Haleakalā Neutron Monitor Workshop and Ribbon Cutting Ceremony

Session

Physics / Space Weather, Data Analysis, and Results

6 Jan 2025, 14:20

11. Space Weather Monitoring with the Neutron Monitor Network

Pierre-Simon Mangeard

06/01/2025, 14:20

12. The Neutron Monitor of Mexico City as a tool for Space Weather Analysis

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.

13. Investigating Cosmic Ray Variation with Semi-Leaded Neutron Monitors and Polar Surveys

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...

14. CMU-ESE Research Activities on Space Weather and Cosmic Rays and its impact

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...

15. Ionospheric and Magnetospheric Responses to Space Weather

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...

17. Low-Latitude Neutron Monitor Science: Solar Neutrons and Galactic Cosmic Rays at High Cutoff Rigidity

David Ruffolo (U Mahidol)

06/01/2025, 16:15

27. Real-time NM leader fractions

Alejandro Sáiz (U Mahidol)

06/01/2025, 16:40

20. Neutron Monitor yield functions: applications and perspectives

Alexander Mishev (OULU)

07/01/2025, 09:40

21. Calibrating NM on Ground with AMS in Space

Cristina Consolandi (UH Manoa)

07/01/2025, 09:55

22. Investigation of Neutron Monitor Response to Cosmic Ray Air Showers.

Chloe Heifner (UDEL)

07/01/2025, 10:45

30. Unusually long scattering mean-free path of suprathermal ions in the turbulent interplanetary magnetic field

Joe Giacalone (University of Arizona)

07/01/2025, 11:15

31. Transport of GV Rigidity Solar Energetic Particles in Turbulent and Non-turbulent Interplanetary Magnetic Field and SEP profiles at 1 AU

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),...