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The '''Richter magnitude scale''' (also '''Richter scale''', ''M''<sub>L</sub>) assigns a magnitude number to quantify the size of an ]. The Richter scale, developed in the 1930s, is a ] ], which defines magnitude as the logarithm of the ratio of the ] of the ]s to an arbitrary, minor amplitude, as recorded on a standardized ] at a standard distance. The '''Richter magnitude scale''' (also '''Richter scale''') assigns a magnitude number to quantify the size of an ]. The Richter scale, developed in the 1930s, is a ] ], which defines magnitude as the logarithm of the ratio of the ] of the ]s to an arbitrary, minor amplitude, as recorded on a standardized ] at a standard distance.


As measured with a ], an earthquake that registers 5.0 on the Richter scale has a shaking amplitude 10 times greater than an earthquake that registered 4.0 at the same distance. As energy release is generally proportional to the shaking amplitude raised to the 3/2 power, an increase of 1 magnitude corresponds to a release of energy 31.6 times that released by the lesser earthquake.<ref name=USGS></ref> This means that, for instance, an earthquake of magnitude 5 releases 31.6 times as much energy as an earthquake of magnitude 4. As measured with a ], an earthquake that registers 5.0 on the Richter scale has a shaking amplitude 10 times greater than an earthquake that registered 4.0 at the same distance. As energy release is generally proportional to the shaking amplitude raised to the 3/2 power, an increase of 1 magnitude corresponds to a release of energy 31.6 times that released by the lesser earthquake.<ref name=USGS></ref> This means that, for instance, an earthquake of magnitude 5 releases 31.6 times as much energy as an earthquake of magnitude 4.

Revision as of 00:23, 23 June 2017

The Richter magnitude scale (also Richter scale) assigns a magnitude number to quantify the size of an earthquake. The Richter scale, developed in the 1930s, is a base-10 logarithmic scale, which defines magnitude as the logarithm of the ratio of the amplitude of the seismic waves to an arbitrary, minor amplitude, as recorded on a standardized seismograph at a standard distance.

As measured with a seismometer, an earthquake that registers 5.0 on the Richter scale has a shaking amplitude 10 times greater than an earthquake that registered 4.0 at the same distance. As energy release is generally proportional to the shaking amplitude raised to the 3/2 power, an increase of 1 magnitude corresponds to a release of energy 31.6 times that released by the lesser earthquake. This means that, for instance, an earthquake of magnitude 5 releases 31.6 times as much energy as an earthquake of magnitude 4.

  • Magnitude 3 = 2 gigajoules
  • Magnitude 4 = 63 gigajoules
  • Magnitude 5 = 2 terajoules
  • Magnitude 6 = 63 terajoules
  • Magnitude 7 = 2 petajoules

The Richter scale built on the previous, more subjective Mercalli scale by offering a quantifiable measure of an earthquake's size.

In the United States, the Richter scale was succeeded in the 1970s by the moment magnitude scale. The moment magnitude scale is now the scale used by the United States Geological Survey to estimate magnitudes for all modern large earthquakes.

Development

Charles Francis Richter, circa 1970

In 1935, seismologists Charles Francis Richter and Beno Gutenberg of the California Institute of Technology developed a scale, later dubbed the Richter magnitude scale, for computing the magnitude of earthquakes, specifically those recorded and measured with the Wood-Anderson torsion seismograph in a particular area of California. Originally, Richter reported mathematical values to the nearest quarter of a unit, but the values later were reported with one decimal place; the local magnitude scale compared the magnitudes of different earthquakes. Richter derived his earthquake-magnitude scale from the apparent magnitude scale used to measure the brightness of stars.

Richter established a magnitude 0 event to be an earthquake that would show a maximum, combined horizontal displacement of 1.0 µm (0.00004 in.) on a seismogram recorded with a Wood-Anderson torsion seismograph 100 km (62 mi.) from the earthquake epicenter. That fixed measure was chosen to avoid negative values for magnitude, given that the slightest earthquakes that could be recorded and located at the time were around magnitude 3.0. The Richter magnitude scale itself has no lower limit, and contemporary seismometers can register, record, and measure earthquakes with negative magnitudes.

M L {\displaystyle M_{\text{L}}} (local magnitude) was not designed to be applied to data with distances to the hypocenter of the earthquake that were greater than 600 km (373 mi.). For national and local seismological observatories, the standard magnitude scale in the 21st century is still M L {\displaystyle M_{\text{L}}} . However, this scale cannot measure magnitudes above about M L {\displaystyle M_{\text{L}}} = 7, because the high frequency waves recorded locally have wavelengths shorter than the rupture lengths of large earthquakes.

