从 DSX 星载窄带接收器获取内磁层的电子密度规格

IF 1.6 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS
Radio Science Pub Date : 2024-02-01 DOI:10.1029/2023RS007907
Yi-Jiun Su;John A. Carilli;J. Brent Parham;Xiangning Chu;Ivan A. Galkin;Gregory P. Ginet
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引用次数: 0

摘要

电子密度在波的传播研究中发挥着重要作用,而且已知电子密度与折射率和辐射带扩散系数有关。我们调查的主要目的是探索是否有可能实施一种机载信号处理算法,以便从波谱图的上混合共振迹线中自动获取电子密度,用于未来的任务。我们将为生物医学图像分割开发的 U-Net 用作深度学习架构,并将其结果与更传统的半自动方法提取的结果进行比较。作为产品,我们获得了2019年至2021年整个DSX任务的电子密度和回旋频率,以供进一步分析和应用。由于空间测量有限,提出了一种基于数据统计和随机化的合成图像生成器,作为开发生成式对抗网络的第一步,希望为高级机器学习提供无限的现实数据源。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Electron density specification in the inner magnetosphere from the narrow band receiver onboard DSX
Electron density plays an important role in the study of wave propagation and is known to be associated with the index of refraction and radiation belt diffusion coefficients. The primary objective of our investigation is to explore the possibility of implementing an onboard signal processing algorithm to automatically obtain electron densities from the upper hybrid resonance traces of wave spectrograms for future missions. U-Net, developed for biomedical image segmentation, has been adapted as our deep learning architecture with results being compared with those extracted from a more traditional semi-automated method. As a product, electron densities and cyclotron frequencies for the entire DSX mission between 2019 and 2021 are acquired for further analysis and applications. Due to limited space measurements, a synthetic image generator based on data statistics and randomization is proposed as an initial step toward the development of a generative adversarial network in hopes of providing unlimited realistic data sources for advanced machine learning.
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来源期刊
Radio Science
Radio Science 工程技术-地球化学与地球物理
CiteScore
3.30
自引率
12.50%
发文量
112
审稿时长
1 months
期刊介绍: Radio Science (RDS) publishes original scientific contributions on radio-frequency electromagnetic-propagation and its applications. Contributions covering measurement, modelling, prediction and forecasting techniques pertinent to fields and waves - including antennas, signals and systems, the terrestrial and space environment and radio propagation problems in radio astronomy - are welcome. Contributions may address propagation through, interaction with, and remote sensing of structures, geophysical media, plasmas, and materials, as well as the application of radio frequency electromagnetic techniques to remote sensing of the Earth and other bodies in the solar system.
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