Telonic TEST

Author: James

  • How to check the version of UltraSpectrum software

    How to check the version of UltraSpectrum software

    How to check the version of UltraSpectrum software

    • Start UltraSigma software
    • Select the spectrum analyser that you wish to control by left-clicking on the instrument ID string
    • Right-click and select UltraSpectrum

    • Select Advanced Operation near the upper-right-hand-side of the window and then select About along the lower tab as shown below:

  • Defective UltraSpectrum display with DSA800 series

    Defective UltraSpectrum display with DSA800 series

    If you experience a defective UltraSpectrum display while connected to a DSA800 series spectrum analyser the most likely cause is due to a UltraSpectrum software version mismatch. Software version  00.01.00.27 corrects the issue and can be downloaded from the blue Downloads tab at:

    https://www.rigolna.com/products/spectrum-analyzers/dsa800/

    Here is an example of the UltraSpectrum display using an incompatible version of software:

  • How can sweep time effect my Spectrum Measurements?

    How can sweep time effect my Spectrum Measurements?

    Spectrum analysers can be used to observe modulated signals. But, some settings may have to be adjusted to observe the signals clearly.
    In this example, we are going to show how the sweep time and selected detector type can effect the displayed data.

    Source: Rigol DG4062 60MHz Dual Channel Arbitrary waveform generator.
    Signal: Sine wave, linear sweep from 230KHz – 270KHz, Sweep frequency of 120Hz (~8ms period)
    From the factory preset default mode, many spectrum analysers such as the Rigol DSA815-TG select an automatic sweep time which is determined by the frequency span and the RBW setting. In this example, we set the DSA to sweep from 150KHz to 600KHz at an RBW of 10KHz. The sweep rate default value for these parameters is 10ms.

    In addition, the DSA815-TG collects 601 frequency “bins” per sweep. This means that the data in each bin is collected at a rate of 16us/point (10ms/601 points).
    In this experiment, note that the modulation period (1/120Hz = 8ms) is much lower than the sweep rate (10ms) of the instrument.

    When the sweep time is faster than the modulation, the data collected per sweep may not accurately represent the total span of the modulation. You can use the “Peak Hold” feature that will display the maximum values for successive scans and hold them on the display.

    The figure below is a Peak Hold Scan for the experimental modulated signal described above. 


    You can see that the sweep time is 10mS.

    Also note that the Yellow scan was collected using a Peak detector and the Pink was collected using an RMS Voltage detector.
    How can the Peak and RMS Voltage detectors give the same trace?
    The scan rate is too fast. This results in very small data sets at each frequency bin and can cause the data collected with different detectors to appear very similar.
    Now, let’s change the sweep rate and observe the differences.

    Here is the same input signal with the sweep time set to 1.5s (Peak Hold Disabled/Trace Clear Write selected):


    You can now see that there are some differences in the Positive Peak Data (Yellow) and the RMS Average Voltage (Pink). This includes some of the modulation peaks and a different noise floor.
    Here is the same input signal with the sweep time set to 5s (Peak Hold Disabled/Trace Clear Write selected):

    Now you can observe quite different traces that more accurately represent the modulated data.

    Here is the same input signal with the sweep rate set to 10s (Peak Hold Disabled/Trace Clear Write selected):

    Conclusions: When observing modulated or pulsed signals, you can use the Peak Hold feature to “build” a trace from successive scans.

    You can also gain more visibility into the signal type by changing the detector, but keep in mind that this may require lengthing the sweep time. This will allow the instrument to collect enough data at each frequency value to make more meaningful measurements.

  • EMI Test System Software Getting Started Guide

    EMI Test System Software Getting Started Guide

    The Rigol EMI Test System Software is designed to make precompliance scanning with a Rigol DSA family of Spectrum Analyzer easy. 

    This Note is an addendum to the Software User’s Guide. We will set up a prescan, create an amplitude correction table, set limit lines, and perform a final scan. 

