MAGNETIC-FIELD OBSERVATIONS ON THE AKEBONO (EXOS-D) SATELLITE

被引：53

作者：

FUKUNISHI, H

FUJII, R

KOKUBUN, S

HAYASHI, K

TOHYAMA, T

TONEGAWA, Y

OKANO, S

SUGIURA, M

YUMOTO, K

AOYAMA, I

SAKURAI, T

SAITO, T

IIJIMA, T

NISHIDA, A

NATORI, M

机构：

[1] UNIV TOKYO,GEOPHYS RES LAB,BUNKYO KU,TOKYO 113,JAPAN

[2] NATL INST POLAR RES,ITABASHI KU,TOKYO 113,JAPAN

[3] TOKAI UNIV,FAC ENGN,HIRATSUKA,KANAGAWA 25912,JAPAN

[4] TOKAI UNIV,INST RES & DEV,SHIBUYA KU,TOKYO 151,JAPAN

[5] NAGOYA UNIV,ATMOSPHER RES INST,TOYOKAWA 442,JAPAN

[6] INST SPACE & ASTRONAUT SCI,SAGAMIHARA 229,JAPAN

来源：

JOURNAL OF GEOMAGNETISM AND GEOELECTRICITY | 1990年 / 42卷 / 04期

关键词：

D O I：

10.5636/jgg.42.385

中图分类号：

P [天文学、地球科学];

学科分类号：

07 ;

摘要：

The Akebono (EXOS-D) satellite carries triaxial fluxgate and search coil magnetometers with sensors mounted on 5- and 3-m masts, respectively. The fluxgate magnetometer has four automatically switchable ranges from ±1024 to ±65 536 nT (full scale), and resolutions commensurate with a 16-bit A/D converter in each range (0.031 to 2 nT). The rate of sampling is 32 vectors per second. The triaxial search coil magnetometer has a frequency response up to 800 Hz. Signals in the frequency range higher than 100 Hz are used for VLF plasma wave experiments, while signals less than 100 Hz are used for magnetic field experiments. -from Authors

引用

页码：385 / 409

页数：25

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