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Last modified by robert on 2026/08/12 13:08
From version 117.2
edited by robert
on 2026/08/12 12:56
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To version 110.9
edited by Jack Dent
on 2026/06/15 10:22
Change comment: (Autosaved)

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1 -XWiki.robert
1 +XWiki.JackD
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73 73  
74 74  If you come to collect your node and it is missing~-~- LOOK FOR IT! It may not have gotten far. We have found dozens of nodes by spending 15 minutes looking for them.
75 75  
76 -= External Power =
77 -
78 -Both the 5Hz IGU-16HR and 5s BD3C-5 can be optionally powered via external battery via either a replacement bottom half (the 5Hz nodes) or a battery cable accessory (BD3C-5) using standard lead acid batteries from 9-36v. We have done preliminary testing at 250 Hz with a 12v battery:
79 -
80 -- BD3C-5: ~~2 days of recording per 1 Ah
81 -
82 -- IGU16-HR 3C:  ~~3.5 days of recording per 1 Ah
83 -
84 -- IGU16-HR 1C: ~~7 days of recording per 1 Ah
85 -
86 -Of course, these can also be fit with a solar panel & charge controller which would then theoretically keep them going indefinitely (limited only by the disk storage, which at 250 Hz could be on the order of 12 months).
87 -
88 88  = **Installation** =
89 89  
90 90  (% class="box infomessage" %)
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106 106  
107 107  [[HERE>>http://auspass.edu.au/field/NODES_blank_fieldlog.pdf]] is an example logsheet that works well for nodes, feel free to print and use!
108 108  
109 -== 2. Burial ==
110 -
111 -ALL nodes should be buried flush with the ground, no exceptions. If the node is sticking up the data data quality will be significantly reduced (especially the horizontal channels, see [[below>>https://auspass.edu.au/xwiki/bin/view/Instrumentation/SmartSolo%20Nodes/#HIGU-16Horizontalnoise26howtoavoid]]). It also catches wind, makes them more visible, etc. But mostly it makes the data bad. Don't be lazy: do it right.
112 -
113 -[[An example of what not to do.>>image:1786503344572-296.jpg]]
114 -
115 -== 3. Node Placement ==
97 +== 2. Node Placement ==
116 116  )))
117 117  
118 118  **Site Analysis**:
119 119  
120 -* **Take compass measurements away from the sensor as it will affect your measurement. Use a stick or shovel to help align.**
121 -* Take photographs from various angles to document the site setup thoroughly. Have a colleague stand next to it pointing at it.
122 -* Include a detailed site description in your notes.
102 +* **Take compass measurements away from the sensor as it will affect your measurement.**
103 +* Take photographs from various angles to document the site setup thoroughly.
104 +* Include a detailed site description in your notes
123 123  
124 -== 4. GPS Considerations ==
106 +== 3. GPS Considerations ==
125 125  
126 126  (% class="wikigeneratedid" %)
127 -The GPS antenna is at the top and center of the unit, and will (usually) only receive signal with a clear sky view directly above. The signal is able to penetrate plastic and terracotta planters and a thin (2 cm?) layer of soil, but may struggle if the soil layer is too thick. **These nodes will not start recording without attaining a GPS lock** and repeated attempts will excessively drain the battery.
109 +The GPS antenna is at the top and center of the unit, and will (usually) only receive signal with a clear sky view directly above. The signal is able to penetrate plastic and terracotta planters and a thin layer of soil, but may struggle if the soil layer is too thick. **These nodes will not start recording without attaining a GPS lock** and repeated attempts will excessively drain the battery.
128 128  
129 -== 5. Visibility and Location Marking ==
111 +== 4. Visibility and Location Marking ==
130 130  
131 131  **Flag Placement**: Position a flag, preferably in a bright color (avoid green or yellow), near the instrument to aid in its future location.
132 132  
133 133  **GPS Marking**:
134 134  
135 -* Use a GPS device to mark the instrument's exact location. Most modern cell phones can get to about a 3m error with their internal GPS also; you can probably also get away with investing a few dollars in a good app that shows error and lets you log markers.
136 -* Also write the GPS down on paper (ie your [[LOG SHEET>>http://auspass.edu.au/field/NODES_blank_fieldlog.pdf]]).
117 +* Use a GPS device to mark the instrument's exact location.
118 +* Record this location in both your paper notes and the GPS device.
137 137  
138 -== (% style="color:inherit; font-family:inherit; font-size:max(18px, min(20px, 14.4444px + 0.462963vw))" %)6. Charge Time, Pre-Deployment & Post-Deployment(%%) ==
120 +== (% style="color:inherit; font-family:inherit; font-size:max(18px, min(20px, 14.4444px + 0.462963vw))" %)5. Charge Time, Pre-Deployment & Post-Deployment(%%) ==
139 139  
140 140  * **Charging Duration**: Both types of nodes take approximately 6-8 hours to fully charge from a flat state.
141 141  * **Pre-Deployment Charging**:
142 142  ** Although the nodes hold their charge well, it's beneficial to give them a "top up" charge before deployment.
125 +
143 143  * **Operational Duration**:
144 144  ** When recording at 250 Hz, with GPS on and Bluetooth disabled, the instruments are expected to last about 30 days per charge cycle. If they are set to run only overnight, this can be extended to 60 days.
145 145  
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154 154  ** Charge levels for transport will be advised by the freighter. The required SoC will depend on volume and transport method (air, land, sea).
