Changes for page SmartSolo Node Seismometers
Last modified by robert on 2026/02/27 19:58
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... ... @@ -431,14 +431,12 @@ 431 431 432 432 [[X axis is samples (.01 s), Y axis is velocity (m/s), 0.5-5 Hz filter>>image:IGU16_Z_huddle.png]] 433 433 434 -[[X axis is samples (.01 s), Y axis is velocity (m/s), 0.5-5 Hz bandpassfilter>>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]] 435 435 436 436 == IGU 16-1C == 437 437 438 -The 1C nodes seem to have the sameresponse as the 3-channelIGU-16HR-3C (above),howeverthe response posted at IRIS-NRL seems to implythat there is no poles andzerosinformation (e.g. aflat/linear response).This is 100% notso.438 +The 1C nodes seem to have a slightly different response to the 3C (TBA) 439 439 440 -[[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 - 442 442 == BD3C-5 == 443 443 444 444 'BD3C': {'poles':[(-1720.4+0j), (-1.2+0.9j), (-1.2-0.9j)], ... ... @@ -446,31 +446,14 @@ 446 446 'gain':1.69726e-05, 447 447 'sensitivity': 702651512.6046528} 448 448 449 -Ab ove0.5Hz,theBD3C-5responsefitswell:447 +*image TBA but they have been created in the past~-~- we are 100% confident our published responses are correct 450 450 451 - [[Xaxisissamples(.01s),Yaxis isvelocity (m/s), 0.5-5 Hz filter>>image:BD3C_Z_huddle.0.5.png]]449 +== Horizontal noise & how to avoid == 452 452 453 - [[Xaxis issamples(.01s),Yaxisisvelocity(m/s),0.5-5Hzbandpass filter>>image:BD3C_N_huddle.0.5.png]]451 +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. 454 454 455 -(% class="wikigeneratedid" %) 456 -Below the corner frequency 0.2 Hz (5 seconds) the response still does a good job, but may need to be dialed in a bit. In the next two figures the filter is 0.1 to 5 Hz. We are looking into this.. 453 +[[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]] 457 457 458 - 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 - 474 474 = **Cleaning** = 475 475 476 476 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.
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