Seismic Network Operations

US GOGA

Godfrey, Georgia, USA

US GOGA commences operations on: 1993,068

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Host:
Latitude: 33.411
Longitude: -83.467
Elevation: 116.5
Datalogger: Q330
Broadband: CMG3TB
Accelerometer: EST-S
Telemetry Status at the NEIC: Last Data In Less Than 10 Minutes
Station Photo Station Photo Station Photo 
Location CodeChannel CodeInstrumentFlagsSample RateDipAzimuthDepth
00BH1CMG3TBCG40.000.00112.8033.50
10BH1KS54000CG40.000.00140.40132.60
00BH2CMG3TBCG40.000.00202.8033.50
10BH2KS54000CG40.000.00230.40132.60
00BHZCMG3TBCG40.00-90.000.0033.50
10BHZKS54000CG40.00-90.000.00132.60
20HN1EST-S2GTG200.000.000.000.00
20HN2EST-S2GTG200.000.0090.000.00
20HNZEST-S2GTG200.00-90.000.000.00
30LDOMICROBAROGRAPHCG1.000.000.000.00
00LH1CMG3TBCG1.000.00112.8033.50
10LH1KS54000CG1.000.00140.40132.60
10LH2KS54000CG1.000.00230.40132.60
00LH2CMG3TBCG1.000.00202.8033.50
00LHZCMG3TBCG1.00-90.000.0033.50
10LHZKS54000CG1.00-90.000.00132.60
20LN1EST-S2GCG1.000.000.000.00
20LN2EST-S2GCG1.000.0090.000.00
20LNZEST-S2GCG1.00-90.000.000.00
00VH1CMG3TBCG0.100.00112.8033.50
10VH1KS54000CG0.100.00140.40132.60
00VH2CMG3TBCG0.100.00202.8033.50
10VH2KS54000CG0.100.00230.40132.60
00VHZCMG3TBCG0.10-90.000.0033.50
10VHZKS54000CG0.10-90.000.00132.60
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As part of the annual calibration process, the USGS runs a sequence that includes a random, a step, and several sine wave calibrations.  The USGS analyzes the random binary calibration signal in order to estimate the instrument response.  The figures below show the results from the analysis of the most recent processed calibration at the station.

We use an iterative three-step method to estimate instrument response parameters (poles, zeros, sensitivity and gain) and their associated errors using random calibration signals. First, we solve a coarse non-linear inverse problem using a least squares grid search to yield a first approximation to the solution. This approach reduces the likelihood of poorly estimated parameters (a local-minimum solution) caused by noise in the calibration records and enhances algorithm convergence. Second, we iteratively solve a non-linear parameter estimation problem to obtain the least squares best-fit Laplace pole/zero/gain model. Third, by applying the central limit theorem we estimate the errors in this pole/zero model by solving the inverse problem at each frequency in a 2/3rds-octave band centered at each best-fit pole/zero frequency. This procedure yields error estimates of the 99% confidence interval.

LocChanCal DateEpoch-SpanGradeAmp Nominal Error (dB)Amp Best Fit Error (dB)Phase Nominal Error (degree)Phase Best Fit Error (degree)SensorCal Type
00BHZ2014:1362011:122 to No Ending TimeA0.0190180.00831970.0955940.073087CMG3Random
00BH22014:1362011:122 to No Ending TimeA0.09820.0236670.552470.47294CMG3Random
00BH12014:1362011:122 to No Ending TimeA0.103650.0244230.581320.51186CMG3Random
10BH12014:1372011:122 to No Ending TimeA0.00853390.00702160.075440.06448654000Random
10BH22014:1372011:122 to No Ending TimeA0.0168240.00695730.08430.06605454000Random
10BHZ2014:1372011:122 to No Ending TimeA0.00783950.00687640.0747830.06477254000Random
  1. Current Issues.
    LNZ channel on the Episensor appears to be bad. The horizontal components of the CMG3T show LP pulsing.
  2. 2004-12-13
    Upgraded to Q330 digitizer.