First Results From REPTile‐2 Measurements Onboard CIRBE

Author:

Li Xinlin12ORCID,Selesnick Richard3ORCID,Mei Yang12ORCID,O’Brien Declan12ORCID,Hogan Benjamin12ORCID,Xiang Zheng1,Khoo Lengying4ORCID,Zhao Hong5ORCID,Schiller Quintin6ORCID,Temerin Michael7,Baker Daniel N.1ORCID

Affiliation:

1. Laboratory for Atmospheric and Space Physics University of Colorado Boulder Boulder CO USA

2. Department of Aerospace Engineering Sciences University of Colorado Boulder Boulder CO USA

3. Space Vehicles Directorate Air Force Research Laboratory Kirtland AFB NM USA

4. Department of Astrophysical Sciences Princeton University Princeton NJ USA

5. Department of Physics Auburn University Auburn AL USA

6. Space Science Institute Boulder CO USA

7. Retired from Space Sciences Laboratory University of California, Berkeley Berkeley CA USA

Abstract

AbstractCIRBE (Colorado Inner Radiation Belt Experiment), a 3U CubeSat, was launched on 15 April 2023 into a sun synchronous orbit (97.4° inclination and 509 km altitude). The sole science payload onboard is REPTile‐2 (Relativistic Electron and Proton Telescope integrated little experiment—2), an advanced version of REPTile which operated in space between 2012 and 2014. REPTile‐2 has 60 channels for electrons (0.25–6 MeV) and 60 channels for protons (6.5–100 MeV). It has been working well, capturing detailed dynamics of the radiation belt electrons, including several orders of magnitude enhancements of the outer belt electrons after an intense magnetic storm, multiple “wisps”‐ an electron precipitation phenomenon associated with human‐made very low frequency (VLF) waves in the inner belt, and “drift echoes” of 0.25–1.4 MeV electrons across the entire inner belt and part of the outer belt. These new observations provide opportunities to test the understanding of the physical mechanisms responsible for these features.

Funder

Heliophysics Division

National Science Foundation

Publisher

American Geophysical Union (AGU)

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