Wave field analysis by magnetic measurements at satellite arrays: Generalized minimum variance analysis

1996 ◽  
Vol 18 (8) ◽  
pp. 315-319 ◽  
Author(s):  
U Motschmann ◽  
T.I Woodward ◽  
K.H Glassmeier ◽  
D.J Southwood
1996 ◽  
Vol 101 (A3) ◽  
pp. 4961-4965 ◽  
Author(s):  
U. Motschmann ◽  
T. I. Woodward ◽  
K. H. Glassmeier ◽  
D. J. Southwood ◽  
J. L. Pinçon

2021 ◽  
Author(s):  
Benjamin Schwarz ◽  
Korbinian Sager ◽  
Philippe Jousset ◽  
Gilda Currenti ◽  
Charlotte Krawczyk ◽  
...  

<p><span>Fiber-optic cables form an integral part of modern telecommunications infrastructure and are ubiquitous in particular in regions where dedicated seismic instrumentation is traditionally sparse or lacking entirely. Fiber-optic seismology promises to enable affordable and time-extended observations of earth and environmental processes at an unprecedented temporal and spatial resolution. The method’s unique potential for combined large-N and large-T observations implies intriguing opportunities but also significant challenges in terms of data storage, data handling and computation.</span></p><p><span>Our goal is to enable real-time data enhancement, rapid signal detection and wave field characterization without the need for time-demanding user interaction. We therefore combine coherent wave field analysis, an optics-inspired processing framework developed in controlled-source seismology, with state-of-the-art deep convolutional neural network (CNN) architectures commonly used in visual perception. While conventional deep learning strategies have to rely on manually labeled or purely synthetic training datasets, coherent wave field analysis labels field data based on physical principles and enables large-scale and purely data-driven training of the CNN models. The shear amount of data already recorded in various settings makes artificial data generation by numerical modeling superfluous – a task that is often constrained by incomplete knowledge of the embedding medium and an insufficient description of processes at or close to the surface, which are challenging to capture in integrated simulations.</span></p><p><span>Applications to extensive field datasets acquired with dark-fiber infrastructure at a geothermal field in SW Iceland and in a town at the flank of Mt Etna, Italy, reveal that the suggested framework generalizes well across different observational scales and environments, and sheds new light on the origin of a broad range of physically distinct wave fields that can be sensed with fiber-optic technology. Owing to the real-time applicability with affordable computing infrastructure, our analysis lends itself well to rapid on-the-fly data enhancement, wave field separation and compression strategies, thereby promising to have a positive impact on the full processing chain currently in use in fiber-optic seismology.</span></p>


Solar Physics ◽  
2020 ◽  
Vol 295 (3) ◽  
Author(s):  
Rosemeire Aparecida Rosa Oliveira ◽  
Marcos William da Silva Oliveira ◽  
Arian Ojeda-González ◽  
Victor De La Luz

1997 ◽  
Vol 102 (5) ◽  
pp. 2757-2770 ◽  
Author(s):  
A. J. Berkhout ◽  
D. de Vries ◽  
J. J. Sonke

2020 ◽  
Vol 9 (2) ◽  
pp. 471-481
Author(s):  
Simon Toepfer ◽  
Yasuhito Narita ◽  
Daniel Heyner ◽  
Patrick Kolhey ◽  
Uwe Motschmann

Abstract. Minimum variance distortionless projection, the so-called Capon method, serves as a powerful and robust data analysis tool when working on various kinds of ill-posed inverse problems. The method has not only successfully been applied to multipoint wave and turbulence studies in the context of space plasma physics, but it is also currently being considered as a technique to perform the multipole expansion of planetary magnetic fields from a limited data set, such as Mercury's magnetic field analysis. The practical application and limits of the Capon method are discussed in a rigorous fashion by formulating its linear algebraic derivation in view of planetary magnetic field studies. Furthermore, the optimization of Capon's method by making use of diagonal loading is considered.


Author(s):  
Kerry E. Back

The mean‐variance frontier is characterized with and without a risk‐free asset. The global minimum variance portfolio and tangency portfolio are defined, and two‐fund spanning is explained. The frontier is characterized in terms of the return defined from the SDF that is in the span of the assets. This is related to the Hansen‐Jagannathan bound. There is an SDF that is an affine function of a return if and only if the return is on the mean‐variance frontier. Separating distributions are defined and shown to imply two‐fund separation and mean‐variance efficiency of the market portfolio.


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