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Last modified by robert on 2026/06/29 16:42
From version 110.2
edited by Jack Dent
on 2026/06/15 09:47
Change comment: (Autosaved)
To version 106.1
edited by robert
on 2026/02/17 16:18
Change comment: There is no comment for this version

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1 -XWiki.JackD
1 +XWiki.robert
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312 312  
313 313  * Once a new project is created, the Data Transfer View panel will display connected nodes with details like series number and data size.
314 314  * If “Prospect not matched” appears, it simply means the new project doesn’t match the original programming project. This is not a concern.
315 -* Select all nodes and right-click to “force download”. This starts the download process.[[image:Smartsolo harvesting #4 copy.png]]
315 +* Select all nodes and right-click to “force download”. This starts the download process.
316 316  * Completed downloads will appear as new folders in the Downloaded Data panel.
317 317  )))
318 318  1. (((
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319 319  **Exporting Data in Readable Format**:
320 320  
321 321  * Go to the “Tool” menu and select “export seismic data”.
322 -* Tailor other parameters to project preference and ensure "Sample Interval" matches the setting used during node reset.
323 -* **Ensure export data is set to "COUNTS" (int32), not "mV" (float). This is critical!**
324 -* 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 -Set 'Remove DC' to 'Yes' to centre the data around the zero value
326 -Set the correct Start Time (UTC) and End Time (UTC) of the project to prevent the unnecessary export of older data
327 -* [[image:Smartsolo harvesting #9 copy.png]]
322 +* Tailor other parameters to personal preference and ensure "Sample Interval" matches the setting used during node reset.
323 +* Click “prepare” followed by “run” to start reformatting. Monitor this process in the small panel at the bottom left.
328 328  * (% class="box warningmessage" %)
329 329  (((
330 -
331 -)))Click “prepare” followed by “run” to start reformatting. Monitor this process in the small panel at the bottom left.
326 +* **Ensure to export data as "COUNTS" (int32), not "mV" (float). This is critical!**
327 +
328 +* **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.**
332 332  )))
330 +)))
333 333  
334 334  == Smart Solo IGU-16HR Polarity Notice ==
335 335  
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395 395  **Finalizing the Download**:
396 396  
397 397  * After downloading, mark the //"D"// box on your temporary labels to indicate completion.
396 +
397 +
398 398  )))
399 399  
400 +[[image:1706153266647-145.png||data-xwiki-image-style-alignment="center" height="340" width="603"]]
400 400  
401 401  
402 402  
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430 430  
431 431  [[X axis is samples (.01 s), Y axis is velocity (m/s), 0.5-5 Hz filter>>image:IGU16_Z_huddle.png]]
432 432  
433 -[[X axis is samples (.01 s), Y axis is velocity (m/s), 0.5-5 Hz bandpass filter>>image:IGU16_N_huddle.png]]
434 +[[X axis is samples (.01 s), Y axis is velocity (m/s), 0.5-5 Hz filter>>image:IGU16_N_huddle.png]]
434 434  
435 435  == IGU 16-1C ==
436 436  
437 -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.
438 +The 1C nodes seem to have a slightly different response to the 3C, but the 3C version seems to fit a lot better than the version published at IRIS-NRL which has no PAZ information. We are looking into this.
438 438  
439 -[[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]]
440 -
441 441  == BD3C-5 ==
442 442  
443 443   'BD3C': {'poles':[(-1720.4+0j), (-1.2+0.9j), (-1.2-0.9j)],
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445 445   'gain':1.69726e-05,
446 446   'sensitivity': 702651512.6046528}
447 447  
448 -Above 0.5 Hz, the BD3C-5 response fits well:
447 +[[X axis is samples (.01 s), Y axis is velocity (m/s), 0.5-5 Hz filter>>image:BD3C_Z_huddle.png]]
449 449  
450 -[[X axis is samples (.01 s), Y axis is velocity (m/s), 0.5-5 Hz filter>>image:BD3C_Z_huddle.0.5.png]]
449 +[[X axis is samples (.01 s), Y axis is velocity (m/s), 0.5-5 Hz filter>>image:BD3C_N_huddle.png]]
451 451  
452 -[[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]]
451 +(% class="wikigeneratedid" %)
452 +Below the corner frequency 0.2 Hz (i.e. 5 seconds) the response still does a good job, but may need to be dialed in a bit. We are looking into this.
453 453  
454 454  (% class="wikigeneratedid" %)
455 -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:
455 +
456 456  
457 +[[BD3C 0.1 to 5 Hz bandpass>>image:BD3C_Z_huddle.0.1.png]]
457 457  
458 -[[BD3C **0.1 **to 5 Hz bandpass filter>>image:BD3C_Z_huddle.0.1.png]]
459 +[[BD3C 0.1 to 5 Hz bandpass>>image:BD3C_N_huddle.0.1.png]]
459 459  
460 -[[BD3C **0.1** to 5 Hz bandpass filter>>image:BD3C_N_huddle.0.1.png]]
461 -
462 462  == IGU-16 Horizontal noise & how to avoid ==
463 463  
464 -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.
463 +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.
465 465  
466 466  [[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]]
467 467  
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