Abstract

The exploration of energization and radiation in geospace (ERG) satellite, nicknamed “Arase,” is the second satellite in a series of small scientific satellites created by the Institute of Space and Astronautical Science of the Japan Aerospace Exploration Agency. It was launched on December 20, 2016, by the Epsilon launch vehicle. The purpose of the ERG project is to investigate how high-energy (over MeV) electrons in the radiation belts surrounding Earth are generated and lost by monitoring the interactions between plasma waves and electrically charged particles. To measure these physical processes in situ, the ERG satellite traverses the heart of the radiation belts. The orbit of the ERG is highly elliptical and varies due to the perturbation force: the apogee altitude is approximately 32,200–32,300 km, and the perigee altitude is 340–440 km. In this study, we introduce the scientific background for this project and four major challenges that need to be addressed to effectively carry out this scientific mission with a small satellite: (1) dealing with harsh environmental conditions in orbit and electromagnetic compatibility issues, (2) spin attitude stabilization and avoiding excitation of the libration by flexible structures, (3) attaining an appropriate balance between the mission requirements and the limited resources of the small satellite, and (4) the adaptation and use of a flexible standardized bus. In this context, we describe the development process and the flight operations for the satellite, which is currently working as designed and obtaining excellent data in its mission.

Highlights

  • In the early days of space exploration, the first US satellite, Explorer 1, discovered the existence of high-energy charged particles in space within close proximity of the Earth using its onboard radiation detector

  • In 2012, after a system definition review (SDR), the energization and radiation in geospace (ERG) satellite was classified as a formal Japan Aerospace Exploration Agency (JAXA) project and proceeded to phase B, the preliminary design phase; at this time, an ERG project team was organized

  • Integrated studies involving the satellite, ground networks, and simulations In order to understand the development of space storms and their effects on the radiation belts, it is necessary to understand the phenomena occurring throughout the geospace region

Read more

Summary

Open Access

Exploration of energization and radiation in geospace (ERG): challenges, development, and operation of satellite systems. Yosuke Nakamura1* , Seisuke Fukuda, Yasuko Shibano, Hiroyuki Ogawa, Shin‐ichiro Sakai, Shigehito Shimizu, Ersin Soken, Yu Miyazawa, Hiroyuki Toyota, Akio Kukita, Yusuke Maru, Junichi Nakatsuka, Tomohiko Sakai, Shinsuke Takeuchi, Kenichiro Maki, Makoto Mita, Emiko Ogawa, Yuya Kakehashi, Kumi Nitta, Kazushi Asamura, Takeshi Takashima and Iku Shinohara

Introduction
ERG project
Bus module
Solar array panels
Plasma wave wire probe antenna
Electrical Power
Challenges in the design of the ERG system
Radiation effects
Libration tests of a wire probe antenna on the ground
Declination Right ascension
Power requirements and weight
Thrusters or no thrusters selectable
Development and flight operations
Commissioning Phase
Science Operations Phase
Sun acquisition complete
Findings
Antenna select change
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call