the main focus of the presentation.
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Michael Aspinall06/01/2025, 13:50
Aspinall M1, Alton T1, Binnersley C3, Bradnam S2, Cazzaniga C4, Croft S1, Frost C4, Joyce M1, Mashao D1, Packer L2, Turner T2, Wild J1
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1 Lancaster University, Lancaster, United Kingdom
2 United Kingdom Atomic Energy Authority, Abingdon, United Kingdom
3 Mirion Technologies (Canberra UK) Limited, Warrington, United Kingdom
4 STFC Rutherford Appleton Laboratory, Harwell Campus, Didcot,... -
Pierre-Simon Mangeard06/01/2025, 14:20
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Franando Monterde-Andrade (UNAM)06/01/2025, 14:50
An overview of the space weather events observed by the Neutron Monitor of Mexico City is presented. The detector is located at the Mexico City Cosmic Ray Observatory (MX-CRO) and it has been operating since 1990. The relevance and scope of its data for space weather analysis is discussed.
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Waraporn Nuntiyakul (CMU)06/01/2025, 15:20
This study presents notable progress in cosmic ray research through both semi-leaded (Changvan) and standard neutron monitor configurations, focusing on the Changvan latitude surveys (2018–2024) and altitude comparisons with the Princess Sirindhorn Neutron Monitor (PSNM). Our findings confirm the spectral crossover pattern in cosmic ray modulation, revealing rigidity-dependent phenomena—drifts...
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Siramas Komonjinda (CMU)06/01/2025, 15:45
Chiang Mai University (CMU) has a longstanding history of astronomical research, beginning with the establishment of the Sirindhorn Observatory in the 1980s. Over the years, CMU has expanded its facilities to include advanced infrastructure for monitoring space weather and cosmic rays, such as the Chang Van neutron monitor and the CMU Space Weather War Room. In 2023, CMU launched the Research...
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Suwicha Wannawichian (CMU)06/01/2025, 16:00
Thailand's awareness about space weather has grown significantly in the past decade. It is now commonly accepted that space weather, the dynamics of particles, and radiation outside the Earth can significantly affect human activities on Earth. We have looked at the ionospheric response using GNSS observations during geomagnetically quiet and disturbed times and disturbances produced by the...
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David Ruffolo (U Mahidol)06/01/2025, 16:15
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Alejandro Sáiz (U Mahidol)06/01/2025, 16:40
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Ilya Usoskin (OULU)07/01/2025, 09:00
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Nicholas Larsen (OULU)07/01/2025, 09:20
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Alexander Mishev (OULU)07/01/2025, 09:40
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Cristina Consolandi (UH Manoa)07/01/2025, 09:55
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Chloe Heifner (UDEL)07/01/2025, 10:45
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Joe Giacalone (University of Arizona)07/01/2025, 11:15
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Ashraf Moradi (University of Arizona)07/01/2025, 11:35
Ground-level enhancement (GLE) is triggered by GV rigidity solar energetic particles (SEPs). In such high energies (a few hundred MeV/n to a few GeV/n), the characteristic of an SEP events differs from the more common low-energy SEPs at 1 au. We present several numerical studies on how the characteristics of an SEP event depend on parameters of the interplanetary magnetic field (IMF),...
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Pierre-Simon Mangeard (UDEL)07/01/2025, 13:30
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Achara Seripienlert (CMU)07/01/2025, 14:00
This study presents Monte Carlo simulations using the FLUKA 4-4 package coupled with
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the DMPJET model to analyze the response of neutron monitors at the Princess
Sirindhorn Neutron Monitor (PSNM) in Thailand, the South Pole Neutron Monitor, and a
mobile semi-leaded neutron monitor (Changvan) during a latitude survey. The
atmospheric and detector simulations accounted for deadtime... -
Michael Aspinall (U Lancaster)07/01/2025, 14:15
Aspinall M1, Alton T1, Binnersley C3, Bradnam S2, Cazzaniga C4, Croft S1, Frost C4, Joyce M1, Mashao D1, Packer L2, Turner T2, Wild J1
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1 Lancaster University, Lancaster, United Kingdom
2 United Kingdom Atomic Energy Authority, Abingdon, United Kingdom
3 Mirion Technologies (Canberra UK) Limited, Warrington, United Kingdom
4 STFC Rutherford Appleton Laboratory, Harwell Campus, Didcot,... -
Pierre-Simon Mangeard (UDEL)07/01/2025, 14:45
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Stephanie de la Torre (UNAM)07/01/2025, 15:20
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Nikolay Nikonov (UH Manoa)
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