Math 2.0

Geophysics Definition

Richter magnitude scale

Builds on Natural logarithm

Definition

Let an earthquake be recorded at epicentral distance δ\delta, within local distances of a few hundred kilometres, by a standard Wood–Anderson torsion seismograph. Let AA be the maximum trace amplitude of the record, in millimetres. Let A0(δ)A_0(\delta) be the empirical calibration function of distance, fixed so that an earthquake with A=1A = 1 mm at δ=100\delta = 100 km has magnitude 33. The local or Richter magnitude of the earthquake is ML=log⁡10A−log⁡10A0(δ).M_L = \log_{10} A - \log_{10} A_0(\delta).

Remarks

Equivalently, a magnitude 00 earthquake produces an amplitude of 0.0010.001 mm at 100100 km. Example: an earthquake recorded at 100100 km with A=10A = 10 mm has ML=log⁡1010−log⁡1010−3=1+3=4M_L = \log_{10} 10 - \log_{10} 10^{-3} = 1 + 3 = 4. Non-example: the peak amplitude of an earthquake 50005000 km away is not covered, since A0A_0 is defined only at local distances; teleseismic events use other scales. The value of MLM_L is the average over several stations, each corrected by A0A_0. For large earthquakes the peak amplitude at the short periods of the instrument grows little with size, so MLM_L saturates at about 77. The logarithm is decimal, log⁡10x=ln⁡x/ln⁡10\log_{10} x = \ln x / \ln 10, with ln⁡\ln the natural logarithm.

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Further reading

  1. Web https://en.wikipedia.org/wiki/Richter_scale
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TagRFFQ9A4CA7
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Kinddefinition
WritingW0 stub
MSC86A15
DefinesRichter magnitude scale
UsesNatural logarithm
Changed3 November 2026

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