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POSTER:
A Versatile GPS System for Monitoring Deformation of Active Landslides and Volcanoes


-- Richard G. LaHusen, and Mark E. Reid, 2000,
A Versatile GPS System for Monitoring Deformation of Active Landslides and Volcanoes: Transactions of the American Geophysical Union, v.81, n.48, p.F320

What the Poster Looks Like:



What poster looks like


System Design:

Image, System Design - Field Stations and Base Stations

  • FIELD STATION:
  • GPS Antenna to
  • GPS Receiver with raw data output to
  • USGS V2000 controller card to
  • Radio Modem to
  • Radio Antenna to
  • BASE STATION:
  • Radio Antenna to
  • Radio Modem to
  • Windows PC to
  • Phone or Internet to
  • Graphical Output


Trial Applications:

  • Mission Peak, Fremont, California:
    An ideal first site for trial application is found at Mission Peak Landslide in Fremont, California. A massive rock block at the head of the landslide has intermittently moved several decimeters during the last several years. We installed the system and started its operation the end of January 2000, before seasonal movement began.

    Antenna: Micropulse
    Receiver: Canadian Marconi Allstar
    OEM single frequency
    Transceiver: Microwave Data Systems
    MDS MHz spread spectrum
    Data processing engine: Waypoint Precise DLL
    Baseline length: meters
    Operating schedule: Store forward and process minutes of second
    L1 data every minute intervals

    Image, Mission Peak GPS Monitoring System
    Mission Peak Photo (top): Photo above shows the massive sandstone block with prominent tension cracks. The complete GPS master station (MS) is on stable ground near the ridgetop. The remote instrument station (RS) is located downslope but just off the block for survivability. The remote GPS antenna (RA) is on the block and cabled to the remote station.
    Mission Peak Photo (lower right): The lower station is located on the moving block. Both GPS and radio antennas are on the mast near the electronics package inside a box with a 20 watt solar panel.


Results for Mission Peak:

  • The massive block started moving in late February, initially moving at less than 1 cm/week then accelerated to twice that velocity apparently in response to periods of rainfall. The block decelerated at the cessation of seasonal rains at the end of March, but remained moving at a rate of 1 mm/week until late July. About 5 cm of cumulative displacement were detected over the 4 month period from February 1, 2000 to June 1, 2000.

    Image, Mission Peak GPS Monitoring System
    Mission Peak: Rainfall (top); Landslide Block Movement Daily median values (bottom)


  • The inherent noise in GPS measurements can be seen in this graph (below) showing all of the individual fixed static solutions. These typically showed repeatability +/- 1 cm horizontally and +/- 2cm vertically. In order to better discern and visualize trends in the time-series, the median values for of a variable number of individual static solutions were found. This simple approach was found to be very effective in removing noise from the data and discriminating subtle movements.

    Image, Mission Peak, Filtered and Unfiltered Data
    Mission Peak: Comparison of filtered and unfiltered data.


  • Near real-time data on the Internet. Graphs of filtered and unfiltered solutions are automatically updated every thirty minutes and served via phone or network connections.

    Image, Mission Peak Webpage Examples
    Mission Peak: Graphs of filtered and unfiltered solutions are automatically updated every thirty minutes and served via phone or network connections. Graph on the left shows "Last 4 months - daily average values". Graph on the right shows "Last 2 days - ALL solutions No filtering".


Conclusions:

  • An automated GPS system for near real-time monitoring of remote geohazards was successfully developed and applied. The modular design uses a new low-power controller (USGS V2000) to store and forward raw data from a variety of GPS receivers to a Windows-based PC that controls the remote stations and intermittently calculates fixed static solutions. Initial short baseline (<10 km) applications were configured using L1-only Marconi Allstar receivers and Waypoint Precise DLL for processing. Individual solutions obtained twice per hour from 5-20 minutes of 10-second data showed repeatability of 1 cm horizontal and 2 cm vertical. Simple filtering by finding median of 5 (2 hours) and 48 (24 hour) solutions allowed clear discrimination of sub-centimeter movements.


Mount St. Helens, Washington and Augustine Island, Alaska:

  • Mount St. Helens Volcano, Washington
    One of three stations at Mount St. Helens volcano is located on the dome in the crater. Access to all three remote sites is by helicopter. Another GPS site at Mount St. Helens is housed in a fiberglass shelter with a small solar panel on the roof. Inside the fiberglass shelter is a yagi antenna, 2 batteries, and an environmental case containing a CMC Allstar L1 receiver, the USGS V2000 controller, and a 900 MHz spread spectrum transceiver.

    Antenna: Micropulse
    Receiver: Canadian Marconi Allstar
    OEM single frequency
    Transceiver: Microwave Data Systems
    MDS MHz spread spectrum
    Data processing engine: Waypoint Precise DLL
    Baseline length: 2 to 6 kilometers
    Operating schedule: Store forward and process minutes of second
    L1 data every minute intervals



  • Augustine Island Volcano, Alaska
    Three field stations were installed on Augustine Island Volcano in the Fall of 2000 and data are telemetered to Homer, Alaska. This site is particularly challenging because of difficult access, severe snow and ice accumulations, limited solar influx in Winter and presence of corrosive aerosols.

    Antenna: Micropulse
    Receiver: Canadian Marconi Allstar
    OEM single frequency
    Transceiver: Microwave Data Systems
    MDS MHz spread spectrum
    Data processing engine: Waypoint Precise DLL
    Baseline length: 2 to 4 kilometers
    Operating schedule: Store forward and process minutes of second
    L1 data every minute intervals
    Transmission distance: >100 kilometers


Full-Size PDF Version:

PDF Version of Poster, click to enlarge PDF Version
[10M,PDF]


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12/03/02, Lyn Topinka