Linear filters as a method of real-time prediction of geomagnetic activity

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Important factors controlling geomagnetic activity include the solar wind velocity, the strength of the interplanetary magnetic field (IMF), and the field orientation. Because these quantities change so much in transit through the solar wind, real-time monitoring immediately upstream of the earth provides the best input for any technique of real-time prediction. One such technique is linear prediction filtering which utilizes past histories of the input and output of a linear system to create a time-invariant filter characterizing the system. Problems of nonlinearity or temporal changes of the system can be handled by appropriate choice of input parameters and piecewise approximation … continued below

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16 pages

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McPherron, R.L.; Baker, D.N. & Bargatze, L.F. January 1, 1985.

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Description

Important factors controlling geomagnetic activity include the solar wind velocity, the strength of the interplanetary magnetic field (IMF), and the field orientation. Because these quantities change so much in transit through the solar wind, real-time monitoring immediately upstream of the earth provides the best input for any technique of real-time prediction. One such technique is linear prediction filtering which utilizes past histories of the input and output of a linear system to create a time-invariant filter characterizing the system. Problems of nonlinearity or temporal changes of the system can be handled by appropriate choice of input parameters and piecewise approximation in various ranges of the input. We have created prediction filters for all the standard magnetic indices and tested their efficiency. The filters show that the initial response of the magnetosphere to a southward turning of the IMF peaks in 20 minutes and then again in 55 minutes. After a northward turning, auroral zone indices and the midlatitude ASYM index return to background within 2 hours, while Dst decays exponentially with a time constant of about 8 hours. This paper describes a simple, real-time system utilizing these filters which could predict a substantial fraction of the variation in magnetic activity indices 20 to 50 minutes in advance.

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16 pages

Notes

NTIS, PC A02/MF A01; 1.

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  • Chapman conference on solar wind-magnetosphere energy coupling, Pasadena, CA, USA, 12 Feb 1985

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  • Other: DE85010760
  • Report No.: LA-UR-85-1305
  • Report No.: CONF-850277-2
  • Grant Number: W-7405-ENG-36
  • Office of Scientific & Technical Information Report Number: 5692779
  • Archival Resource Key: ark:/67531/metadc1090463

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Office of Scientific & Technical Information Technical Reports

Reports, articles and other documents harvested from the Office of Scientific and Technical Information.

Office of Scientific and Technical Information (OSTI) is the Department of Energy (DOE) office that collects, preserves, and disseminates DOE-sponsored research and development (R&D) results that are the outcomes of R&D projects or other funded activities at DOE labs and facilities nationwide and grantees at universities and other institutions.

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  • January 1, 1985

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  • Feb. 10, 2018, 10:06 p.m.

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  • Jan. 3, 2020, 6:09 p.m.

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McPherron, R.L.; Baker, D.N. & Bargatze, L.F. Linear filters as a method of real-time prediction of geomagnetic activity, article, January 1, 1985; United States. (https://digital.library.unt.edu/ark:/67531/metadc1090463/: accessed July 16, 2024), University of North Texas Libraries, UNT Digital Library, https://digital.library.unt.edu; crediting UNT Libraries Government Documents Department.

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