Jul 12 – 23, 2021
Europe/Berlin timezone

Time-Delay Measurements from Antarctic Neutron Monitor Stations Indicate Weak Spectral Changes during 27-day Variations

Jul 14, 2021, 6:00 PM
1h 30m


Talk SH | Solar & Heliospheric Discussion


Mr Pradiphat Muangha (Mahidol University)


Using neutron time-delay data from neutron monitors (NMs), we can extract the leader fraction, L, of neutron counts that do not follow a previous neutron count in the same counter tube due to the cosmic ray shower. L is the inverse of the neutron multiplicity and serves as a proxy of the cosmic ray spectral index over the rigidity range of the NM response function. We have outfitted several Antarctic NMs with special electronics to collect neutron time delay distributions. We present a comparative analysis of L during two time periods: 1) during December 2015 to January 2017, for NMs at South Pole (SP), McMurdo (MC), and Jang Bogo (JB), and 2) during February 2020 to February 2021, for NMs at SP, JB, and Mawson (MA). To first order L varies in concert with the count rate C, reflecting unrolling of the Galactic cosmic ray (GCR) spectrum as part of solar modulation during the declining phase of solar cycle 24 and during solar minimum. However, during 27-day variations in C due to high-speed solar wind streams (HSSs) and corotating interaction regions (CIRs), L usually had a very weak variation. Our results indicate weak GeV-range GCR spectral variation due to HSSs and CIRs, relative to the flux variation, in contrast with the strong observed spectral variation due to solar modulation.


neutron monitor; solar modulation; corotating interaction regions; high-speed solar wind streams

Subcategory Experimental Results

Primary author

Mr Pradiphat Muangha (Mahidol University)


Prof. David Ruffolo (Mahidol University) Dr Alejandro Sáiz (Mahidol University) Chanoknan Banglieng (Rajamangala University of Technology Thanyaburi, Thailand) Prof. Paul Evenson (University of Delaware) Prof. Surujhdeo Seunarine (University of Wisconsin) Prof. Suyeon Oh (Department of Earth Science Education, Chonnam National University) Jongil Jung (Department of Astronomy, Space Science and Geology, Chungnam National University) Prof. Marc Duldig (School of Natural Sciences, University of Tasmania) Prof. John Humble (School of Natural Sciences, University of Tasmania)

Presentation materials