Whole hole Round Multi-Sensor Logger (WRMSL) User Guide

Manual Information

Table Of Contents

Table of Contents
maxLevel

3 exclude Table of Contents

Introduction

This User Guide provides an overview on how to use the IMS application to run the Whole Round and Special Task Multi-Sensor Loggers (WRMSL and STMSL). It assumes that the calibrations are complete and logging systems are ready to measure . (That means that all of the necessary configuration and calibration procedures are completed.)sections.

Launch the IMS Application

Launch IMS from (1) the Windows Start menu or the desktop icon (2Figure 1) a desktop icon. 

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Figure 1. IMS Icon

At launch, the program begins the an initialization process:

• Testing instrument communications
• Reloading configuration values
• Homing the pusher arm of the motion control system.

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After successful initialization, the IMS

Control and

Instruments' windows appear (

Figure 2). The IMS Control window is on the left and the

Instruments' windows on the right

. 

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Figure 2. IMS Control and Instrument Windows.

Start a Measurement

1. Place the whole-round section on the track between the top-of-section sensor and the pusher arm (Figure 3).
2. Orient the section with the blue endcap towards the top-of-section sensor with working label UP.
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3. Click START to open the Section Information window. 
4. When the Section Information window opens (aboveFigure 4) opens, the cursor should be in the SCAN input box. If not, click in the box.
5. Hold the scanner over the label and center the dot-code with the red crosshairs while pulling the trigger.
6. At the scanner beep, the Sample_ID and the LIMS_ID should correctly display on the screen. If not, rescan.

1. re-scan.
2. Click Measure. The pusher arm moves forward and pushes the section until the blue endcap breaks the light beam

1. of the

1. sensor. The pusher then moves the section into the first measurement position and triggers the instruments to measure.
2. The move and measure process repeats until the pusher arm reaches its motion limits. The pusher retracts to the home position, ready to receive the next section, and

1. the Section Information

1.  window opens to repeat the process.

Measurement Sequence

The WRMSL and STMSL are push tracks; each section pushes the previous section(s) through a set of instruments. Although it is possible to continuously process cores without a break, some of the instruments require a periodic background measurement to correct for sensor drift. The track in the immediate area of the instruments must be free of cores for this background measurement.

By convention, we break the sequence of sections for background measurement between succeeding cores. To push the last section through we use a "pusher," which is a piece of core liner filled with DI water long enough to push the end of the last section through the last sensor on the track.
 
Therefore, the functional definition of a sequence is from the first section measured after the "pusher" (or the launch of IMS) and ends the next time the "pusher" is used. Generally, this corresponds to the first and last section of a core.

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Preparing IMS

Intentions and Assumptions

This section covers the steps needed to take meaningful measurements. Perform these steps prior to starting measurements on a new site. This does not cover physical setup of the hardware or initial deployment of the software.

A Quick Introduction to the IMS Program Structure

IMS is a modular program. Individual modules are as follows:

• INST plug-ins: codes for each of the instruments
• MOTION plug-in: codes for the motion control system
• DAQ Engine: code that organizes INST and MOTION plug-ins into a track system

The IMS Main User Interface (IMS-UI) calls these modules, instructs them to initialize, and provides a user interface to their functionality.

1. Clicking Cancel button (and confirming) will cause loss of data for the sections which have not completed all of their measurements for a particular instrument. 

Note:  The label ID is used to query LIMS for the curated length. If not connected to the web servers, the length in the label bar code is used. Knowing the length is not critical, as the track will actually measure the length as part of its section handling process. If the top of the section is missing because a whole-round sample was removed, enter the length of the missing interval in the left hand area (Figure 4) so the sample position can be corrected. DO NOT place any type of spacer in front of the section to make up for the missing interval. Whole-rounds taken from the bottom of the section will not affect the measurement process.

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Figure 3. Blue end cap near the top-of-section sensor, clear end (bottom of section) touching the pusher.

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Figure 4. Section Information scanning window.
.

Measurement Sequence

The WRMSL and STMSL are push tracks; each section pushes the previous section(s) through a set of instruments. Although it is possible to continuously process cores without a break, some of the instruments require a periodic background measurement to check and correct, if necessary, sensor drift. The track in the immediate area of the instruments must be free of cores for this background measurement.

By convention, we break the sequence of sections for background measurement between succeeding cores. To push the last section through we use a "pusher," which is a piece of core liner filled with DI water long enough to push the end of the last section through the last sensor on the track.
 
Therefore, the functional definition of a sequence is from the first section measured after the "pusher" (or the launch of IMS) and ends the next time the "pusher" is used. Generally, this corresponds to the first and last section of a core.

To run the "pusher", click the PUSHER END SEQUENCE (Figure 5) button located in the Section Information window.
To configure or calibrate the track, read the following sections.         Image Added

Figure 5. End of Sequence Pusher button.

Preparing IMS

Perform these steps prior to starting measurements on a new site. This does not cover physical setup of the hardware or initial deployment of the software.

