Changes for page Testing Procedures
Last modified by robert on 2024/12/09 16:08
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... ... @@ -474,7 +474,7 @@ 474 474 475 475 The following sample calibration files are supplied with the Centaur. These files may be used to visually verify functionality and approximate sensitivity of the sensor by inspection of the output waveform: 476 476 477 -* **sine_5V_30s** generates a 1 Hz sine wave with 5 V amplitude lasting 30 seconds. 477 +* **sine_5V_30s** generates a 1 Hz sine wave with 5 V amplitude lasting 30 seconds. **This is the default test for ANU as well as Nanometrics.** 478 478 * **step_0V_to_5V_15s** generates a 0 V signal for 15 seconds followed by a positive 5 V step function lasting 15 seconds. 479 479 * **prb 1V 20ms 10min** generates a 10 minute PRB sequence using 20 ms pulses and 1 V amplitude. 480 480 * **prb 1V 5s 150min** generates a 2.5 hour PRB sequence using 5 second pulses and 1 V amplitude. ... ... @@ -488,7 +488,7 @@ 488 488 1. From the Calibration panel at the top page, select **Type** from the drop-down list and choose Sine. 489 489 1. For the CTR4 series models, additional option to select between Voltage or Current is available. 490 490 1. Click on the **Configure** button to access the calibration dialog box for the selected **Playback**. 491 -1. Configure the signal characteristics by selecting 5V, 30 sec with gain of 1. 491 +1. Configure the signal characteristics by selecting **5V, 30 sec with gain of 1.** 492 492 1. Configure the padding before and after the calibration signal, enter 5 seconds. 493 493 1. The **Duration (s)** time can be made shorter or longer as required by user. NOTE, for shorter frequencies a longer duration will be required for the signal to complete its full cycle and to capture the entire waveform on the screen. 494 494 1. Click OK button to close the dialog box and save the settings. ... ... @@ -517,7 +517,7 @@ 517 517 ))) 518 518 519 519 520 -=== Following materials are required ===520 +=== Following materials are required === 521 521 522 522 * Solar panel for testing 523 523 * Digital multi-meter (DMM) ... ... @@ -527,7 +527,7 @@ 527 527 * Spreadsheet with formulae 528 528 * Marker/ pen 529 529 530 -=== Test Method ===530 +=== Test Method === 531 531 532 532 1. Clearly label each solar panel to keep track of measurements. 533 533 1. Record the manufacturers power rating of the solar panel. **Perform all measurement outdoors under bright sunny conditions! ** ... ... @@ -542,7 +542,7 @@ 542 542 543 543 544 544 545 -=== Developing a spreadsheet ===545 +=== Developing a spreadsheet === 546 546 547 547 Create a spreadsheet with following cells 548 548 ... ... @@ -624,17 +624,15 @@ 624 624 625 625 Inside the “Vrl (Theoretical)” cell enter the following formula using the corresponding cells. 626 626 627 - V_{RL}=I_{oc}\timesR_L627 +[[image:Screenshot 2024-12-09 103334.png||height="28" width="141"]] 628 628 629 - 630 630 Inside the “Rated Power” cell enter the following formula using the corresponding cells. 631 631 632 - P_{oc}=V_{oc}\timesI_{oc}631 +[[image:Screenshot 2024-12-09 103419.png||height="31" width="157"]] 633 633 634 - 635 635 Inside the “Load Power” cell enter the following formula using the corresponding cells. 636 636 637 - P_{RL}=\frac{V_{RL}}{R_L}\timesV_{oc}635 +[[image:Screenshot 2024-12-09 103432.png||height="67" width="176"]] 638 638 639 639 640 640 Inside the “Power Loss %” cell enter the following formula using the corresponding cells. ... ... @@ -641,10 +641,9 @@ 641 641 642 642 The calculated values that are negative represent power loss, and positive values are power gain. Performing “conditional formatting” on these cells with colour gradient (defined by colour break limits) would yield visually easy to recognise defective panels. 643 643 642 +[[image:Screenshot 2024-12-09 103639.png||height="63" width="304"]] 644 644 645 -Power\ Loss\ \%=\frac{P_{RL}}{P_{oc}}\times 100-100 646 646 647 - 648 648 Perform all the calculations for each solar panel ID entered. 649 649 650 650 Solar panels with power loss of 20% or more should be clearly marked as defective and not be used in any future deployments.
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