Later, to express the size of earthquakes around the planet, Gutenberg and Richter developed a surface wave magnitude scale ( M s {\displaystyle M_{\text{s}}} ) and a body wave magnitude scale ( M b {\displaystyle M_{\text{b}}} ). These are types of waves that are recorded at teleseismic distances. The two scales were adjusted such that they were consistent with the M L {\displaystyle M_{\text{L}}} scale. That adjustment succeeded better with the M s {\displaystyle M_{\text{s}}} scale than with the M b {\displaystyle M_{\text{b}}} scale. Each scale saturates when the earthquake is greater than magnitude 8.0.

Because of this, researchers in the 1970s developed the moment magnitude scale ( M w {\displaystyle M_{\text{w}}} ). The older magnitude-scales were superseded by methods for calculating the seismic moment, from which was derived the moment magnitude scale.

About the origins of the Richter magnitude scale, C.F. Richter said:

I found a paper by Professor K. Wadati of Japan in which he compared large earthquakes by plotting the maximum ground motion against distance to the epicenter. I tried a similar procedure for our stations, but the range between the largest and smallest magnitudes seemed unmanageably large. Dr. Beno Gutenberg then made the natural suggestion to plot the amplitudes logarithmically. I was lucky, because logarithmic plots are a device of the devil.

— Charles Richter Interview, abridged from the Earthquake Information Bulletin, Vol. 12, No. 1, January-February, 1980.

Details

The Richter scale was defined in 1935 for particular circumstances and instruments; the particular circumstances refer to it being defined for Southern California and "implicitly incorporates the attenuative properties of Southern California crust and mantle." The particular instrument used would become saturated by strong earthquakes and unable to record high values. The scale was replaced in the 1970s by the moment magnitude scale (MMS); for earthquakes adequately measured by the Richter scale, numerical values are approximately the same. Although values measured for earthquakes now are M w {\displaystyle M_{w}} (MMS), they are frequently reported by the press as Richter values, even for earthquakes of magnitude over 8, when the Richter scale becomes meaningless. Anything above 5 is classified as a risk by the USGS.

The Richter and MMS scales measure the energy released by an earthquake; another scale, the Mercalli intensity scale, classifies earthquakes by their effects, from detectable by instruments but not noticeable, to catastrophic. The energy and effects are not necessarily strongly correlated; a shallow earthquake in a populated area with soil of certain types can be far more intense in effects than a much more energetic deep earthquake in an isolated area.

Several scales have historically been described as the "Richter scale", especially the local magnitude M L {\displaystyle M_{\text{L}}} and the surface wave M s {\displaystyle M_{\text{s}}} scale. In addition, the body wave magnitude, m b {\displaystyle m_{\text{b}}} , and the moment magnitude, M w {\displaystyle M_{\text{w}}} , abbreviated MMS, have been widely used for decades. A couple of new techniques to measure magnitude are in the development stage by seismologists.

All magnitude scales have been designed to give numerically similar results. This goal has been achieved well for M L {\displaystyle M_{\text{L}}} , M s {\displaystyle M_{\text{s}}} , and M w {\displaystyle M_{\text{w}}} . The m b {\displaystyle m_{\text{b}}} scale gives somewhat different values than the other scales. The reason for so many different ways to measure the same thing is that at different distances, for different hypocentral depths, and for different earthquake sizes, the amplitudes of different types of elastic waves must be measured.

M L {\displaystyle M_{\text{L}}} is the scale used for the majority of earthquakes reported (tens of thousands) by local and regional seismological observatories. For large earthquakes worldwide, the moment magnitude scale (MMS) is most common, although M s {\displaystyle M_{\text{s}}} is also reported frequently.

The seismic moment, M o {\displaystyle M_{o}} , is proportional to the area of the rupture times the average slip that took place in the earthquake, thus it measures the physical size of the event. M w {\displaystyle M_{\text{w}}} is derived from it empirically as a quantity without units, just a number designed to conform to the M s {\displaystyle M_{\text{s}}} scale. A spectral analysis is required to obtain M o {\displaystyle M_{o}} , whereas the other magnitudes are derived from a simple measurement of the amplitude of a specifically defined wave.

All scales, except M w {\displaystyle M_{\text{w}}} , saturate for large earthquakes, meaning they are based on the amplitudes of waves which have a wavelength shorter than the rupture length of the earthquakes. These short waves (high frequency waves) are too short a yardstick to measure the extent of the event. The resulting effective upper limit of measurement for M L {\displaystyle M_{L}} is about 7 and about 8.5 for M s {\displaystyle M_{\text{s}}} .