A Quick Introduction to the IMS Program Structure

IMS is a modular program. Individual modules are as follows:

• INST plug-ins: codes for each of the instruments
• MOTION plug-in: codes for the motion control system
• DAQ Engine: code that organizes INST and MOTION plug-ins into a track system

The IMS Main User Interface (IMS-UI) calls these modules, instructs them to initialize, and provides a user interface to their functionality.

The WRMSL and STMSL systems are built with three INST modules (Gamma Ray Attenuation, P-wave, and Magnetic Susceptibility), one MOTION module, and one DAQ Engine module. Each module manages a configuration file that opens the IMS program at the same state it was when previously closed and provides utilities for user edit or modification of the configuration data and calibration routines.

The five buttons on the  IMS Control window provide access to utilities/editors via drop-down menus (Figure 6).

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Figure 6. Five buttons from IMS Control window. Menus within each button.

Initial Instrument Setup

Click on the Instruments menu to select each instrument's Setup Editor (Figure 7). In general, the values shown in the Setup Editor rarely need to be changed. Regardless, check these values at the beginning of every expedition. Note: Do not change these values without reading the vendor's documentation.

GRA: Setup

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Figure 7. GRA Setup Editor.

General Information

Instrument X Offset: Offset along the X-axis (push direction) from the home switch to the center of the gamma ray source collimator.
Sensor Width

The five buttons on the IMS-UI window provide access to utilities/editors via dropdown menus as shown below.
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Click on the Instrument menu to select each instrument's Setup Editor. In general, the values shown in the Setup Editor rarely need to be changed. Regardless, check these values at the beginning of every expedition!

GRA: Setup

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General Information

Instrument X Offset: Offset along the X-axis (push direction) from the home switch to the center of the gamma ray source collimator.
Sensor Width: Width along the core axis that influences the measured value; used in calculating edge clearance (if enabled).
Analysis Name: Defined JR_LIMS analysis.
Instrument Group: Defined JR_LIMS instrument group component.
Model: Instrument model number/name of the sensing component.
S/N: Instrument serial number of the sensing component.
Manufacturer's Name: Name of the manufacturer of the sensing component of the instrument.
Menu Name: Name used in the IMS menus
Full Name: Name used in IMS Reports and displays.

Instrument-Specific Information (digiBase Detector)

Detector Address: Instrument unique addressing ID set with the MAESTRO software provided by the vendor.
High Voltage: High voltage value applied to the photomultiplier tube.
Fine Gain: Used in conjunction with coarse gain (jumper setting in the digiBase) to amplify the signal. Affects the peak's position and width in the reported channels.
Gauss STD of Fit: Used to determine the quality of the Gaussian peak fit over the Cs peak (empirically determined).
Start Channel: Start channel of the ROI (region-of-interest).
Number of Channels: Number of channels for the ROI.
Display Width: Width of display about the peak center during acquisition.

Standard Information

Select the standard from the list box to use when the calibrate function is executed. Selecting a standard updates the values displayed below. To edit the values, use the GRA Edit Standards function in the Instrument menu.                         

Calibration DAQ

Parameters used when measuring the GRA standard:
CAL Live Preset: Live time of the measurement.
Core Diameter: Internal diameter of the core liner.
Aluminum Density: Density of the aluminum alloy used to fabricate the standard.

MS: Setup

General Information

Instrument X Offset: Offset along the X-axis (push direction) from the home switch to the center of the MS loop.
Contact Width: Width along the core axis that influences the measured value; used when calculating edge clearance (if enabled).
Units: Set to SI; must match the physical MS meter setting.
Range: Set to 1.0; must match the physical MS meter setting.
Analysis Name: Defined JR_LIMS analysis.
Instrument Group: Defined JR_LIMS instrument group component.
Model: Instrument model number/name of the sensing component.
S/N: Instrument serial number of the sensing component.
Manufacturer's Name: Name of the manufacturer of the sensing component of the instrument.
Menu Name: Name used in the IMS menus.
Full Name: Name used in IMS Reports and displays.

Standard Information

Correction: The vendor provides this value.

• For standard-frequency loops (80 and 90 mm, 565 Hz), this value is 1.000.
• For 10% high loops (80 mm only, 621 Hz), this value is 0.908.
• For 10% low loops (80 mm only, 513 Hz), this value is 1.099.
• For 20% low loops (90 mm only, 452 Hz), this value is 1.174.

PWL: Setup

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General Information

Instrument X Offset: Offset along the X-axis (push direction) from the home switch to the center of the PWL transducers.
Contact Width: Width along the core axis that influences the measured value used when calculating edge clearance (if enabled).
Analysis Name: Defined LIMS analysis value.
Instrument Group: Defined LIMS instrument group component.
Model: Instrument model number/name of the sensing component.
S/N: Instrument serial number of the sensing component.
Manufacturer's Name: Name of the manufacturer of the sensing component of the instrument
Menu Name: Name used in the IMS menus.
Full Name: Name used in IMS Reports and displays.

Liner Correction

Liner Thickness: Thickness of the core liner.
Liner Velocity: Acoustic velocity of the core liner (butyrate).
Liner Delay: Calculated value equivalent to the liner thickness divided by the liner velocity.

