Izvestiya, Physics of the Solid Earth

, Volume 48, Issue 5, pp 395–409

Recognition of disturbances with specified morphology in time series: Part 2. Spikes on 1-s magnetograms

  • A. A. Soloviev
  • S. M. Agayan
  • A. D. Gvishiani
  • Sh. R. Bogoutdinov
  • A. Chulliat
Article

DOI: 10.1134/S106935131204009X

Cite this article as:
Soloviev, A.A., Agayan, S.M., Gvishiani, A.D. et al. Izv., Phys. Solid Earth (2012) 48: 395. doi:10.1134/S106935131204009X

Abstract

Preliminary magnetograms contain different types of temporal anthropogenic disturbances: spikes, baseline jumps, drifts, etc. These disturbances should be identified and filtered out during the preprocessing of the preliminary records for the definitive data. As of now, at the geomagnetic observatories, such filtering is carried out manually. Most of the disturbances in the records sampled every second are spikes, which are much more abundant than those on the magnetograms sampled every minute. Another important feature of the 1-s magnetograms is the presence of a plenty of specific disturbances caused by short-period geomagnetic pulsations, which must be retained in the definitive records. Thus, creating an instrument for formalized and unified recognition of spikes on the preliminary 1-s magnetograms would largely solve the problem of labor-consuming manual preprocessing of the magnetic records. In the context of this idea, in the present paper, we focus on recognition of the spikes on the 1-s magnetograms as a key point of the problem. We describe here the new algorithm of pattern recognition, SPs, which is capable of automatically identifying the spikes on the 1-s magnetograms with a low probability of missed events and false alarms. The algorithm was verified on the real magnetic data recorded at the French observatory located on Easter Island in the Pacific.

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Copyright information

© Pleiades Publishing, Ltd. 2012

Authors and Affiliations

  • A. A. Soloviev
    • 1
  • S. M. Agayan
    • 1
  • A. D. Gvishiani
    • 1
  • Sh. R. Bogoutdinov
    • 1
  • A. Chulliat
    • 2
  1. 1.Geophysical Center of the Russian Academy of SciencesMoscowRussia
  2. 2.Institute de Physique du Globe de ParisParisFrance

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