niRFSA_ConfigureResolutionBandwidth
- Updated2025-02-03
- 1 minute(s) read
niRFSA_ConfigureResolutionBandwidth
ViStatus niRFSA_ConfigureResolutionBandwidth(ViSession vi, ViConstString channelList, ViReal64 resolutionBandwidth);
Purpose
Configures the resolution bandwidth of a spectrum acquisition. The resolution bandwidth controls the width of the frequency bins in the power spectrum computed by NI-RFSA. A larger value for resolution bandwidth means the frequency bins are wider, so you get fewer bins, or spectral lines.
By default, the resolution bandwidth value corresponds to the 3 decibels (dB) bandwidth of the window type NI-RFSA uses to compute the spectrum. To directly specify the frequency bin width, set the NIRFSA_ATTR_RESOLUTION_BANDWIDTH_TYPE attribute to NIRFSA_VAL_BIN_WIDTH.
Supported Devices: PXIe-5644/5645/5646, PXI-5661, PXIe-5663/5663E/5665/5667/5668, PXIe-5820/5830/5831/5832/5840/5841/5842/5860
Related Topics
Parameters
Input | ||
Name | Type | Description |
vi | ViSession | Identifies your instrument session. vi is obtained from the niRFSA_init or niRFSA_InitWithOptions function. |
channelList | ViConstString | Identifies which channels to apply settings. Specify an empty string as the value of this parameter. |
resolutionBandwidth | ViReal64 | Specifies the resolution bandwidth of a spectrum acquisition. The value is expressed in hertz (Hz). Configure the type of resolution bandwidth with the NIRFSA_ATTR_RESOLUTION_BANDWIDTH_TYPE attribute. |
Return Value
Name | Type | Description | ||||||||
status | ViStatus | Returns the status code of this operation. The status code either indicates success or describes an error or warning condition. Examine the status code from each call to an NI-RFSA function to determine if an error has occurred. To obtain a text description of the status code and additional information about the error condition, call the niRFSA_GetError function. To clear the error information from NI-RFSA, call the niRFSA_ClearError function. The general meaning of the status code is as follows:
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