Velocity Filter

The filter purpose is to remove extremely low or high velocities.
Velocity Filter: Enable or disable filtering.
Min Velocity Filter: Velocities below this value are not reported.
Max Velocity Filter: Velocities above this value are not reported.

Velocity Filter

Waveform Stack: The number of waveforms stacked and averaged. Minimum 50.

Instrument Calibration

To access an instrument's calibration procedure, click on the Instrument menu and select the instrument's calibration function. Good practice is to calibrate the instrument prior to receiving cores at each new site.

GRA: Calibration

The GRA standard is an aluminum bar inserted into a core liner, which is sealed and filled with DI water. The aluminum bar is machined into discrete steps that provide composite density values for creating a calibration curve of counts vs. density. Before calibration, use the Standard Editor to enter offset and thickness of each step's center. Under the Instrument menu, select GRA: Edit Standards. This only has to be done once, as the values are retained in the configuration file.
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Define two standard sets in the Standard Editor: Density and Water.

• Density: the offset (measured from liner top to center of step) and the thickness of each step are the values shown in the diagram above. Define the offsets in the order they are measured on the track.
• Water: (1) define an offset past the aluminum standard and (2) enter water density (1 g/cm³) as the given value. The water measurement is used to validate the density calibration.

GRA Calibration Process

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PWL: Setup

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General Information

Instrument X Offset: Offset along the X-axis (push direction) from the home switch to the center of the PWL transducers.
Contact Width: Width along the core axis that influences the measured value used when calculating edge clearance (if enabled).
Analysis Name: Defined LIMS analysis value.
Instrument Group: Defined LIMS instrument group component.
Model: Instrument model number/name of the sensing component.
S/N: Instrument serial number of the sensing component.
Manufacturer's Name: Name of the manufacturer of the sensing component of the instrument
Menu Name: Name used in the IMS menus.
Full Name: Name used in IMS Reports and displays.

Liner Correction

Liner Thickness: Thickness of the core liner.
Liner Velocity: Acoustic velocity of the core liner (butyrate).
Liner Delay: Calculated value equivalent to the liner thickness divided by the liner velocity.

Velocity Filter

The filter purpose is to remove extremely low or high velocities.
Velocity Filter: Enable or disable filtering.
Min Velocity Filter: Velocities below this value are not reported.
Max Velocity Filter: Velocities above this value are not reported.

Velocity Filter

Waveform Stack: The number of waveforms stacked and averaged. Minimum 50.

Instrument Calibration

To access an instrument's calibration procedure, click on the Instrument menu and select the instrument's calibration function. Good practice is to calibrate the instrument prior to receiving cores at each new site.

GRA: Calibration

The GRA standard is an aluminum bar inserted into a core liner, which is sealed and filled with DI water. The aluminum bar is machined into discrete steps that provide composite density values for creating a calibration curve of counts vs. density. Before calibration, use the Standard Editor to enter offset and thickness of each step's center. Under the Instrument menu, select GRA: Edit Standards. This only has to be done once, as the values are retained in the configuration file.
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Define two standard sets in the Standard Editor: Density and Water.

• Density: the offset (measured from liner top to center of step) and the thickness of each step are the values shown in the diagram above. Define the offsets in the order they are measured on the track.
• Water: (1) define an offset past the aluminum standard and (2) enter water density (1 g/cm³) as the given value. The water measurement is used to validate the density calibration.

GRA Calibration Process

1. Place the standard on the track with the first step defined in the standard toward the GRA sensor.
2. In the Instrument menu, select GRA: Calibration.
3. The pusher engages the standard and pushes it until it trips the top-of-section sensor, then moves the standard to all of the defined offsets, taking a measurement at each position.
4. After the second position is measured, the calibration data display in the graph along with the calibration line.Image Added
   
   
5. After measuring the last step, the pusher moves the standard to the offset for the water measurement.
6. Using the new calibration data, a density value for water is calculated and compared to the known value of 1 gm/cm3. The curve fit provides the coefficients used in the density calculations, ln I = B(μd) + C; where μ= Compton attenuation coefficient, d = sample diameter, I₀ = gamma ray source intensity, and I = measured intensity of gamma rays passing through the sample. Allowing bulk density to calculated by using, ρ = 1/(μd) × ln (I₀/I).
7. Choose to apply the calibration to all future measurements by clicking OK-APPLY or click CANCEL to restore the previous values.

PWL Calibration

PWL Calibration process

In the Instrument menu, select PWL: Calibration and the PWL Calibration window will open.

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The window opens as seen above. Begin by following the steps on the right sight of the window.

Setting Up a Measurement

Use the controls shown to set the measurement parameters.
Requested Stack: Sets the number of waveforms to average to increase the signal-to-noise ratio.
Threshold: A millivolt value used to find the first arrival peak. For more information on the first arrival determination, see Appendix 1.

Measuring Standard

1. Place the aluminum standard between the transducers. Close the transducers. Aluminum standard width is 76.2mm. Select Laser Offset Correction. Confirm that the Distance matches the standard width.
2. Enter the Aluminum Standard velocity. 6295.00 m/s. Select Determine System Delay. Verify that the Velocity matches the Aluminum Standard.
   
