Pulsars produce regular radio pulses, but the recording available to us is
already sampled, filtered and often folded over many rotations. We inspect a
pulse profile before deciding whether to audify amplitude, trigger an event or
compress time.
Radio intensity over time → remove baseline → identify period → fold repeated
pulses → map amplitude to loudness. Tempo grids are not part of the source
unless the designer adds them.
The ATNF Pulsar Catalogue
provides published pulsar parameters and makes a useful provenance starting
point for the first signal study.
Observation guide 04
Periodicity
Use this page before the slides, then return to the checkpoint after the lab.
After this week, you can
Read a pulsar period and pulse profile without treating either as music.
Explain what folding preserves and what repeated averaging removes.
Compare raw event timing with a folded representation.
Inspectable teaching model
relative radio intensity
0.080.120.760.210.090.100.160.720.250.11
Synthetic intensity bins across two repeated rotations. Values are a teaching model, not an astronomical observation.
Worked notebook
Fold repeated pulses
Synthetic intensity bins across two repeated rotations.
Use five bins as the stated rotation period.
Align the second group of five bins beneath the first.
Average corresponding phase bins to create one folded profile.
Compare the folded peak with the two original pulse heights.
What the method supportsFolding strengthens a stable phase pattern and suppresses differences between rotations. The folded profile cannot show which individual pulse was stronger.
CheckpointWhy would adding a steady drum grid to irregular pulse arrivals create a stronger claim than the source supports?Reveal the reasoning
The grid introduces regular musical timing that was not measured.
A published period supports phase alignment over many rotations. It does not make every detected pulse identical or every arrival free of noise. A drum grid can hide those distinctions.