• 한국자기학회지
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• 제8권1호
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• pp.21-26
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• 1998

온도에 따른 비정질 금속 Co66Fe4Ni1B14Si15의 자기 임피던스의 변화를 저온 장치를 써서 시료의 온도를 10K∼300K까지 변화시키면서 측정하였다. 이때, 시료에 겉어준 교류전류를 10mA로 고정시키고 주파수를 100KHz에서 10MHz 까지 변화시켰다. MIR (Magneto-Impedance Ratio)은 온도가 증가함에 따라 급격히 증가하였으며, MIR(T)≡MIR(0)exp(cT2)의 관계식으로 나타났다. 상온에서 측정한 MIR 값은 측정 주파수내에서 10K에서의 값보다 2∼3배 크게 나타났다. 이 결과는 MI 온도 효과를 이용한 온도 센서로서의 가능성을 제시한다. MIR 곡선의 모양은 온도의 증가에 따라 큰 변화가 없었으며 MIR은 주파수 증가에 따라 커지면서 MIR 곡선의 모양이 퍼지는 전형적인 경향을 나타냈다.

• Journal of Astronomy and Space Sciences
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• 제37권1호
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• pp.19-27
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• 2020

Pc1 pulsations are important to consider for the interpretation of wave-particle interactions in the Earth's magnetosphere. In fact, the wave properties of these pulsations change dynamically when they propagate from the source region in the space to the ground. A detailed study of the wave features can help understanding their time evolution mechanisms. In this study, we statistically analyzed Pc1 pulsations observed by a Bohyunsan (BOH) magneto-impedance (MI) sensor located in Korea (L = 1.3) for ~one solar cycle (November 2009-August 2018). In particular, we investigated the temporal occurrence ratio of Pc1 pulsations (considering seasonal, diurnal, and annual variations in the solar cycle), their wave properties (e.g., duration, peak frequency, and bandwidth), and their relationship with geomagnetic activities by considering the Kp and Dst indices in correspondence of the Pc1 pulsation events. We found that the Pc1 waves frequently occurred in March in the dawn (1-3 magnetic local time (MLT)) sector, during the declining phase of the solar cycle. They generally continued for 2-5 minutes, reaching a peak frequency of ~0.9 Hz. Finally, most of the pulsations have strong dependence on the geomagnetic storm and observed during the early recovery phase of the geomagnetic storm.