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The IMAP Magnetometer

delete2026-05-04
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OA
AI
T
T. S. Horbury *
H
H. L. O’Brien
C
C. Greenaway
A
A. Roberts
A
A. Crabtree
M
M. Tomes
M
M. Facchinelli
M
M. Finlayson
M
M. Bharatia
E
E. Fauchon-Jones
M
M. Tapley
S
S. Pope
D
D. Jones
I
I. Richter
C
C. Russell
N
N. A. Schwadron
M
M. Gkioulidou
D
D. J. McComas
DOI：10.1007/s11214-026-01277-8delete
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摘要

摘要

En 中文
磁力计（MAG）是星际测绘与加速探测器（IMAP）的十种科学仪器之一，它将从日地L1晕轨道进行原位和远程测量。MAG有助于实现IMAP的科学目标，即研究高能粒子的加速和传播，并提供实时空间天气监测数据。该磁力计是一种传统的双传感器磁通门仪器，噪声水平低于10 pT（1 Hz），以每秒2个向量的速度连续进行科学测量，并具有每秒64个向量的爆发模式，每天至少运行8小时。它还提供每4秒一次的实时空间天气监测产品。本文描述了该仪器的需求、设计和性能，包括一种新颖的无损压缩算法。文中展示了数据产品、处理和校准计划。
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期刊

Space Science Reviews 封面图
Space Science Reviews
IF:
7.4
论文数:
4.2K
被引数:
1.8W

机构

A
applied physics laboratory
学者数:
71
论文数: 25
被引数: 0
T
Technical University of Braunschweig
学者数:
71
论文数: 37
被引数: 0
D
Department of Astrophysical Sciences
学者数:
46
论文数: 17
被引数: 0
U
university of new hampshire
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4.2K
论文数: 3.4K
被引数: 8
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imperial college london
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9.9K
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ucla
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1.1K
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Southwest Research Institute
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2.0K
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U
university of oxford
学者数:
9.8W
论文数: 8.6W
被引数: 137
U
University of Lancashire
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424
论文数: 258
被引数: 0
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引用论文

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