From version 1.1 >
edited by Barry Bishop
on 2018/02/11 10:36
To version < 4.1 >
edited by ahirtl
on 2018/02/13 14:18
>
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Summary

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1 1  
2 +
2 2  === Details ===
3 3  
4 -|**Acronym**|
5 -|**Description**|
6 -|**Principal Investigator (PI)**|
7 -|**Organisation** |
5 +|**Acronym**|None given
6 +|**Description**|Geophone Nodes are self-contained seismic data recorders that can measure seismic waves both passive and those generated by a source e.g Hammer and a plate.
7 +|**Principal Investigator (PI)**|Mohammed Al Hosni
8 +|**Organisation** |Petroleum Development Oman
8 8  
9 9  === Summary ===
10 10  
12 +The self-contained light weight Geophone units can record subtle seismic waves passively and from an active source for more than 50 continuous days. Using these nodes allows a robust deployment of a seismic survey along with a simple hammer source or passive source can allow the detection of shallow aquifers by detecting changes in seismic impedance (velocity x density in the subsurface).
11 11  
12 12  === Objectives ===
13 13  
16 +It is essential to know if there is water present in Mars shallow subsurface. This experiment will utilize a sensitive self-contained geophones to record both active and passive seismic signal to delineate shallow aquifers. The experiment will highlight the deployment of self-contained geophone units for subsurface investigation.
14 14  
15 15  === Experiment Data ===
16 16  
17 17  |=Date|=Files
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21 +|[[05-Feb-2018>>https://mission.oewf.org/archive_downloads/amadee18/19-WaterExplorer/2018-02-05/]]|Measurements file
22 +|[[10-Feb-2018>>https://mission.oewf.org/archive_downloads/amadee18/19-WaterExplorer/2018-02-10/]]|Notes
23 +|[[11-Feb-2018>>https://mission.oewf.org/archive_downloads/amadee18/19-WaterExplorer/2018-02-11/]]|Notes
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