New techniques to avoid the saturation problem and to measure magnitudes rapidly for very large earthquakes are being developed. One of these is based on the long period P-wave; the other is based on a recently discovered channel wave.

The energy release of an earthquake, which closely correlates to its destructive power, scales with the 3⁄2 power of the shaking amplitude. Thus, a difference in magnitude of 1.0 is equivalent to a factor of 31.6 ( = ( 10 1.0 ) ( 3 / 2 ) {\displaystyle =({10^{1.0}})^{(3/2)}} ) in the energy released; a difference in magnitude of 2.0 is equivalent to a factor of 1000 ( = ( 10 2.0 ) ( 3 / 2 ) {\displaystyle =({10^{2.0}})^{(3/2)}} ) in the energy released. The elastic energy radiated is best derived from an integration of the radiated spectrum, but an estimate can be based on m b {\displaystyle m_{\text{b}}} because most energy is carried by the high frequency waves.

Richter magnitudes

The Richter magnitude of an earthquake is determined from the logarithm of the amplitude of waves recorded by seismographs (adjustments are included to compensate for the variation in the distance between the various seismographs and the epicenter of the earthquake). The original formula is:

M L = log 10 A log 10 A 0 ( δ ) = log 10 [ A / A 0 ( δ ) ] ,   {\displaystyle M_{\mathrm {L} }=\log _{10}A-\log _{10}A_{\mathrm {0} }(\delta )=\log _{10},\ }

where A is the maximum excursion of the Wood-Anderson seismograph, the empirical function A0 depends only on the epicentral distance of the station, δ {\displaystyle \delta } . In practice, readings from all observing stations are averaged after adjustment with station-specific corrections to obtain the M L {\displaystyle M_{\text{L}}} value.

Because of the logarithmic basis of the scale, each whole number increase in magnitude represents a tenfold increase in measured amplitude; in terms of energy, each whole number increase corresponds to an increase of about 31.6 times the amount of energy released, and each increase of 0.2 corresponds to a doubling of the energy released.

Events with magnitudes greater than 4.5 are strong enough to be recorded by a seismograph anywhere in the world, so long as its sensors are not located in the earthquake's shadow.

The following describes the typical effects of earthquakes of various magnitudes near the epicenter. The values are typical only. They should be taken with extreme caution, since intensity and thus ground effects depend not only on the magnitude, but also on the distance to the epicenter, the depth of the earthquake's focus beneath the epicenter, the location of the epicenter and geological conditions (certain terrains can amplify seismic signals).

Magnitude Description Mercalli intensity Average earthquake effects Average frequency of occurrence (estimated)
1.0–1.9 Micro I Microearthquakes, not felt, or felt rarely. Recorded by seismographs. Continual/several million per year
2.0–2.9 Minor I to II Felt slightly by some people. No damage to buildings. Over one million per year
3.0–3.9 III to IV Often felt by people, but very rarely causes damage. Shaking of indoor objects can be noticeable. Over 100,000 per year
4.0–4.9 Light IV to VI Noticeable shaking of indoor objects and rattling noises. Felt by most people in the affected area. Slightly felt outside. Generally causes none to minimal damage. Moderate to significant damage very unlikely. Some objects may fall off shelves or be knocked over. 10,000 to 15,000 per year
5.0–5.9 Moderate VI to VII Can cause damage of varying severity to poorly constructed buildings. At most, none to slight damage to all other buildings. Felt by everyone. 1,000 to 1,500 per year
6.0–6.9 Strong VIII to X Damage to a moderate number of well-built structures in populated areas. Earthquake-resistant structures survive with slight to moderate damage. Poorly designed structures receive moderate to severe damage. Felt in wider areas; up to hundreds of miles/kilometers from the epicenter. Strong to violent shaking in epicentral area. 100 to 150 per year
7.0–7.9 Major X or greater Causes damage to most buildings, some to partially or completely collapse or receive severe damage. Well-designed structures are likely to receive damage. Felt across great distances with major damage mostly limited to 250 km from epicenter. 10 to 20 per year
8.0–8.9 Great Major damage to buildings, structures likely to be destroyed. Will cause moderate to heavy damage to sturdy or earthquake-resistant buildings. Damaging in large areas. Felt in extremely large regions. One per year
9.0 and greater At or near total destruction – severe damage or collapse to all buildings. Heavy damage and shaking extends to distant locations. Permanent changes in ground topography. One per 10 to 50 years

(Based on U.S. Geological Survey documents.)

The intensity and death toll depend on several factors (earthquake depth, epicenter location, population density, to name a few) and can vary widely.

