Main Image
Volume 358 - 36th International Cosmic Ray Conference (ICRC2019) - CRI - Cosmic Ray Indirect
The Energy Calibration Using the Moon Shadow of LHAASO-WCDA Detector
Y. Wang,* M.Z.Z.C. Xin Zhang
*corresponding author
Full text: pdf
Pre-published on: 2019 July 22
Published on:
Abstract
The shadow of the Moon observed with cosmic rays can be utilized to study the pointing error and the angular resolution of the ground-based air shower arrays, also offers a good ability to do below a few TeV energy calibration based on the bending of cosmic rays when they travel through the geomagnetic field. Water Cherenkov Detector Array (WCDA), one of components of Large High Altitude Air Shower Observation (LHAASO), has high observation sensitivity, lower threshold, and high duty cycle, which make itself a very good facility in this aspect. In this presentation, we study the ability of the westward displacement of the Moon shadow based on
an accurate simulation and experimental data analysis, some systematic uncertainties related with energy calibration are also discussed.
Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.