14–24 Jul 2025
CICG - International Conference Centre - Geneva, Switzerland
Europe/Zurich timezone
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Study of secondary cosmic ray variations during extreme space weather event on May 10-11, 2024

Not scheduled
20m
Levels -1 & 0

Levels -1 & 0

Poster Cosmic-Ray Indirect PO-1

Speaker

Pranali Thakur (Indian Institute of Geomagnetism, Navi Mumbai)

Description

The Forbush decrease (FD) is a short-term decrease in cosmic ray flux observed during the passage of transient interplanetary disturbances such as interplanetary counterpart of coronal mass ejection (ICME) and Co-rotating interaction regions (CIR). On 8-13 May 2024, multiple ICMEs erupted from active region AR 13664. On May 10, 2024, after the arrival of ICME shock at 17:04 UT, deep FD is seen in various Neutron Monitors (NMs) stations located worldwide. We have done comprehensive analysis of neutron monitor data using high-resolution (2-minute) from 28 NM stations, along with gamma-ray flux data at Maitri, Antarctica, using a NaI (Tl) detector. Enhancement in neutron flux before FD commencement is noticed at stations located at higher altitudes (>1000 m) with geomagnetic rigidity 4-7 GV, and the variation of FD amplitude with rigidity shows a decreasing trend in general, with a minimum amplitude near 6-7 GV. During the recovery phase of FD, enhancement is observed between 1:50-3:00 UT on 11 May 2024, which is linked with Ground Level Enhancement (GLE#74). GOES satellite observations confirm the arrival of GLE, associated with an X5.8 solar flare that occurred on May 11 at 1:36 UT. The dependence of pre-FD, FD, and GLE amplitude on the rigidity and elevation height of the NM station will be discussed.

Authors

Mrs Geeta Vichare (Indian Institute of Geomagnetism, Navi Mumbai) Pranali Thakur (Indian Institute of Geomagnetism, Navi Mumbai)

Presentation materials

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