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Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea, Sweden
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Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Dec 18, 2015

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Page 1: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Statistical detection of meteor showers using data from the Swedish infrasound network

Ludwik Liszka

Swedish Institute of Space Physics

SLU

901 83 Umea, Sweden

Page 2: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Swedish Infrasound Network

Present stations:

Kiruna

Jamton

Lycksele

Uppsala

Page 3: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Search for small and medium meteor events – objectives:

• To search for meteor events below the infrasonic background level

• To establish a set of indicators which can be used to discriminate a single event

• To develop techniques for extraction of events from combined multi-station data

Page 4: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Meteor on 2002-12-30 in Morjärv, Northern Sweden

Page 5: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Morjärv Meteor

Page 6: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Morjärv Meteor

Angle-of-arrival = 208º Vp = 350 m/s

Page 7: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Morjärv Meteor

Page 8: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

How to optimize the indicators?

Principal Component Analysis (PCA) of multiple indicator data

Indicators are distributions of variables:

Angle-of-arrival

Phase velocity

Crosscorrelation

Spectral slope

Page 9: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Principal component analysis

• Purpose: to find a direction where maximum variance may be found in multivariate data

Page 10: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

PCA

• Direction of maximum variance

Page 11: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Angle-of-arrival

Entropy = -1.18 (Emax=0, Emin=-2.42)

Page 12: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Phase velocity Vp

Page 13: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Cross-correlation

Page 14: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Spectral slope

Page 15: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Parameters of the analysis

• 1 window = 128 data points (7.11 sec)

• The window is moved in 32p steps (overlap)

• Distributions are created for each sample of 50 positions of the window

• 16 samples / 30 minutes

Page 16: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Discrimination of meteor impacts

Selection of data to find proper combination of indicators:

• Concorde vs. North Sea Meteor

Another approach is to apply PCA without pre-selecting transformation coefficients

Page 17: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Comparison of indicators

Page 18: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Plot of component loadings

Page 19: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

High cross-correlation counts

Page 20: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Meteor discrimination

Page 21: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Bavarian Meteor 2002-04-065th principal component

Page 22: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Discriminant function based on 5th PC

Page 23: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Small meteors – meteor showersLeonids – 2002-11-18

  

Page 24: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Small meteors – meteor showersLeonids – 2001-11-18

Page 25: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Combination of information from 2 stations (North Sea Meteor) Lycksele - Jamton

Page 26: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Combination of information from 2 stations (North Sea Meteor) Lycksele - Kiruna

Page 27: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Combination of information from 2 stations (Leonids 2002-11-18)

Lycksele - Jamton

Page 28: Statistical detection of meteor showers using data from the Swedish infrasound network Ludwik Liszka Swedish Institute of Space Physics SLU 901 83 Umea,

Conclusions

• PCA may be used to discriminate events with a specific signature, like meteor impacts

• The method may be applied to events below the noise level, for example, meteor showers