| Budget Amount *help |
¥17,160,000 (Direct Cost: ¥13,200,000、Indirect Cost: ¥3,960,000)
Fiscal Year 2020: ¥7,410,000 (Direct Cost: ¥5,700,000、Indirect Cost: ¥1,710,000)
Fiscal Year 2019: ¥1,820,000 (Direct Cost: ¥1,400,000、Indirect Cost: ¥420,000)
Fiscal Year 2018: ¥4,940,000 (Direct Cost: ¥3,800,000、Indirect Cost: ¥1,140,000)
Fiscal Year 2017: ¥2,990,000 (Direct Cost: ¥2,300,000、Indirect Cost: ¥690,000)
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| Outline of Final Research Achievements |
We investigated the magnetometer to obtain electron-scale electromagnetic turbulence and shock waves in the solar wind, to study the mechanism of plasma heating due to wave-particle interactions that occur universally in the solar system. We examined the techniques to measure high-time resolution and highly precise waveforms of magnetic field disturbances in the space, and in parallel to drastically reduce the weight and power consumption of the hardware. We applied newly developed techniques to the magnetometer test model, which would be useful also for future small spacecraft missions where the weight and power resources would be strictly limited.
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