Japan Geoscience Union Meeting 2021

Presentation information

[E] Oral

P (Space and Planetary Sciences ) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM08] Space Weather and Space Climate

Fri. Jun 4, 2021 3:30 PM - 5:00 PM Ch.06 (Zoom Room 06)

convener:Ryuho Kataoka(National Institute of Polar Research), A Antti Pulkkinen(NASA Goddard Space Flight Center), Kanya Kusano(Institute for Space-Earth Environmental Research, Nagoya University), Kaori Sakaguchi(National Institute of Information and Communications Technology), Chairperson:Antti A Pulkkinen(NASA Goddard Space Flight Center), Ryuho Kataoka(National Institute of Polar Research)

3:45 PM - 4:00 PM

[PEM08-08] Relativistic Electron Precipitation Detections with CALET on the International Space Station

*Alessandro Bruno1,2, Georgia A. de Nolfo2, Anthony W. Ficklin3, T. Gregory Guzik3, Lauren Blum4 (1.Department of Physics, Catholic University of America, Washington, DC, USA, 2.Heliophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, MD,, 3.Department of Physics and Astronomy, Louisiana State University, Baton Rouge, LA, USA, 4.University of Colorado, Boulder, CO, USA)

Keywords:Relativic Electron Precipitation, Space Weather, Cosmic Rays, Spacecraft Measurements

The CALorimetric Electron Telescope (CALET) is a high-energy astroparticle experiment installed on the International Space Station and operating since October 2015. While conceived for the investigation of the origin and the propagation of galactic cosmic-rays, CALET has been also providing a continuous monitoring of space weather phenomena in the near-Earth environment, including solar energetic particle and relativistic electron precipitation (REP) events. In particular, the low-Earth orbit detections from CALET complement the equatorial observations made by other spacecraft at higher altitudes, such as the twin Van Allen Probes, enabling a more complete picture of energetic electron precipitation and its contribution to the radiation belt dynamics. In this work we present the preliminary results obtained over a four-year (2015-2019) acquisition time.