Minor earthquakes occur every day and hour. On the other hand, great earthquakes occur once a year, on average. The largest recorded earthquake was the Great Chilean earthquake of May 22, 1960, which had a magnitude of 9.5 on the moment magnitude scale. The larger the magnitude, the less frequent the earthquake happens.

Beyond 9.5, while extremely strong earthquakes are theoretically possible, the energies involved rapidly make such earthquakes on Earth effectively impossible without an extremely destructive source of external energy. For example, the asteroid impact that created the Chicxulub crater and caused the mass extinction that may have killed the dinosaurs has been estimated as causing a magnitude 13 earthquake (see below), while a magnitude 15 earthquake could destroy the Earth completely. Seismologist Susan Hough has suggested that 10 may represent a very approximate upper limit, as the effect if the largest known continuous belt of faults ruptured together (along the Pacific coast of the Americas).

Energy release equivalents

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The following table lists the approximate energy equivalents in terms of TNT explosive force – though note that the earthquake energy is released underground rather than overground. Most energy from an earthquake is not transmitted to and through the surface; instead, it dissipates into the crust and other subsurface structures. In contrast, a small atomic bomb blast (see nuclear weapon yield) will not, it will simply cause light shaking of indoor items, since its energy is released above ground.

Approximate magnitude Approximate TNT equivalent for
seismic energy yield
Joule equivalent Example
0.0 15 g 63 kJ
0.2 30 g 130 kJ Large hand grenade
1.5 2.7 kg 11 MJ Seismic impact of typical small construction blast
2.1 21 kg 89 MJ West fertilizer plant explosion
3.0 480 kg 2.0 GJ Oklahoma City bombing, 1995
3.5 2.7 metric tons 11 GJ PEPCON fuel plant explosion, Henderson, Nevada, 1988
3.87 9.5 metric tons 40 GJ Explosion at Chernobyl nuclear power plant, 1986
3.91 11 metric tons 46 GJ Massive Ordnance Air Blast bomb
6.0 15 kilotons 63 TJ Approximate yield of the Little Boy atomic bomb dropped on Hiroshima (~16 kt)
7.9 10.7 megatons 45 PJ Tunguska event
8.35 50 megatons 210 PJ Tsar Bomba—Largest thermonuclear weapon ever tested. Most of the energy was dissipated in the atmosphere. The seismic shock was estimated at 5.0–5.2
9.15 800 megatons 3.3 EJ Toba eruption 75,000 years ago; among the largest known volcanic events.
13.0 100 teratons 420 ZJ Yucatán Peninsula impact (creating Chicxulub crater) 65 Ma ago (10 megatons; over 4×10 ergs = 400 ZJ).

Magnitude empirical formulae

These formulae for Richter magnitude M L {\displaystyle \textstyle M_{\mathrm {L} }} are alternatives to using Richter correlation tables based on Richter standard seismic event ( M L {\displaystyle M_{\mathrm {L} }} =0, A=0.001mm, D=100 km). Below, Δ {\displaystyle \textstyle \Delta } is the epicentral distance (in kilometers unless otherwise specified).

The Lillie empirical formula:

M L = log 10 A 2.48 + 2.76 log 10 Δ , {\displaystyle M_{\mathrm {L} }=\log _{10}A-2.48+2.76\log _{10}\Delta ,}

Where A {\displaystyle A} is the amplitude (maximum ground displacement) of the P-wave, in micrometers, measured at 0.8 Hz.

For distances D {\displaystyle D} less than 200 km,

M L = log 10 A + 1.6 log 10 D 0.15 , {\displaystyle M_{\mathrm {L} }=\log _{10}A+1.6\log _{10}D-0.15,}

and for distances between 200 km and 600 km,

M L = log 10 A + 3.0 log 10 D 3.38 , {\displaystyle M_{\mathrm {L} }=\log _{10}A+3.0\log _{10}D-3.38,}

where A {\displaystyle A} is seismograph signal amplitude in mm and D {\displaystyle D} is in km.

The Bisztricsany (1958) empirical formula for epicentral distances between 4˚ to 160˚:

M L = 2.92 + 2.25 log 10 ( τ ) 0.001 Δ , {\displaystyle M_{\mathrm {L} }=2.92+2.25\log _{10}(\tau )-0.001\Delta ^{\circ },}

Where τ {\displaystyle \tau } is the duration of the surface wave in seconds, and Δ {\displaystyle \Delta } is in degrees. M L {\displaystyle M_{\mathrm {L} }} is mainly between 5 and 8.