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3. Open transducers. Remove Aluminum Standard. Position the Water Standard in place. Close transducers. Turn on Liner Delay. Liner Thickness is 0.275 cm. Determine Liner Velocity. Verify that the water velocity matches the calculated H2O velocity +/- 1% (liner velocity is calculated based on this).
4. Open transducers. Accept Changes

Quality Assurance/Quality Control

Analytical Batch

The analytical batch is defined by the number of samples run between each sensor calibration. Each sample in the batch run with the current calibration is associated with that calibration data in the LIMS.
Calibrations and calibration timestamps are accessible through each sensor Instrument Interface screen.

Calibration

GRA

Calibration assumes a two-phase system model for sediments and rocks: minerals and interstitial water. Aluminum has an attenuation coefficient similar to common minerals and is used as the mineral phase standard. Pure water is used as the interstitial water phase standard. A piece of core liner containing a telescoping aluminum rod (5 varying thicknesses) and filled with distilled water is measured as a calibration standard. The largest diameter aluminum rod has a porosity of 0% and a bulk density of 2.7 g/cm³. Water has a porosity of 100% and density of 1.00 g/cm³. Intermediate elements verify the linearity of the log density relationship and the alignment of core and sensor. A linear least-squares fit through 3–5 calibration points yields the calibration coefficient. Total measured counts are divided by the counting time to normalize coefficients to counts per second.

MSL

Absolute susceptibility: Sample cubes are measured using the Kappabridge and results compared with corresponding readings from the Bartington instrument. Empirical correction factors have been calculated.

PWL

Pulse detection settings are checked by IODP technicians on a regular basis and do not require adjustments by the user.
Pulse time is a constant which is included in the total time measured as a result of the threshold peak detection procedure used. This value changes depending on the wiring of the system. The user does not need to make adjustments to this factor.
Transducer displacement and traveltime delay calibrations are performed simultaneously and should be executed once per expedition on a routine basis. Displacement measured in volts is calibrated to millimeters by measuring 3 standard acrylic cylinders. A linear least-squares fit to the points defined by the voltage readings (x-axis) and the known standard thickness in millimeters (y-axis) yields the linear coefficients used in the calculation.
Measured travel distance and time must be corrected for twice the liner thickness. This calibration is performed by IODP technicians. Vendor specifications for the wall thickness of the liner are used.

Accuracy

GRA

GRA accuracy is limited by the assumption that the measured material has the same attenuation coefficient as the calibration standards used. For general sediment-water mixtures, this should be the case and error should be <5%.

MSL

Accuracy of the susceptibility meter and sensor loop is 5% (according to Bartington).

PWL

PWL accuracy can be evaluated by measuring pure water at varying and exactly known temperatures. Past experience shows that for a properly calibrated system and good acoustic coupling, the disagreement with published sonic velocity values is less than ±20 m/s.

Precision

GRA

GRA precision is proportional to the square root of the counts measured, as gamma ray emission is subject to Poisson statistics. Measurements with the system have typical count rates of 10,000 (dense rock) to 20,000 (soft mud). If measured for 4 s, statistical error is <40,000 ± 200 cps, or 0.5%.

MSL

MSL precision is 2 x 10^–6 SI. Susceptibility values in natural marine sediment samples over an interval of only a few meters (Milankovitch or millennial scale cyclicity) can range from a few tens to several thousands of 10^–6 SI units. Typically, variations are 2–3 orders of magnitude greater than the precision, making magnetic susceptibility one of the most precise proxies for stratigraphic changes.

PWL

Measurements on standard materials such as water and calibration standards are repeatable within ±1 km/s.

Motion Control

The track's push system consists of a NSK linear actuator driven by Schneider Electric stepping motor: MDrive23. The MDrive 23 is a high torque 1.8º integrated motor-driver-controller that connects to the PC via USB-RS485 cable. An IODP-built interface board (below) provides power control, emergency, limit/home switches, specialty I/O connections, and status lights. With the exception of a built in "Home" function, the MDive's IMS motion software module provides direct control of the motor's functions. The motor can be installed directly out of the box without any special preparation.

At IMS launch, a series of commands are sent to place the motor into a known state and then to search for the home switch and zero the encoder's position out put.

It is assumed that the hardware has been installed correctly and powered up. On the very first launch, a set of default values will be loaded that should get the track safely running. BUT BE READY to kill the motion using the E-stop button. Generally, a run-off is caused by incorrect scaling factors for the gear ratio, screw pitch, and or encoder counts per revolution. Setting these up correctly usually correct the issue.
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MDrive Set up

When you select Setup from the Motion menu bar, the window to the right appears.

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Track Options

Click Motion and Track Options to open the window below. Here is where the relationship between motor revolutions and linear motion of the track is defined.

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Select Axis: In the case of the WRMSL and STMSL, it is always X.
Encoder Pulses/rev: Defined by the manufacturer of the MDrive as 2048.
Screw Pitch: Defined by the NSK actuator manufacturer as 2 cm/screw revolution.
Gear Ratio: In the current configuration, this is 4 to 1 but it can be changed.
Direction: This depends… The STMSL is a right-hand track and a CCW rotation moves the pusher in a positive (from home to end of track) direction. The WRMSL is a left-hand track so this value is set to CW. 

