日本地球惑星科学連合2016年大会

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セッション記号 S (固体地球科学) » S-TT 計測技術・研究手法

[S-TT52] 空中からの地球計測とモニタリング

2016年5月23日(月) 09:00 〜 10:30 A07 (アパホテル&リゾート 東京ベイ幕張)

コンビーナ:*楠本 成寿(富山大学大学院理工学研究部(理学))、大熊 茂雄(産業技術総合研究所地質情報研究部門)、小山 崇夫(東京大学地震研究所)、光畑 裕司(独立行政法人 産業技術総合研究所)、座長:楠本 成寿(富山大学大学院理工学研究部(理学))、大熊 茂雄(産業技術総合研究所地質情報研究部門)、小山 崇夫(東京大学地震研究所)、光畑 裕司(独立行政法人 産業技術総合研究所)

10:00 〜 10:15

[STT52-05] 空中,海上および深海地磁気3成分測定による青ヶ島の3次元磁化構造調査

松尾 淳1伊勢崎 修弘2、*佐柳 敬造2 (1.OYOインターナショナル株式会社、2.東海大学海洋研究所)

キーワード:地磁気3成分異常、磁化ベクトル、3次元磁化構造、汎用型3成分磁力計、船上3成分磁力計、深海曳航式3成分磁力計

Measurement of magnetic anomaly vectors is absolutely essential to obtain a magnetization structure of the magnetized body. We have developed a new magnetometer for measurement of the vector magnetic field, called High Precision Magnetic survey System (HPMS), which can be used in various situations, for instance, in the air, on the sea surface and in the deep-sea. We have applied the HPMS as Heliborne Three Component Magnetometer (HTCM), Deep-tow Three Component Magnetometer (DTCM) and Shipboard Three Component Magnetometer (STCM) for airborne surveys (2006 and 2009) and marine magnetic surveys (2014) over and around the volcanic island, Aogashima. A helicopter of Nakanihon air service and Tokai University Vessel 'Bousei-Maru' were used for the HTCM surveys and for the STCM and DTCM surveys, respectively. The Aogashima Island is an active volcanic island included in the Izu-Ogasawara volcanic arc. The objectives of this study were to obtain magnetic anomaly vectors on Aogashima volcano by aero-, sea surface and deep-sea magnetic surveys, and to clarify 3 dimensional spaced 3 component magnetization structure of the volcano.
In the HTCM surveys, a towing frame mounted with the HPMS, GPS and wireless LAN devices was towed using a fiber rope below the helicopter. In the DTCM survey, the towing frame mounted with the HPMS, acoustic positioning (SSBL) and acoustic communication devices was towed near the sea bottom using a wire rope. In the STCM survey, the towing frame mounted with the HPMS and GPS devices was fixed on the after-deck of the ship. Three components of the observed geomagnetic field, F = (Hh, Hs, Hv), and gyro data (yaw, pitch, roll) are sampled in 10Hz. SSBL positions are fixed every 10 seconds. F, the vector in ship's coordinate (heading, starboard, vertical) is rotated to the vector in Earth's coordinate (X, Y, Z: north, east, vertical down) using the gyro data. From the rotated vector (X, Y, Z), the IGRF field is subtracted to get three components of a magnetic anomaly (dX, dY, dZ).
3D spaced 3 component magnetizations of the Aogashima volcano are analyzed by solving the linear least square equation for the obtained magnetic anomaly vectors. We tried 4 layer block model which consists of blocks with width of 500m, depth of 500m, and thickness of 250 m, 500 m, 750 m and 1000 m. The total number of the blocks is 2,492. The upper surface of Layer 1 approximates topographic surface. 25,536 data of three components of magnetic anomalies were inputted, and 7,476 data of three components of magnetization of 3D magnetized body were obtained by magnetization inversion with least square method using a dumping factor.
The figure shows three components of magnetization of each layer. Thin contour lines show the topography. The Aogashima Island is located at the center of each map. The shallower layers have complicated magnetization distribution, especially in Layer 1. There are larger magnetization to the north of the island as seen in Layers 1 and 2. The deeper layers such as Layers 3 and 4 have smooth magnetization distribution comparing with Layers 1 and 2. Layers 3 and 4 show the following characteristic distributions: relatively large positive north component of magnetization to the north of the island, contours of east component of that elongated along the ridge, and small downward component of that along the ridge in Layer 3 and under the island in Layer 4.
In conclusion, we have developed the versatile and useful equipment corresponding to a multiplatform that can survey the vector magnetic fields in the air, on the sea surface and in the deep-sea. That enables us to calculate the 3 dimensional and 3 components magnetization. The HPMS should make a contribution for more detailed and reliable magnetic geophysical surveys.