EGU24-4775, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-4775
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

First results from the radiation belt monitors onboard the 6U CubeSat X-Ray Observatory NinjaSat

Yo Kato1 and the NinjaSat Team*
Yo Kato and the NinjaSat Team
  • 1RIKEN, Saitama, Japan (yo.kato.jw@riken.jp)
  • *A full list of authors appears at the end of the abstract

NinjaSat, a 6U CubeSat-sized (30 cm x 20 cm x 10 cm) X-ray observation satellite, was launched into a low Earth orbit at an altitude of 550 km in November 2023. NinjaSat is equipped with two 1U CubeSat-sized (10 cm x 10 cm x 10 cm) gas X-ray detectors (GMC) as primary detectors for astronomical observations of bright X-ray sources such as neutron stars and black holes. Initial operations of NinjaSat have been underway since January 2024.

NinjaSat is also equipped with two radiation belt monitors (RBM) as sub-detectors to protect the GMCs from discharges in the gas cells potentially caused by excessive amount of incident charged particles. NinjaSat RBM uses a 9 mm x 9 mm Si-PIN photodiode to detect any increase in the count rate of either protons or electrons by exploiting the difference in the sensor's response to protons and electrons, and sends alert signals to GMCs which help ramping down high voltage applied to gas cells in the region of high charged particle rates. NinjaSat RBM is approximately 6% of the size of a 1U CubeSat in volume and weighs only 70 grams. Because NinjaSat RBM uses inexpensive, commercially available sensors and operates on an internal board independent of the primary detectors, it can be installed on other small satellites which need to monitor surrounding charged particle environment with relatively few development resources.

Since NinjaSat will operate in a sun-synchronous orbit, a global map of charged particles can be obtained. We will present the development of NinjaSat RBM and the first results of charged particle maps in the radiation belt obtained during the initial operational period of NinjaSat.

NinjaSat Team:

Toru Tamagawa (RIKEN), Teruaki Enoto (Kyoto University), Takao Kitaguchi (RIKEN), Tatehiro Mihara (RIKEN), Wataru Iwakiri (Chiba University), Masaki Numazawa (Tokyo Metropolitan University), Tomoshi Takeda (Tokyo University of Science), Yuto Yoshida (Tokyo University of Science), Naoyuki Ota (Tokyo University of Science), Syoki Hayashi (Tokyo University of Science), Sota Watanabe (Tokyo University of Science), Arata Jujo (Tokyo University of Science), Amira Aoyama (Tokyo University of Science), Satoko Iwata (Tokyo University of Science), Yuanhui Zhou (Tokyo University of Science), Keisuke Uchiyama (Tokyo University of Science), Hiroki Sato (Shibaura Institute of Technology), Kentaro Taniguchi (RIKEN), Chin-ping Hu (National Changhua University of Education), Hiromitsu Takahashi (Hiroshima University), Hirokazu Odaka (Osaka University), Tsubasa Tamba (ISAS/JAXA)

How to cite: Kato, Y. and the NinjaSat Team: First results from the radiation belt monitors onboard the 6U CubeSat X-Ray Observatory NinjaSat, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-4775, https://doi.org/10.5194/egusphere-egu24-4775, 2024.