Click Open Utilities to test these settings.
Click Done to save the values or Cancel to return to the previous values.

Fixed Positions

Click Fixed Positions to open the window below. In this window, define fixed track locations used by IMS and enable the top of section (TOS) switch and the runout switch (ROS).

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Select Axis: In the case of the WRMSL and STMSL it is always X.
Max Section Length: Maximum length of section that can be placed in the track and still expect the track to handle and measure correctly. This value is set to 155 cm.
Track length: Distance in cm between the limit switches. Use the motion Utility to determine this value.
Load and Unload: Offset in cm where the track will stop when ready to load a new section of core. In the case of both the WRMSL and STMSL, this the same as the home switch.
Top-of-Section Switch: THIS MUST ALWAYS BE enabled! The IMS software uses this switch to determine the physical length of the section, which is critical to the calculations that move the cores through the sensor. Without a TOS switch, the track is not functional.
Top-of-Section Switch Offset: Distance in cm from the home switch to the TOS switch. There is a utility under the DAQ > Find Top-of-Section Switch menu that will determine this value based on the current DAQ Move motion parameters (discussed in this section). ANY change in the motion profile requires that this utility be run because the final position (where the pusher bar stops) changes.
Push Past: The offset from the TOS to where the pusher to should stop. This value set the maximum measurement interval but MUST be several centimeters less than the distance from the TOS to the limit switch.
Fast Offset: Distance the pusher will move at a higher speed before slowing down to find the TOS switch. This value MUST be several centimeters less than the distance from the TOS to the maximum section length with the pusher arm in the home position.
Run Out Switch: Switch at the end of the track that when enabled pauses the motion, preventing the section from being pushed onto the floor.
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Click Open Utilities to test these settings. Click Done to save the values or Cancel to return to the previous values.

Limit and Home Switches

Click Limit and Home switches to open the window below.

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Select Axis: In the case of the WRMSL and STMSL it is always X.

The MDrive can be used with either a dedicated Home switch or a limit switch as a home switch. These tracks use the dedicated Home switch. Select the appropriate setup for the track in use. Use the Utilities to execute the Home command and verify the correct setting. If the home switch position of detection edge changes, verify the instrument offsets and relocate the TOS switch are still correct. Setting the edge from CW to CCW will change the offset by a least 1 cm

PWL Calibration

PWL Calibration process

In the Instrument menu, select PWL: Calibration and the PWL Calibration window will open.

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The window opens as seen above. Begin by following the steps on the right sight of the window.

Setting Up a Measurement

Use the controls shown to set the measurement parameters.
Requested Stack: Sets the number of waveforms to average to increase the signal-to-noise ratio.
Threshold: A millivolt value used to find the first arrival peak. For more information on the first arrival determination, see Appendix 1.

Measuring Standard

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Quality Assurance/Quality Control

Analytical Batch

The analytical batch is defined by the number of samples run between each sensor calibration. Each sample in the batch run with the current calibration is associated with that calibration data in the LIMS.
Calibrations and calibration timestamps are accessible through each sensor Instrument Interface screen.

Calibration

GRA

Calibration assumes a two-phase system model for sediments and rocks: minerals and interstitial water. Aluminum has an attenuation coefficient similar to common minerals and is used as the mineral phase standard. Pure water is used as the interstitial water phase standard. A piece of core liner containing a telescoping aluminum rod (5 varying thicknesses) and filled with distilled water is measured as a calibration standard. The largest diameter aluminum rod has a porosity of 0% and a bulk density of 2.7 g/cm³. Water has a porosity of 100% and density of 1.00 g/cm³. Intermediate elements verify the linearity of the log density relationship and the alignment of core and sensor. A linear least-squares fit through 3–5 calibration points yields the calibration coefficient. Total measured counts are divided by the counting time to normalize coefficients to counts per second.

MSL

Absolute susceptibility: Sample cubes are measured using the Kappabridge and results compared with corresponding readings from the Bartington instrument. Empirical correction factors have been calculated.

PWL

Pulse detection settings are checked by IODP technicians on a regular basis and do not require adjustments by the user.
Pulse time is a constant which is included in the total time measured as a result of the threshold peak detection procedure used. This value changes depending on the wiring of the system. The user does not need to make adjustments to this factor.
Transducer displacement and traveltime delay calibrations are performed simultaneously and should be executed once per expedition on a routine basis. Displacement measured in volts is calibrated to millimeters by measuring 3 standard acrylic cylinders. A linear least-squares fit to the points defined by the voltage readings (x-axis) and the known standard thickness in millimeters (y-axis) yields the linear coefficients used in the calculation.
Measured travel distance and time must be corrected for twice the liner thickness. This calibration is performed by IODP technicians. Vendor specifications for the wall thickness of the liner are used.

Accuracy

GRA

GRA accuracy is limited by the assumption that the measured material has the same attenuation coefficient as the calibration standards used. For general sediment-water mixtures, this should be the case and error should be <5%.

