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A tool to maximize the scientific output of PWI target physics:
Intelligent Signal Detector Module
J. Lichtenberger (1), P. Steinbach (2) and L. Bodnár (3)
(1) Space Research Group, Department of Geophysics, Eötvös University, Budapest, Hungary
(2) MTA-ELTE Research Group for Geoinformatics and Space Sciences(3) BL Electronics, Solymár, Hungary
Science vs. Technology?
Science in a space experiments is limited by technology → cannot speak about science without taking technology into account
Hard limits: sensors/preamps/sensor location, etc.
Soft(er) limits: data collection/processing policy, mode of operation
Science vs. Technology?
Example 1: measurement averaged over 4 sec spin of MMO (a planned mode) → most of the phenomena (physics) shorter than this period is lost
Example 2: achieving ~1Hz@60kHz resolution at ULF band in PWI, a very long (32768 point) FFT window has to be used, this window is >500msec → the physics inside is lost
Short lived phenomena in Hermean magnetosphere
1. Lion roars: narrow-banded whistler-mode wave packets at the bottom of magnetic trough of magnetosheath mirror waves. (Smith and Tsurutani,1976; Zhang et al. 1998 on Geotail). f~0.1 fce.
May be in Hermean magnetosphere (Baumjohann et. al, 2006)
Short lived phenomena in Hermean magnetosphere
2. Seismo-electromagnetic phenomena (intensive research in Earth): short e.m. emissions (impulses) propagating in magnetoionic medium → dispersion
Is Mercury active in seismological sense?
Mercur model B=20[nT] Ne=1[1/cm3] x=5000[km]
Time [msec]
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0 50 100 150 200 250 3000
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Mercur model B=220[nT] Ne=1[1/cm3] x=5000[km]
Time [msec]
Fre
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[kH
z]
0 50 100 150 200 250 3000
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Short lived phenomena in Hermean magnetosphere
1. Triggered emissions: wave-particle interaction in Hermean magnetosphere with radiation belt particles
Has Mercury radiation belt and ring current (Blomberg and Cumnock, 2004) ?
Technology to maximize the scientific output of PWI target physics:
Intelligent Signal Detector Module
1. Scientific goalDetecting events in PWI VLF data that are shorter
than spinning time (4 sec) of MMO and thus beyond the capabilities of general modes of operation.
The target events are :a. transients generated by
atmospheric/magnetospheric processeslithospheric processesSolar wind-atmosphere interactions
Technology to maximize the scientific output of PWI target physics:
Intelligent Signal Detector Module
b. whistler mode waves generated bytransients (see a.)wave-particle interactionsnonlinear processesSolar wind – magnetosphere interactions
Estimated event durations:for a.: microseconds-few millisecondsfor b.: ten milliseconds-second
Technology to maximize the scientific output of PWI target physics:
Intelligent Signal Detector Module
c. any new phenomena - limited in time- limited in frequency
Theoretical background: UWB short impulse solution of Maxwell’s Equations with arbitrary excitation signal – modeling!
Technology to maximize the scientific output of PWI target physics:
Intelligent Signal Detector Module
Functional description
a. Input data
Raw waveform from EWO or spectrogram (dynamic spectra) of the selected component.
b. Output data
Survey mode: the number of a selected event type during the given period
Burst mode: detected event waveform or spectrogram
Noise background monitoring
Technology to maximize the scientific output of PWI target physics:
Intelligent Signal Detector Module
Functional description
c. Algorithm
2D image correlation using the spectrogram or matched filtering on time domain depending on the signal and CPU load.
d. Patterns
The patterns are generated using theoretical models/assumptions and can be:
- predefined stored in code memory segment
- generated on the fly using different parameter sets and adaptive -procedures depending on the available processing power
- uploaded from the Earth (second phase of operation when enough experience/knowledge have been gathered during the mission)
Technology to maximize the scientific output of PWI target physics:
Intelligent Signal Detector Module
Functional description
c. Algorithm
2D image correlation using the spectrogram or matched filtering on time domain depending on the signal and CPU load.
d. Patterns
The patterns are generated using theoretical models/assumptions and can be:
- predefined stored in code memory segment
- generated on the fly using different parameter sets and adaptive -procedures depending on the available processing power
- uploaded from the Earth (second phase of operation when enough experience/knowledge have been gathered during the mission)
Technology to maximize the scientific output of PWI target physics:
Intelligent Signal Detector Module
HeritageISDM concept is based on various satellite
experiment : - ACTIVE, - COMPASS-2 - SAS2 using ISDM concept flew
here - DEMETER satellites projects in developing phase:
ISS-OBSTANOVKA, VOLCANO series, Venus Entry Probe Mission)
Automatic Whistler Detector and Analyzer system working on various sites all over the world (Hungary; SANAE, Halley, Rothera – Antarctica; South Africa, New Zealand)
Event detection SW diagram
Input DataStream
Evaluationof events
Event dependentdata proc.
Send data toTM process
MDP op system
Publishevent forother apps.
Triggering !
Technology caveat and solution
High frequency resolution in ULF range ↔ optimal time resolution in VLF range.
The domain of signal energy localization proportional to time-bandwidth product T x B
Heisenberg-Gabor inequality: T x B ≥ 1 – a signal cannot have arbitrarily small resolution in time and in frequency
Solution:
a. Alternating long and short FFT window
b. Open ULF data stream with hardware or software