Changes for page SmartSolo Node Seismometers
Last modified by robert on 2026/02/27 19:58
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... ... @@ -427,9 +427,9 @@ 427 427 'gain':1, 428 428 'sensitivity': 257019225.55108312} 429 429 430 -[[X axis is samples (.01 s), Y axis is velocity (m/s) , 0.5-5 Hz filter>>image:IGU16_Z_huddle.png]]430 +[[X axis is samples (.01 s), Y axis is velocity (m/s)>>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]]432 +[[X axis is samples (.01 s), Y axis is velocity (m/s)>>image:IGU16_N_huddle.png]] 433 433 434 434 == IGU 16-1C == 435 435 ... ... @@ -448,7 +448,7 @@ 448 448 449 449 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. 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]] 451 +[[Power spectrum huddle test vs a CMG-6TD (S1) and TC120/Centaur combo, all filtered 0.5-5 Hz. The N and E channels have excess noise above 10Hz due to "sticking up" out of the ground.>>image:IGU16_spectrum.png]] 452 452 453 453 = **Cleaning** = 454 454