MSL

Accuracy of the susceptibility meter and sensor loop is 5% (according to Bartington).

PWL

PWL accuracy can be evaluated by measuring pure water at varying and exactly known temperatures. Past experience shows that for a properly calibrated system and good acoustic coupling, the disagreement with published sonic velocity values is less than ±20 m/s.

Precision

GRA

GRA precision is proportional to the square root of the counts measured, as gamma ray emission is subject to Poisson statistics. Measurements with the system have typical count rates of 10,000 (dense rock) to 20,000 (soft mud). If measured for 4 s, statistical error is <40,000 ± 200 cps, or 0.5%.

MSL

MSL precision is 2 x 10^–6 SI. Susceptibility values in natural marine sediment samples over an interval of only a few meters (Milankovitch or millennial scale cyclicity) can range from a few tens to several thousands of 10^–6 SI units. Typically, variations are 2–3 orders of magnitude greater than the precision, making magnetic susceptibility one of the most precise proxies for stratigraphic changes.

PWL

Measurements on standard materials such as water and calibration standards are repeatable within ±1 km/s.

Motion Control

The track's push system consists of a NSK linear actuator driven by Schneider Electric stepping motor: MDrive23. The MDrive 23 is a high torque 1.8º integrated motor-driver-controller that connects to the PC via USB-RS485 cable. An IODP-built interface board (below) provides power control, emergency, limit/home switches, specialty I/O connections, and status lights. With the exception of a built in "Home" function, the MDive's IMS motion software module provides direct control of the motor's functions. The motor can be installed directly out of the box without any special preparation.

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MDrive Set up

When you select Setup from the Motion menu bar, the window to the right appears.

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Track Options

Click Motion and Track Options to open the window below. Here is where the relationship between motor revolutions and linear motion of the track is defined.

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Click Open Utilities to test these settings.
Click Done to save the values or Cancel to return to the previous values.

Fixed Positions

Click Fixed Positions to open the window below. In this window, define fixed track locations used by IMS and enable the top of section (TOS) switch and the runout switch (ROS).

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Limit and Home Switches

Click Limit and Home switches to open the window below.

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Motion Profiles

Click Limit and Home switches to open the window below. The profiles are used to set the speed and acceleration profiles used by the track.

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DAQ Move: This profile controls moves between measurement positions. Set this to a reasonable speed with gradual acceleration so the pusher does not bump the sections.
Limit Seek: This profile finds the limit switch locations. Do not exceed 3 cm/sec and use a large deceleration value or the core could overrun the limit switch and hit the mechanical stop.
Home Final: This profile finds the final location of the home switch. Do not exceed 1 cm/sec and use a large deceleration value.
Load/Unload: This profile moves the pusher back to the load position. Set this to a reasonable but high speed with gradual acceleration and deceleration values. Setting this too slow will waste time, but keep safety in mind.
Push-Slow: This profile allows the pusher to move the new section into contact with the previous section and to locate the top of section. Use a speed a little less than the DAQ Move speed with slightly lower acceleration and deceleration values.
Push-Fast: This profile allows the pusher to move quickly to the TOS switch. Typically, it is set the same as the Load/Unload values.
User Define: This profile is used for testing only in the Motion Utilities program.

Click Open Utilities to test these settings.
Click Done to save the values or Cancel to return to the previous values.

Uploading Data To Lims

Image Removed To up load the images into the database MegaUploadaTron must be running in background. If not already started do the following:

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Data Management

Appendices

Appendix 1: P-wave: Waveform Acquisition and First Arrival Detection

Signal Processing

Figure 2 on the following page summarizes the following signal processing discussion.

Acquisition and Ensemble Averaging

Image Removed

Figure 1

The received waveform is 60 µsec long and digitized at 10 nsec intervals. The first 10 µsec of the waveform is replaced with zeros to remove a large spike that occurs at the beginning of the outgoing pulse. We believe that this noise is generated by the electrical "cross-talk" within the pulser-receiver. 

A Butterworth Bandpass filter is applied to the waveform to reject frequencies less than 0.4 MHz and above 1.0 MHZ. The results of this filtering is stacked, summed, and averaged (ensemble averaging). The size of the stack is pre-set by the user to a value between 10 and 100.
Even with this initial filtering and ensemble averaging, the resulting signal can still contain significant noise generated by the shipboard environment. Figure 1 is typical of the signal quality.

Picking the 1^st Arrival

Attempts to use a cross-correlation method (popular in seismic analysis) have not been successfully applied to IODP data. Coefficients developed for one type of lithology fail when the lithology changes. Therefore, we depend on a threshold-crossing process to determine first arrival time. The weakness of this method is that any high-amplitude noise can cause a false, early pick.
To increase the likelihood of a correct pick, the P-wave Logger software on the Whole Round Multi-Sensor Track (WRMSL) uses a series of mathematical and data manipulation techniques to suppress the noise relative to the peak of the first arrival. Another goal is to eliminate the constant adjustment of the threshold value as the amplitude of the waveform changes due to variation in signal attenuation along the core. As the P-wave Logger is an automated system, constant supervision and adjustment is not practical.

