日本地球惑星科学連合2019年大会

講演情報

[J] ポスター発表

セッション記号 S (固体地球科学) » S-EM 固体地球電磁気学

[S-EM18] 地磁気・古地磁気・岩石磁気

2019年5月26日(日) 17:15 〜 18:30 ポスター会場 (幕張メッセ国際展示場 8ホール)

コンビーナ:清水 久芳(東京大学地震研究所)、佐藤 雅彦(東京大学地球惑星科学専攻学専攻)

[SEM18-P15] 超伝導量子干渉素子(SQUID)顕微鏡の感度および実用性の改良

*久保田 勇祐1Kirschvink Joseph2,1Isaac Hilburn2Jennifer Buz3小林 厚子1,2加藤 千恵4 (1.東京工業大学、2.California Institute of Technology、3.Northern Arizona University、4.九州大学)

キーワード:SQUID顕微鏡、岩石磁気学

Superconducting quantum interference device (SQUID) microscopes have been used for mapping the distribution of ferromagnetic materials in a variety of industrial, biological, and geological materials. The advantage of the SQUID microscope is the wide dynamic range and spatial resolution down to the 25 μm scale, as well as the ability to quantify the direction and intensity of extraordinarily tiny magnetic dipoles. However, a major drawback of earlier versions of this instrument has been the need to cool the superconducting sensors with liquid helium and nitrogen, which limits the system’s utility and drives up maintenance costs. One previous instrument (at Caltech) incorporated a closed-cycle pulse-tube cryocooler and managed to achieve good sensitivity by averaging precisely over one pulse cycle to remove the periodic magnetic signal from the pulse tube ferrite chain. In this study, we report a new design of SQUID microscope at TokyoTech that improves substantially on this. First, a large-volume μ-metal shielded room provides an environment with low spatial magnetic gradients, although it does allow ~ 5 nT low-frequency signals from local train lines to penetrate. Next, the pulse-tube is encased in a superconducting shield made of Pb, lowering the noise from that source. Finally, we placed a second SQUID sensor, parallel to the axis, ~4 cm from the first and calibrated it to correct for background fluctuations. The final system is approximately 5-10 times more sensitive than the previous configuration and is being applied to a variety of biological and single-crystal rock magnetic studies.