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Properties of Forbush decreases of electrons and positrons revealed by the Dark Matter Particle Explorer

Not scheduled
20m
Poster 中微子物理、粒子天体物理与宇宙学

Speaker

wenhao li (purple mountain observatory)

Description

The Forbush Decrease (FD) is a rapid decline in the observed intensity of galactic cosmic rays following intense solar activity, such as a coronal mass ejection (CME). This phenomenon occurs due to fast solar wind sweeping away cosmic rays propagating in the space near the Earth. The Dark Matter Particle Explorer (DAMPE) is a satellite-based cosmic ray experiment with high precision in detecting electrons and positrons, providing a unique opportunity to study electron and positron FDs, which have been rarely studied before. In this contribution, we present the results of a study on the properties of electron and positron FDs from 2016 to 2023. WSA-Enlil is a large-scale, physics-based model that predicts solar wind structures and Earth-directed CMEs. Our study offers new insights into the relationship between FD recovery time and observed CME data, as well as the WSA-Enlil simulations.

Primary authors

wenhao li (purple mountain observatory) jingjing zang (CMS/AMS) Qiang Yuan (Purple Mountain Observatory) Dr Chuan Yue (Purple Mountain Observatory)

Presentation materials