Agilent Technologies ESA-E Series Programmer's Manual page 242

Esa spectrum analyzers
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LINear|LOGarithmi
Sets the frequency interpolation to linear or logarithmic for the
specified correction set.
Remarks:
Front Panel
Access:
Perform Amplitude Correction
[:SENSe]:CORRection:CSET[1]|2|3|4[:STATe] OFF|ON|0|1
[:SENSe]:CORRection:CSET[1]|2|3|4[:STATe]?
Turns the amplitude correction function on or off for the given set.
[:SENSe]:CORRection:CSET:ALL[:STATe] must be on for this command
NOTE
to function.
Factory Preset
and *RST:
Remarks:
Front Panel
Access:
Input Impedance Correction
[:SENSe]:CORRection:IMPedance[:INPut][:MAGNitude] <number>
[:SENSe]:CORRection:IMPedance[:INPut][:MAGNitude]?
Amplitude correction is applied to the display data to adjust for
measurement situations where the unit under test has a different
impedance than the 50Ω input impedance of the analyzer. Some Agilent
ESA analyzers have Option 1DP, 75Ω input. In this case, you may want
to convert the data to make measurements in a 50Ω system.
Chapter 5
Logarithmic frequency scale corrections are linearly
interpolated between correction points with respect to
the logarithm of the frequency. Linear frequency scale
corrections are interpolated along straight lines,
connecting adjacent points on a linear scale.
AMPLITUDE/Y Scale, Corrections, Modify, Freq Interp Log
Lin
Off
CSET number equivalents to front panel access
definitions are as follows:
CSET1 is Antenna
CSET2 is Cable
CSET3 is Other
CSET4 is User
AMPLITUDE/Y Scale, Corrections, Modify, Correction On
Off
Language Reference
SENSe Subsystem
5-87

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