Signal-to-Noise Ratio (SNR) Enhancement

Methods employed are partly based on Dr. Tom O'Haver's 2006 publication: A Pragmatic Introduction to Signal Processing (http://terpconnect.umd.edu/~toh/spectrum/IntroToSignalProcessing.pdf).
Image Removed

Figure 2

The ensemble averaging done at the acquisition stage is effective at eliminating nearly all of the random noise. Unfortunately, our signals contain a great deal of systematic environmental noise that shielding signal cables cannot fully eliminate. To suppress this noise, we need to exploit small differences between the noise and the acoustic pulse. The parameters used in the smoothing operators were developed empirically by measuring a variety of materials and by degrading the signal by attenuation at the pulser-receiver. Time was limited on Expedition 361 to select the best smoothing operators and their parameters. Further experimentation is needed to improve the process and validate that it will work for all possible lithologies recovered by IODP.

1. The first smoothing step passes the waveform through a Savitzky-Golay filter that applies a polynomial least-square fit step-wise through the data (similar to a running average). Experimentation shows that using a 6^th-order polynomial across a 126 data point window will reduce high-amplitude, high-frequency noise while retaining the shape of the acoustic pulse.
2. After the first smoothing operation, we take the 1^st derivative (central-difference) which suppresses the low-frequency noise. The downside to the differentiation is that the process adds back in high-frequency noise.
3. A second smoothing step using FIR operator is then used to reject this noise. The FIR filter coefficients were calculated using LabVIEW tools.

Image Removed

Figure 3. Waveform as absolute values

Figure 3 shows the waveform (as absolute values) before and after the 3-step process and illustrates the significant noise suppression achieved. Attempting to find the first arrival on the unprocessed data would have failed because the amplitude of the noise is greater than the first arrival peak.

Normalization

At this point in the process, a copy of the waveform is normalized to scale between the values of –1 and 1. A copy of the processed waveform is converted to its absolute value and then normalized with the waveform scaled between values of 0 and 1. This normalization is critical to making the threshold picking process indifferent to either amplification or attenuation of the signal. Experience has shown that the threshold value needs little adjustment once chosen unless there is a significant lithology change.

1^st Arrival Time

The threshold crossing is performed on the absolute copy of the waveform. The crossing time is then used as the starting point to find the first zero-crossing in the derivative waveform. From this time value, we subtract 1.5 µsec to account for ¼ wavelength phase shift caused by the 1^st derivative operation and ½ wavelength correction back to the first arrival. See Figure 4 below.
Image RemovedImage Removed

Figure 4: The left-hand graph shows the threshold (Horizontal cursor) crossing the first peak of the acoustic pulse and the 1^st zero-crossing (vertical cursor). After correcting the time, the right-hand graph shows the pick on the original stacked waveform.

Waveform Data

The process described above greatly distorts the original waveform. Artificially induced time shifts are eliminated by the P-wave calibration and rolled into the system time delay value. The waveform archived in the JR_LIMS database is taken after the original signal has been band-pass filtered and ensemble averaged. The data from further processing is discarded after the 1^st arrival has been determined.

to save the values or Cancel to return to the previous values.

Motion Profiles

Click Limit and Home switches to open the window below. The profiles are used to set the speed and acceleration profiles used by the track.

Setting the correct values for the motion profile takes a little experimentation to make the track run efficiently and safely.

Image Added

DAQ Move: This profile controls moves between measurement positions. Set this to a reasonable speed with gradual acceleration so the pusher does not bump the sections.
Limit Seek: This profile finds the limit switch locations. Do not exceed 3 cm/sec and use a large deceleration value or the core could overrun the limit switch and hit the mechanical stop.
Home Final: This profile finds the final location of the home switch. Do not exceed 1 cm/sec and use a large deceleration value.
Load/Unload: This profile moves the pusher back to the load position. Set this to a reasonable but high speed with gradual acceleration and deceleration values. Setting this too slow will waste time, but keep safety in mind.
Push-Slow: This profile allows the pusher to move the new section into contact with the previous section and to locate the top of section. Use a speed a little less than the DAQ Move speed with slightly lower acceleration and deceleration values.
Push-Fast: This profile allows the pusher to move quickly to the TOS switch. Typically, it is set the same as the Load/Unload values.
User Define: This profile is used for testing only in the Motion Utilities program.

Click Open Utilities to test these settings.
Click Done to save the values or Cancel to return to the previous values.

Uploading Data To Lims

Image Added To up load the images into the database MegaUploadaTron must be running in background. If not already started do the following:

1. On the desktop click the MUT icon on the bottom task bar.
2. The following will appear:
   Image Added
   
   
3. Check Automatic Upload in the lower right hand corner and then click the minimize window and MUT will run in background.

Data Management

Once all sections for the Expedition have been sent through the track, all data needs to be placed in the appropriate folders on data1 (S:\data1).
1. Copy *.MS files from archive and place them in the 3.2 Petrophysics WRMSL – MS magnetic susceptibility folder. Confirm relocation. Delete all *.MS files off the local drive.
2. Copy *. GRA files from archive an place them in the 3.1 Petrophysics WRMSL – GRA gamma ray attenuation folder. Confirm relocation. Delete all *.GRA files off the local drive.
3. Copy *.PWL files from archive and place them in 3.4 Petrophysics WRMSL – PWLvelocity on sections folder. Confirm relocation. Delete all *.PWL files off the local drive.

