Research and learning

1946 observations; 1947 report

Payne-Scott: Timing Solar Bursts

Start with separate radio-frequency receivers, then correct an original three-channel timing fixture and explain why a recorded delay is not automatically a source delay.

Three invented receiver records separate channel delay from corrected arrival time and relative lag.
2 s
Both corrected lags relative to A in the original model

The short answer

Simultaneous observing requires more than three numbers on a chart. Each channel has a route from arriving radiation to a recorded mark, so a timing comparison needs a stated model of that route.

Selected evidence and original reasoning

Recorded and corrected lags

A common clock and known fixed delays are stipulated.

Seconds are relative to the same arbitrary origin.
ChannelRecorded/receiver delayInferred arrival
A10/1 s9 s
B15/4 s11 s
C19/8 s11 s

Chronology

A timeline of the turning points

  1. Separate receiver records

    Solar bursts compared across frequencies.

  2. Timing fixture

    Subtract fixed receiver delays before comparing arrivals.

What was compared

The public abstract describes observations mainly from July and August 1946 at 200, 75 and 60 Mc/s, with a few at 30 Mc/s. Each frequency had a separate receiving system and recording meter. Loudspeakers supplied aural confirmation.

The historical unit Mc/s means millions of cycles per second, the same frequency scale now written MHz. The inspected abstract establishes this multi-channel design; it does not supply every trace or a complete calibration record.

Sources for this section: [1]

An original timing equation

For this fixture define recorded time tแตข=arrival time aแตข+known receiver delay dแตข. Assume one common clock, no clock drift, and exact fixed delays. Invent recorded times 10, 15, 19 seconds for channelsA, B, C, and delays 1, 4, 8 seconds respectively. Channel labels and values are ours, not the historical traces.

Find the arrival times and lags relative to A. Compare them with the raw recorded lags. Which apparent difference disappears after correction?

Sources for this section: [1]

Reference answer

Subtract the delays: a=(9, 11, 11) seconds. Relative to A, the corrected lags are (0, 2, 2) seconds. Raw recorded lags were (0, 5, 9) seconds. B and C were four seconds apart on the recordings but have equal inferred arrival times in this model.

The correction does not make all three arrivals simultaneous: A still precedes the other two by 2 seconds. Nor does equal corrected timing mean equal intensity, shape or source position. Those quantities were not supplied.

Sources for this section: [1]

What an unexplained residual needs

A remaining lag could be investigated only after the assumed clock and receiver behaviour were tested. If delays varied or clocks were offset, the simple subtraction would be inadequate. No propagation speed or coronal height follows from these invented times alone. The task isolates a timing comparison rather than reproducing the historical observation or its full astrophysical interpretation.

Sources for this section: [1]

Continue the chronology

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Quick answers

Common questions

Are the three times from the original paper?
No. The fixture is original; only the selected public abstract was inspected.
Does a corrected lag give a source speed?
Not without a propagation model, geometry and further observations.

Primary and institutional sources

How this history was checked

Selected records ground the historical explanation. Original models have their own stated assumptions. This article was reviewed on 31 October 2026.

  1. Ruby Payne-Scott, D. E. Yabsley, J. G. Bolton, Nature 160, 256โ€“257, 23 August 1947Relative Times of Arrival of Bursts of Solar Noise on Different Radio Frequencies
  2. Colin Ward, CSIROpedia, 2011/updated 2020Ruby Payne-Scott 1912โ€“1981