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Last modified by robert on 2026/06/29 16:42
From version 104.2
edited by robert
on 2026/02/17 12:37
Change comment: There is no comment for this version
To version 110.3
edited by Jack Dent
on 2026/06/15 09:52
Change comment: (Autosaved)

Summary

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1 -XWiki.robert
1 +XWiki.JackD
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6 6  
7 7  ANSIR supply two types of three-channel nodes, and one type of one-channel node:
8 8  
9 -* **SmartSolo IGU 16HR 3C (5 Hz, 'very' short period)**
9 +* **SmartSolo IGU-16HR 3C (5 Hz, 'very' short period)**
10 10  * **SmartSolo BD3C-5 (5 second, short period)**
11 -* **SmartSolo IGU 16 1C (5 Hz, 'very' short period, single channel)**
11 +* **SmartSolo IGU-16 1C (5 Hz, 'very' short period, single channel. Not 'HR')**
12 12  
13 +Visit the [[SmartSolo page>>https://smartsolo.com/igu.html]] for more detail.
14 +
13 13  The three-channel nodes have a theoretical battery capacity of ~~30 days, whereas the single-channel type has a capacity of ~~50 days. The programming, operation and downloading procedures for all types of SmartSolo nodes are also similar.
14 14  
15 15  (% class="box infomessage" %)
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310 310  
311 311  * Once a new project is created, the Data Transfer View panel will display connected nodes with details like series number and data size.
312 312  * If “Prospect not matched” appears, it simply means the new project doesn’t match the original programming project. This is not a concern.
313 -* Select all nodes and right-click to “force download”. This starts the download process.
315 +* Select all nodes and right-click to “force download”. This starts the download process.[[image:Smartsolo harvesting #4 copy.png]]
314 314  * Completed downloads will appear as new folders in the Downloaded Data panel.
315 315  )))
316 316  1. (((
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317 317  **Exporting Data in Readable Format**:
318 318  
319 319  * Go to the “Tool” menu and select “export seismic data”.
320 -* Tailor other parameters to personal preference and ensure "Sample Interval" matches the setting used during node reset.
321 -* Click “prepare” followed by “run” to start reformatting. Monitor this process in the small panel at the bottom left.
322 +* Tailor other parameters to project preference and ensure "Sample Interval" matches the setting used during node reset.
322 322  * (% class="box warningmessage" %)
323 323  (((
324 -* **Ensure to export data as "COUNTS" (int32), not "mV" (float). This is critical!**
325 -
326 -* **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.**
325 +**Ensure export data is set to "COUNTS" (int32), not "mV" (float). This is critical!**
327 327  )))
327 +* 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.
328 +* Set 'Remove DC' to 'Yes' to centre the data around the zero value
329 +* Set the correct Start Time (UTC) and End Time (UTC) of the project to prevent the unnecessary export of older data
330 +* [[image:Smartsolo harvesting #9 copy.png]]
331 +* Click “prepare” followed by “run” to start reformatting. Monitor this process in the small panel at the bottom left.
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
328 328  )))
329 329  
330 330  == Smart Solo IGU-16HR Polarity Notice ==
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391 391  **Finalizing the Download**:
392 392  
393 393  * After downloading, mark the //"D"// box on your temporary labels to indicate completion.
394 -
395 -
396 396  )))
397 397  
398 -[[image:1706153266647-145.png||data-xwiki-image-style-alignment="center" height="340" width="603"]]
399 399  
400 400  
401 401  
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429 429  
430 430  [[X axis is samples (.01 s), Y axis is velocity (m/s), 0.5-5 Hz filter>>image:IGU16_Z_huddle.png]]
431 431  
432 -[[X axis is samples (.01 s), Y axis is velocity (m/s), 0.5-5 Hz filter>>image: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]]
433 433  
434 434  == IGU 16-1C ==
435 435  
436 -The 1C nodes seem to have a slightly different response to the 3C (TBA)
438 +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.
437 437  
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]]
441 +
438 438  == BD3C-5 ==
439 439  
440 440   'BD3C': {'poles':[(-1720.4+0j), (-1.2+0.9j), (-1.2-0.9j)],
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442 442   'gain':1.69726e-05,
443 443   'sensitivity': 702651512.6046528}
444 444  
445 -*image TBA but they have been created in the past~-~- we are 100% confident our published responses are correct
449 +Above 0.5 Hz, the BD3C-5 response fits well:
446 446  
447 -== Horizontal noise & how to avoid ==
451 +[[X axis is samples (.01 s), Y axis is velocity (m/s), 0.5-5 Hz filter>>image:BD3C_Z_huddle.0.5.png]]
448 448  
449 -The 5 Hz nodes are susceptible to horizontal noise due to the placement of geophones in the units, **but this can be mitigated by completely burying the units flush with the ground.** In the below example, the node was set on the floor of our basement set on its plastic carrying case support. As such the amount of horizontal noise noticeably increases above ~~ 10Hz.
453 +[[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]]
450 450  
451 -[[Power spectrum huddle test vs a CMG-6TD (S1) and TC120/Centaur combo. The N and E channels have excess noise above 10Hz due to "sticking up" out of the ground.>>image:IGU16_spectrum.png]]
455 +(% class="wikigeneratedid" %)
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:
452 452  
458 +
459 +[[BD3C **0.1 **to 5 Hz bandpass filter>>image:BD3C_Z_huddle.0.1.png]]
460 +
461 +[[BD3C **0.1** to 5 Hz bandpass filter>>image:BD3C_N_huddle.0.1.png]]
462 +
463 +== IGU-16 Horizontal noise & how to avoid ==
464 +
465 +The** 5 Hz nodes** are susceptible to horizontal noise due to the placement of geophones in the units, **but this can be mitigated by completely burying the units flush with the ground.** In the below example, the node was set on the floor of our basement set on its plastic carrying case support. As such the amount of horizontal noise noticeably increases above ~~ 10Hz.
466 +
467 +[[IGU-16HR-3C Power spectrum huddle test vs a CMG-6TD (S1) and TC120/Centaur combo. The N and E channels have excess noise above 10Hz due to "sticking up" out of the ground.>>image:IGU16_spectrum.png]]
468 +
469 +(% class="wikigeneratedid" %)
470 +The BD3C-5 nodes do not have this issue:
471 +
472 +[[BD3C-5 test, as above. There is no additional noise on the horizontal channels.>>image:BD3C_psd.png]]
473 +
453 453  = **Cleaning** =
454 454  
455 -When assembled, the nodes are water resistant but not submersible. They can handle a good spray and wipe-down. A strong, non-wire brush is helpful to reach areas between the metal spikes on the bottom.
476 +When assembled, the nodes are water resistant but not submersible. They can handle a good spray and wipe-down. A stiff plastic brush is helpful to reach areas between the metal spikes on the bottom.
456 456  
457 457  = **Weights (for shipping)** =
458 458  
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