    Initial Setup: 

    –    Download the latest version of UltraSigma and the EMI Test System Software from the Rigol website. 
    –    Connect your instrument (USB, LAN, or other) and set up the physical test environment (cabling, Device-Under-Test, etc..) 
    –    Start UltraSigma 
    –    USB connected instruments should appear in the UltraSigma Resource tree as shown below: 


    –   Right-click on the resource and select EMI Test System 
      

    –    The EMI Test System will perform a screen grab of the Spectrum Analyzer and open: 
     
          

    Configure Prescan Parameters 
     
    –    Press Edit Scan to open the scan parameters window 
     
     
    –    A Pre Scan consists of subrange elements. You can use the Pre Scan Configure window to set the overall Scan Start, Scan Stop, Range, and Detector type to use throughout the test: 
     
          
    Pre Scan Configuration sets the overall test parameters used in each subrange scan. Using a Positive Peak detector will allow you to perform a faster scan and identify problem areas: 
     
    In this example, we have configured the first subrange to sweep from 9kHz to 10MHz  at an RBW of 1MHz, no attenuation, and no preamplifier. 
     
      
     
    –    Subrange Configuration sets the parameters used for each subrange step: 
     
    In this example, we add a second step that goes from 10MHz to 30MHz in  at an RBW of 300kHz: 
     
      
    Build successive subrange configurations using Range Start and Range Stop values and use the Add, Insert Before, After, and Delete to arrange the scan 
     
    –    Press OK after you have built the Pre Scan list: 
     
      
     
    –    Press Prescan to collect prescan data: 
     
      
          
    After the scan is complete, you should have a graphical display of each subrange stitched together onto one graph: 

      
     
    –    Now you can add amplitude correction by pressing Ampt Corr: 
     
        
    –    You can select Antenna, Cable, Other, or the User tab to specify which correction table to edit.  
     
    –    Enter the frequency point and corresponding  correction level. Press Add to add the correction point to the table. Repeat until the full correction table is built. 
     
    –    To apply a correction table, select the type (Antenna, Cable, Other, or User) from the check boxes and press Correction: 
      
     
    –    You can save the correction files for later use by pressing the Save button. 
     
    You can add limit lines by pressing Peak Search to bring up the Peak Search window: 

          
    –    You can add points to the limit line one-at-a-time by entering the frequency and level, then press add. Here, we have built a limit line comprise of four sections. You can also save the limit lines to recall them later by pressing Save: 
     
      
    –    Use History to recall saved limit lines 
     
    –    Press OK to apply the limit lines 
     
     
    –    All of the peaks that have failed the limit test are shown at the bottom of the display: 
     
          
    –    You can find specific peaks by clicking on the Peak number: 
     
      
    –    You can also change the Vertical and Horizontal Scales by selecting the scales from the Y Unit and X Axis drop down boxes: 
      
     
    –    You can print out a report of scanned data by pressing the Report button and filling in any information that you need. 

     
    –    If you have found areas that fail the limit lines, you can save time by performing another prescan. This time, set the start and stop frequencies to encompass the failing peak(s). 
     
    –    In this more focused scan, you may also want to use a Quasi Peak detector and FCC RBW settings (if your analyser is equipped with those options.

  • DSA800 Prefix: How to more easily save filenames

    DSA800 Prefix: How to more easily save filenames

    The latest revision of firmware (DSA815 00.01.12) has the ability to save a prefix for use with file saves. This can make data entry a bit easier.

    –    Press SYSTEM > Down arrow to page 2 > Select Name Prefix

    –    Select EDIT PREFIX and use the keypad to enter the text you want to start the files with

    –    Press OK

    –    Here, we have saved TEST as the prefix

    –    Set PREFIX SWITCH to ON when you want to use the prefix

    NOTE: You can leave the text box in the numeric control (“1” shown in lower corner) when you close the text entry window. It will appear in the same state next time you save a file. You can simply press 1,2,3..etc.. to increment the file.

  • How do you add a correction file to the S1210 software tool?

    How do you add a correction file to the S1210 software tool?

    Select Tools at the top of the S1210 application window.



    You can now open the Data Manager and select CSV to convert a CSV file into a correction file.