Appendices

Appendix 1: P-wave: Waveform Acquisition and First Arrival Detection

Signal Processing

Figure 2 on the following page summarizes the following signal processing discussion.

Acquisition and Ensemble Averaging

Image Added

Figure 1

The received waveform is 60 µsec long and digitized at 10 nsec intervals. The first 10 µsec of the waveform is replaced with zeros to remove a large spike that occurs at the beginning of the outgoing pulse. We believe that this noise is generated by the electrical "cross-talk" within the pulser-receiver. 

A Butterworth Bandpass filter is applied to the waveform to reject frequencies less than 0.4 MHz and above 1.0 MHZ. The results of this filtering is stacked, summed, and averaged (ensemble averaging). The size of the stack is pre-set by the user to a value between 10 and 100.
Even with this initial filtering and ensemble averaging, the resulting signal can still contain significant noise generated by the shipboard environment. Figure 1 is typical of the signal quality.

Picking the 1^st Arrival

Attempts to use a cross-correlation method (popular in seismic analysis) have not been successfully applied to IODP data. Coefficients developed for one type of lithology fail when the lithology changes. Therefore, we depend on a threshold-crossing process to determine first arrival time. The weakness of this method is that any high-amplitude noise can cause a false, early pick.
To increase the likelihood of a correct pick, the P-wave Logger software on the Whole Round Multi-Sensor Track (WRMSL) uses a series of mathematical and data manipulation techniques to suppress the noise relative to the peak of the first arrival. Another goal is to eliminate the constant adjustment of the threshold value as the amplitude of the waveform changes due to variation in signal attenuation along the core. As the P-wave Logger is an automated system, constant supervision and adjustment is not practical.

Signal-to-Noise Ratio (SNR) Enhancement

Methods employed are partly based on Dr. Tom O'Haver's 2006 publication: A Pragmatic Introduction to Signal Processing (http://terpconnect.umd.edu/~toh/spectrum/IntroToSignalProcessing.pdf).
Image Added

Figure 2

The ensemble averaging done at the acquisition stage is effective at eliminating nearly all of the random noise. Unfortunately, our signals contain a great deal of systematic environmental noise that shielding signal cables cannot fully eliminate. To suppress this noise, we need to exploit small differences between the noise and the acoustic pulse. The parameters used in the smoothing operators were developed empirically by measuring a variety of materials and by degrading the signal by attenuation at the pulser-receiver. Time was limited on Expedition 361 to select the best smoothing operators and their parameters. Further experimentation is needed to improve the process and validate that it will work for all possible lithologies recovered by IODP.

The SNR enhancement process consists of 3 steps: (1) smoothing, (2) 1^st derivative, and (3) smoothing.

1. The first smoothing step passes the waveform through a Savitzky-Golay filter that applies a polynomial least-square fit step-wise through the data (similar to a running average). Experimentation shows that using a 6^th-order polynomial across a 126 data point window will reduce high-amplitude, high-frequency noise while retaining the shape of the acoustic pulse.
2. After the first smoothing operation, we take the 1^st derivative (central-difference) which suppresses the low-frequency noise. The downside to the differentiation is that the process adds back in high-frequency noise.
3. A second smoothing step using FIR operator is then used to reject this noise. The FIR filter coefficients were calculated using LabVIEW tools.

Image Added

Figure 3. Waveform as absolute values

Figure 3 shows the waveform (as absolute values) before and after the 3-step process and illustrates the significant noise suppression achieved. Attempting to find the first arrival on the unprocessed data would have failed because the amplitude of the noise is greater than the first arrival peak.

Normalization

At this point in the process, a copy of the waveform is normalized to scale between the values of –1 and 1. A copy of the processed waveform is converted to its absolute value and then normalized with the waveform scaled between values of 0 and 1. This normalization is critical to making the threshold picking process indifferent to either amplification or attenuation of the signal. Experience has shown that the threshold value needs little adjustment once chosen unless there is a significant lithology change.

1^st Arrival Time

The threshold crossing is performed on the absolute copy of the waveform. The crossing time is then used as the starting point to find the first zero-crossing in the derivative waveform. From this time value, we subtract 1.5 µsec to account for ¼ wavelength phase shift caused by the 1^st derivative operation and ½ wavelength correction back to the first arrival. See Figure 4 below.
Image AddedImage Added

Figure 4: The left-hand graph shows the threshold (Horizontal cursor) crossing the first peak of the acoustic pulse and the 1^st zero-crossing (vertical cursor). After correcting the time, the right-hand graph shows the pick on the original stacked waveform.

Waveform Data

The process described above greatly distorts the original waveform. Artificially induced time shifts are eliminated by the P-wave calibration and rolled into the system time delay value. The waveform archived in the JR_LIMS database is taken after the original signal has been band-pass filtered and ensemble averaged. The data from further processing is discarded after the 1^st arrival has been determined.