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groups:homestake:meetings:20170413 [2017/04/13 11:56] mandicgroups:homestake:meetings:20170413 [2017/04/13 12:20] (current) mandic
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       * Daniel/Gary/Pat: this only includes the errors introduced by the matrix inversion, which depends only on the gamma-factors, i.e. data is not included.        * Daniel/Gary/Pat: this only includes the errors introduced by the matrix inversion, which depends only on the gamma-factors, i.e. data is not included. 
     * Parameter estimation for Rayleigh and Love (Pat/Levi) [[http://homepages.spa.umn.edu/~meyers/local_r_wave_velocity/Transient%20Analysis%20%5bLocal%20r-wave%20velocity%5d.html|local r-wave velocities]]     * Parameter estimation for Rayleigh and Love (Pat/Levi) [[http://homepages.spa.umn.edu/~meyers/local_r_wave_velocity/Transient%20Analysis%20%5bLocal%20r-wave%20velocity%5d.html|local r-wave velocities]]
 +      * Trying to estimate the local Rayleigh wave velocity by cross correlating different stations. Get a large difference when compared to the velocity estimate from the location of the source (mining explosion). Have to be careful distinguishing between the group and phase velocities. 
 +      * Vuk: have different ways of estimating the velocity: Pat/Tanner's work, active excitations, Daniel's work. Should try to bring them together, make comparisons. Pat will start a page where we can summarize these estimates. 
     * [[http://web.gps.caltech.edu/~dbowden/Homestake/2017-04-13_bowden.pdf|Daniel slides]]     * [[http://web.gps.caltech.edu/~dbowden/Homestake/2017-04-13_bowden.pdf|Daniel slides]]
       * Repeated the studies of noise variations over the entire data set, now that it is available. Find similar trends to Tanner's, horizontal directions on the surface are much noisier due to tilt noise (weather, temperature etc). Also find that all channels on the surface are noisier than underground, due to anthropogenic sources. Observe a bump at 2 Hz in all channels, with some variation over time - not sure what causes this.       * Repeated the studies of noise variations over the entire data set, now that it is available. Find similar trends to Tanner's, horizontal directions on the surface are much noisier due to tilt noise (weather, temperature etc). Also find that all channels on the surface are noisier than underground, due to anthropogenic sources. Observe a bump at 2 Hz in all channels, with some variation over time - not sure what causes this.
       * Also looked at a teleseismic event in more detail: using N-1 stations to predict the incident waveform, and then compute the expected waveform at the N-th station and compare with the observed waveform at the N-th station. Assume simple reflection off of a plane, no coupling P-S waves, assumes known isotropic velocity etc. Still gets a very good agreement, but can improve it in multiple ways.        * Also looked at a teleseismic event in more detail: using N-1 stations to predict the incident waveform, and then compute the expected waveform at the N-th station and compare with the observed waveform at the N-th station. Assume simple reflection off of a plane, no coupling P-S waves, assumes known isotropic velocity etc. Still gets a very good agreement, but can improve it in multiple ways. 
 +      * Interested in trying something like a Wiener filter on a transient event (as opposed to background data), will work with Michael.
  
   * Papers   * Papers
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       * Leads: Vuk, Gary, Victor       * Leads: Vuk, Gary, Victor
       * target: Seism. Research Lett., 6000 words, 10 figures.       * target: Seism. Research Lett., 6000 words, 10 figures.
 +      * No time to discuss, aim to update the paper draft over the next 3 weeks and have a more polished draft by next meeting.
  
     * Active excitation overview paper     * Active excitation overview paper
groups/homestake/meetings/20170413.1492102572.txt.gz · Last modified: 2017/04/13 11:56 by mandic