心理磁力调查

IF 9.1 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Space Science Reviews Pub Date : 2023-01-01 Epub Date: 2023-03-28 DOI:10.1007/s11214-023-00965-z
Benjamin P Weiss, José M G Merayo, Jodie B Ream, Rona Oran, Peter Brauer, Corey J Cochrane, Kyle Cloutier, Linda T Elkins-Tanton, John L Jørgensen, Clara Maurel, Ryan S Park, Carol A Polanskey, Maria de Soria Santacruz-Pich, Carol A Raymond, Christopher T Russell, Daniel Wenkert, Mark A Wieczorek, Maria T Zuber
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引用次数: 0

摘要

Psyche 磁强计调查的目的是检验小行星 (16) Psyche 是由分化的行星核心形成的这一假设。为此,Psyche 磁强计将测量小行星周围的磁场,寻找剩磁的证据。对陨石的古地磁测量和动力理论表明,多种多样的类星体曾经在其金属内核中产生过动力磁场。同样,在 Psyche 发现强磁矩(> 2 × 10 14 Am 2)很可能表明该天体曾经产生过内核动力磁场,这意味着它是由火成岩分异形成的。Psyche 磁强计由两个三轴磁通门传感器单元(SU)组成,沿 2.15 米长的吊杆相距 0.7 米,与航天器总线上的两个电子单元(EU)相连。磁强计的采样频率高达 50 赫兹,量程为 ± 80 , 000 nT,仪器噪声为 39 pT 轴 - 1 3 σ,综合频率为 0.1 至 1 赫兹。两对 SU 和 EU 提供了冗余,使梯度测量能够抑制来自飞行系统磁场的噪声。磁强计将在发射后不久接通电源,并在整个飞行任务期间获取数据。地面数据系统处理磁强计的测量结果,以获得 Psyche 偶极矩的估计值。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

The Psyche Magnetometry Investigation.

The Psyche Magnetometry Investigation.

The Psyche Magnetometry Investigation.

The Psyche Magnetometry Investigation.

The objective of the Psyche Magnetometry Investigation is to test the hypothesis that asteroid (16) Psyche formed from the core of a differentiated planetesimal. To address this, the Psyche Magnetometer will measure the magnetic field around the asteroid to search for evidence of remanent magnetization. Paleomagnetic measurements of meteorites and dynamo theory indicate that a diversity of planetesimals once generated dynamo magnetic fields in their metallic cores. Likewise, the detection of a strong magnetic moment ( > 2 × 10 14 Am 2 ) at Psyche would likely indicate that the body once generated a core dynamo, implying that it formed by igneous differentiation. The Psyche Magnetometer consists of two three-axis fluxgate Sensor Units (SUs) mounted 0.7 m apart along a 2.15-m long boom and connected to two Electronics Units (EUs) located within the spacecraft bus. The Magnetometer samples at up to 50 Hz, has a range of ± 80 , 000 nT , and an instrument noise of 39 pT axis - 1 3 σ integrated over 0.1 to 1 Hz. The two pairs of SUs and EUs provide redundancy and enable gradiometry measurements to suppress noise from flight system magnetic fields. The Magnetometer will be powered on soon after launch and acquire data for the full duration of the mission. The ground data system processes the Magnetometer measurements to obtain an estimate of Psyche's dipole moment.

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来源期刊
Space Science Reviews
Space Science Reviews 地学天文-天文与天体物理
CiteScore
19.70
自引率
3.90%
发文量
60
审稿时长
4-8 weeks
期刊介绍: Space Science Reviews (SSRv) stands as an international journal dedicated to scientific space research, offering a contemporary synthesis across various branches of space exploration. Emphasizing scientific outcomes and instruments, SSRv spans astrophysics, physics of planetary systems, solar physics, and the physics of magnetospheres & interplanetary matter. Beyond Topical Collections and invited Review Articles, Space Science Reviews welcomes unsolicited Review Articles and Special Communications. The latter encompass papers related to a prior topical volume/collection, report-type papers, or timely contributions addressing a robust combination of space science and technology. These papers succinctly summarize both the science and technology aspects of instruments or missions in a single publication.
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