  • How to save a trace as a CSV with the DSA800 Series

    How to save a trace as a CSV with the DSA800 Series

    To save a trace as a CSV: 

    1) Insert USB stick into the USB port on the front panel 
     
    NOTE: The format of the USB stick must be FAT32 
     
    2)    Press STORAGE > Set BROWSER to DIR. You can press the button next to the Browser label to toggle the selection. 
     
     
    NOTE: The spectrum analyzer uses binary files (*.trc) and cannot use CSV files (*.csv) natively. CSV will not be available as a valid format if you are trying to save the file to the local drive (D:) 
     
     
     
    3)    Use the scroll wheel to select Mobile Disk (E:) 
      
           
     
    4)    Change File Type to Trace and press the back arrow to get back to the storage screen 
     
      
     
    5)    Set Format to CSV  
     
      
           
    6)    Press Save, use the keypad to write a filename (I use numbers, they are faster), and press OK 
     
      

  • RSA3000, RSA3000E and RSA5000 Alternative Factory Reset and Firmware Upgrade

    RSA3000, RSA3000E and RSA5000 Alternative Factory Reset and Firmware Upgrade

    To reset the RSA3000, RSA3000E and the RSA5000 series to factory settings without using the System menu:

    1) Power cycle the instrument
    2) During the boot sequence, quickly and repeatedly press the Back button directly below the keypad on the instrument. 


    To upgrade the firmware on the RSA3000, RSA3000E and the RSA5000 series to factory settings without using the System menu:

    1) Power cycle the instrument
    2) Insert a flash drive into the front of the instrument with the latest firmware version loaded onto the root directory of the drive. 
    3) During the boot sequence, quickly and repeatedly press the Preset button in the upper right hand corner of the instrument.

  • RSA3000/3000E/5000 series Open Source Acknowledgment

    RSA3000/3000E/5000 series Open Source Acknowledgment

    RIGOL’s RSA3000/3000E/5000 series product uses a number of open source software packages. This document lists the open source software packages used in RSA3000/3000E/5000 series product. 

    https://beyondmeasure.rigoltech.com/acton/attachment/1579/f-be0541d6-bc36-481f-b448-ec059be1b26e/1/-/-/-/-/RSA3000_3000E_5000.pdf

  • How to save a screen shot on the RSA3000 and RSA5000 series at the push of a button.

    How to save a screen shot on the RSA3000 and RSA5000 series at the push of a button.

    In order to take a screen shot on the RSA5000, RSA3000 or RSA3000E and have it automatically save to your flash drive follow the steps below.
    1) Insert flash drive into the instrument and confirm that you can identify it in the File Explore menu.
    2) Press the Save button
    3) Press Quicksave Path
    4) Press Set Path
    5) Select your flash drive
    6) Press OK.
    This will change the quick save buttons path from saving a screen shot internally to your flash drive.

  • Booting the DSA800 series Spectrum Analysers from a USB memory stick

    Booting the DSA800 series Spectrum Analysers from a USB memory stick

    If your DSA800 series spectrum analyser does not boot when powered up it may be possible to correct the issue by booting off of a USB memory stick.

    When the spectrum analyser is powered on you will see a message at the bottom left corner of the display that says:

    Waiting Input… (Press ‘Preset’ to boot from the U-Disk)

    At this time press the green Preset key on the left side of the display. You will need to do this pretty quick as the message quickly disappears. Once Preset is pressed you should then see a second message that says:

    Testing  U-Disk…(Please Insert U-Disk)

    Now insert the USB memory stick that contains the firmware image in the root directory.

    If successful the spectrum analyser will complete the boot up sequence using the memory stick and the firmware image will be restored on the instrument.

  • S1210 – Using dBuV units successfully

    S1210 – Using dBuV units successfully

    Recent versions of DSA815 Firmware and S1210 software improved the operation of the amplitude units in the software. These versions are:

    Instrument Firmware – 00.01.19

    1210 Software – 05.00.07

    On occasion it is still possible to show a data offset due to changing units such as this:

    This is usually caused by using the instrument from the front panel and setting the amplitude to dBuV manually. The software is expecting the instrument to be in default dBm before it runs. The best way to for data to be correctly processed is to hit the green PRESET button if you have been changing settings on the instrument between software runs.

    With the factory preset active the data is correct in dBuV: