To: | [email protected] |
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Subject: | Re: VLF: DK7FC's 7th VLF kite experiment |
From: | Daniele Tincani <[email protected]> |
Date: | Thu, 7 Oct 2010 23:01:14 -0700 (PDT) |
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References: | <[email protected]> |
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Hello Stefan, VLF,
Paul Nicholson (on his web page about his great work on data from Stefan's recent experiment) writes:
Best results were obtained with the loop antenna oriented towards DK7FC (rather than oriented to null the average background noise). Sferic blanking made a useful reduction in background. The signal was band-limited to 6-12kHz before applying blanking with threshold equal to the mean amplitude and no dwell time. Blanking was activated approximately 60% of the time and effectively removed all non-Gaussian noise components. I would like to apply spheric-blanking on recorded data by using SpectrumLab. How do translate Paul's indications in SpecLab blanker parameters, I mean how should I proceed in practice to set the blanker thresholdto the mean amplitude with no dwell time?
Many thanks to all in advance for suggestions.
Best regards Daniele
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