Design and development of a deployable boom for the MAG payload onboard Aditya-L1 spacecraft

IF 2.2 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Vipin K. Yadav, Pankaj Agarwal, Narendra S., Vijay Shankar Rai, Vijaya Y., Monika Mahajan, Mallikarjun K.V.L.N., Srikar P. Tadepalli
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引用次数: 0

Abstract

To measure the local magnetic field in space, magnetometers are regularly flown onboard space missions. In general, the spacecrafts carrying the magnetic field measuring instruments themselves generate a magnetic field which acts as magnetic noise thereby compromising the accurate measurements of magnetic fields onboard. To overcome this handicap, the spacecrafts employ long booms so that the magnetic field sensors are placed near the tip of these booms away from the spacecraft and the magnetic contamination produced by it can be avoided. The first Indian solar mission, to continuously observe and study the Sun, Aditya-L1 is placed in a halo-orbit around the first Lagrangian (L1) point. A fluxgate magnetometer (MAG) is one of the seven payloads onboard Aditya-L1 spacecraft to measure the interplanetary magnetic field (IMF) around the L1 point. A 6 m long non-conducting deployable boom holds two sets of the MAG sensors. In this paper, the technical design and the realization of this MAG boom is described which is working as expected in an orbit around the L1 point.

Abstract Image

Aditya-L1航天器上用于MAG有效载荷的可展开吊臂的设计和发展
为了测量太空中的局部磁场,磁力计经常在太空任务中飞行。一般来说,携带磁场测量仪器的航天器本身会产生磁场,产生磁噪声,从而影响对航天器上磁场的准确测量。为了克服这一缺陷,航天器采用了长臂,这样磁场传感器就被放置在远离航天器的长臂顶端附近,这样就可以避免由此产生的磁污染。印度的第一个太阳任务,持续观察和研究太阳,Aditya-L1被放置在围绕第一个拉格朗日点(L1)的光环轨道上。磁通门磁强计(MAG)是Aditya-L1航天器上用于测量L1点周围行星际磁场(IMF)的七个有效载荷之一。一个6米长的非导电可展开吊杆容纳两套MAG传感器。本文介绍了在L1点轨道上按预期工作的MAG弹臂的技术设计和实现。
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来源期刊
Experimental Astronomy
Experimental Astronomy 地学天文-天文与天体物理
CiteScore
5.30
自引率
3.30%
发文量
57
审稿时长
6-12 weeks
期刊介绍: Many new instruments for observing astronomical objects at a variety of wavelengths have been and are continually being developed. Furthermore, a vast amount of effort is being put into the development of new techniques for data analysis in order to cope with great streams of data collected by these instruments. Experimental Astronomy acts as a medium for the publication of papers of contemporary scientific interest on astrophysical instrumentation and methods necessary for the conduct of astronomy at all wavelength fields. Experimental Astronomy publishes full-length articles, research letters and reviews on developments in detection techniques, instruments, and data analysis and image processing techniques. Occasional special issues are published, giving an in-depth presentation of the instrumentation and/or analysis connected with specific projects, such as satellite experiments or ground-based telescopes, or of specialized techniques.
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