155 155  
156 156  (((
157 -== 7. Data Sharing and Metadata Creation ==
140 +== 6. Data Sharing and Metadata Creation ==
158 158  )))
159 159  
160 160  **GPS Data**:
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169 169  
170 170  * Create and organize metadata according to the [[ANU metadata standard txt file>>attach:example_metadata.txt]]. This is going to be particularly important if you are reusing nodes at different sites... not documenting the serial numbers (of the **top half** of the node) and the times they were deployed can lead to station mix-ups.
171 171  
172 -== 8. Additional Best Practices ==
155 +== 7. Additional Best Practices ==
173 173  
174 174  * **Training and Familiarisation**: Make sure all team members are adequately trained in using the GPS devices, compass use, and other equipment to ensure consistent and accurate data collection.
175 175  
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336 336  **Exporting Data in Readable Format**:
337 337  
338 338  * Go to the “Tool” menu and select “export seismic data”.
339 -* Tailor other parameters to project preference and ensure "Sample Interval" matches the setting used during node reset (note: the standard used by ANU is 4ms, or 250hz)
322 +* Tailor other parameters to project preference and ensure "Sample Interval" matches the setting used during node reset.
340 340  * (% class="box warningmessage" %)
341 341  (((
342 342  **Ensure export data is set to "COUNTS" (int32), not "mV" (float). This is critical!**
343 343  )))
344 344  * Set "Remove Gain" to the same decibel gain as during programming. By default ANU sets this to 24db for short period nodes (a scaling factor of 15.848932), and 6db (a factor of 2.0) for broadband nodes.
345 -* Set "Remove DC" to "Yes" to centre the data around the zero value
328 +* Set 'Remove DC' to 'Yes' to centre the data around the zero value
346 346  * Set the correct Start Time (UTC) and End Time (UTC) of the project to prevent the unnecessary export of older data
347 347  * [[image:Smartsolo harvesting #9 copy.png]]
348 348  * Click “prepare” followed by “run” to start reformatting. Monitor this process in the small panel at the bottom left.
349 -* The data will be exported to the SOLODATA folder. For a windows system, the following file explorer page is where you must navigate to to locate your project folder[[image:Smartsolo harvesting #8 copy.png]]
332 +* The data will be exported to the SOLODATA folder. For a windows system, the following file explorer page is where you must navigate to to locate your project folder
350 350  )))
351 351  
352 352  == Smart Solo IGU-16HR Polarity Notice ==
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446 446   'gain':1,
447 447   'sensitivity': 257019225.55108312}
448 448  
449 -[[X axis is samples (.01 s), Y axis is velocity (m/s), 0.5-5 Hz filter>>image:16HR_Z_huddle.png||alt="IGU16_Z_huddle.png"]]
432 +[[X axis is samples (.01 s), Y axis is velocity (m/s), 0.5-5 Hz filter>>image:IGU16_Z_huddle.png]]
450 450  
451 -[[X axis is samples (.01 s), Y axis is velocity (m/s), 0.5-5 Hz bandpass filter>>image:16HR_N_huddle.png||alt="IGU16_N_huddle.png"]]
434 +[[X axis is samples (.01 s), Y axis is velocity (m/s), 0.5-5 Hz bandpass filter>>image:IGU16_N_huddle.png]]
452 452  
453 453  == IGU 16-1C ==
454 454  
455 455  The 1C nodes seem to have the same response as the 3-channel IGU-16HR-3C (above), however the response posted at IRIS-NRL seems to imply that there is no poles and zeros information (e.g. a flat/linear response). This is 100% not so.
456 456  
457 -[[IGU-16 1C, X axis is samples (.01 s), Y axis is velocity (m/s), 0.5-5 Hz bandpass filter. Seems to be same response as IGU-16HR-3C.>>image:16HR1C_Z_huddle.png||alt="IGU16_1C_Z_huddle.png"]]
440 +[[IGU-16 1C, X axis is samples (.01 s), Y axis is velocity (m/s), 0.5-5 Hz bandpass filter. Seems to be same response as IGU-16HR-3C.>>image:IGU16_1C_Z_huddle.png]]
458 458  
459 459  == BD3C-5 ==
460 460  
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470 470  [[X axis is samples (.01 s), Y axis is velocity (m/s), 0.5-5 Hz bandpass filter>>image:BD3C_N_huddle.0.5.png]]
471 471  
472 472  (% class="wikigeneratedid" %)
473 -Below the corner frequency (0.2 Hz) the phase response still fares well, but amplitude response may need to be dialed in a bit (it seems a bit high). We are working to try to calibrate this a bit better. In the next two figures the filter is **0.1** to 5 Hz:
456 +Below the corner frequency (0.2 Hz) the phase response still fares well, but amplitude response may need to be dialed in a bit (it seems a bit high). In the next two figures the filter is **0.1** to 5 Hz:
474 474  
475 475  
476 476  [[BD3C **0.1 **to 5 Hz bandpass filter>>image:BD3C_Z_huddle.0.1.png]]
16HR1C_Z_huddle.png
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XWiki.XWikiComments[0]
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1 -Mark Goldman
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1 -I can verify that the default orientation for the SmartSolo 3C nodes is positive values for case motion to the South, West, and downwards. We have co-located nodes with permanent stations and noticed this correlation when comparing waveforms.
Date
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1 -2026-07-09 10:45:51.967