Datasheet
Advanced triggers
As well as the standard range 
of triggers found on most 
oscilloscopes, the PicoScope 
6000 Series has a built-in set 
of advanced triggers to help 
you capture the data you 
need.
All triggering is digital, resulting in high threshold resolution with 
programmable hysteresis and optimal waveform stability.
Maths channels
With PicoScope 6 you can perform a variety of mathematical 
calculations on your input signals. You can calculate the sum, 
difference, product or inverse, or create your own custom function 
using standard arithmetic, exponential and trigonometric functions.
Automatic measurements
PicoScope allows you to automatically display a table of calculated 
measurements for troubleshooting and analysis. 
Using the built-in measurement statistics you can see the average, 
standard deviation, maximum and minimum of each measurement 
as well as the live value.
You can add as many measurements as you need on each view. Each 
measurement includes statistical parameters showing its variability.
For information on the measurements available in scope 
and spectrum modes, see Automatic  Measurements in the 
Specifications table.
PicoScope 6000 Series PC Oscilloscopes
Digital triggering
Most digital oscilloscopes sold today still use an analog trigger 
architecture based on comparators. This can cause time and 
amplitude errors that cannot always be calibrated out. The use of 
comparators often limits the trigger sensitivity at high bandwidths. 
In 1991 Pico pioneered the use of fully digital triggering using the 
actual digitized data. This technique reduces trigger errors and 
allows our oscilloscopes to trigger on the smallest signals, even 
at the full bandwidth. Trigger levels and hysteresis can be set with 
high precision and resolution.
Digital triggering also reduces re-arm delay and this, combined 
with the segmented memory, allows the triggering and capture of 
events that happen in rapid sequence. At the fastest timebase you 
can use rapid triggering to collect 10,000 waveforms in under 10 
milliseconds. The mask limit testing function can then scan through 
these waveforms to highlight any failed waveforms for viewing in 
the waveform buffer.
11 spectrum mode measurements
15 scope mode measurements
15 scope mode measurements
11 spectrum mode measurements