The Tsumura empirical formula:

M L = 2.53 + 2.85 log 10 ( F P ) + 0.0014 Δ {\displaystyle M_{\mathrm {L} }=-2.53+2.85\log _{10}(F-P)+0.0014\Delta ^{\circ }}

Where F P {\displaystyle F-P} is the total duration of oscillation in seconds. M L {\displaystyle M_{\mathrm {L} }} is mainly between 3 and 5.

The Tsuboi, University of Tokyo, empirical formula:

M L = log 10 A + 1.73 log 10 Δ 0.83 {\displaystyle M_{\mathrm {L} }=\log _{10}A+1.73\log _{10}\Delta -0.83}

Where A {\displaystyle A} is the amplitude in micrometers.

See also

References

  1. ^ The Richter Magnitude Scale
  2. ^ Richter, C.F. (1935). "An instrumental earthquake magnitude scale" (PDF). Bulletin of the Seismological Society of America. 25 (1–2). Seismological Society of America: 1–32.
  3. ^ "USGS Earthquake Magnitude Policy (implemented on January 18, 2002)". United States Geological Survey. January 30, 2014.
  4. Reitherman, Robert (2012). Earthquakes and Engineers: An International History. Reston, VA: ASCE Press. pp. 208–209. ISBN 9780784410714.
  5. ^ Woo, Wang-chun (September 2012). "On Earthquake Magnitudes". Hong Kong Observatory. Retrieved December 18, 2013.
  6. William L. Ellsworth (1991). "SURFACE-WAVE MAGNITUDE ( M s {\displaystyle M_{\text{s}}} ) AND BODY-WAVE MAGNITUDE (mb)". USGS. Retrieved September 14, 2008. {{cite journal}}: Cite journal requires |journal= (help)
  7. "Explanation of Bulletin Listings, USGS".
  8. Richter, C.F., "Elementary Seismology", ed, Vol., W. H. Freeman and Co., San Francisco, 1956.
  9. Hanks, T. C. and H. Kanamori, 1979, "Moment magnitude scale", Journal of Geophysical Research, 84, B5, 2348.
  10. "Richter scale". Glossary. USGS. March 31, 2010.
  11. Di Giacomo, D., Parolai, S., Saul, J., Grosser, H., Bormann, P., Wang, R. & Zschau, J., 2008. "Rapid determination of the energy magnitude Me," in European Seismological Commission 31st General Assembly, Hersonissos.
  12. Rivera, L. & Kanamori, H., 2008. "Rapid source inversion of W phase for tsunami warning," in European Geophysical Union General Assembly, pp. A-06228, Vienna.
  13. Marius Vassiliou and Hiroo Kanamori (1982): "The Energy Release in Earthquakes," Bull. Seismol. Soc. Am. 72, 371-387.
  14. "Measuring the Size of an Earthquake". Earthquakes and Volcanoes. 21 (1). 1989. {{cite journal}}: Unknown parameter |authors= ignored (help)
  15. Ellsworth, William L. (1991). "The Richter Scale M L {\displaystyle M_{\text{L}}} , from The San Andreas Fault System, California (Professional Paper 1515)". USGS: c6, p177. Retrieved September 14, 2008. {{cite journal}}: Cite journal requires |journal= (help)
  16. This is what Richter wrote in his Elementary Seismology (1958), an opinion copiously reproduced afterwards in Earth's science primers. Recent evidence shows that earthquakes with negative magnitudes (down to −0.7) can also be felt in exceptional cases, especially when the focus is very shallow (a few hundred metres). See: Thouvenot, F.; Bouchon, M. (2008). "What is the lowest magnitude threshold at which an earthquake can be felt or heard, or objects thrown into the air?," in Fréchet, J., Meghraoui, M. & Stucchi, M. (eds), Modern Approaches in Solid Earth Sciences (vol. 2), Historical Seismology: Interdisciplinary Studies of Past and Recent Earthquakes, Springer, Dordrecht, 313–326.
  17. "Anchorage, Alaska (AK) profile: population, maps, real estate, averages, homes, statistics, relocation, travel, jobs, hospitals, schools, crime, moving, houses, news". City-Data.com. Retrieved October 12, 2012.
  18. "Earthquake Facts and Statistics". United States Geological Survey. November 29, 2012. Retrieved December 18, 2013.
  19. "Largest Earthquakes in the World Since 1900". November 30, 2012. Retrieved December 18, 2013.
  20. Silver, Nate (2013). The signal and the noise : the art and science of prediction. London: Penguin. ISBN 9780141975658.
  21. Usgs Faqs (January 15, 2014). "FAQs – Measuring Earthquakes". Earthquake.usgs.gov. Retrieved February 16, 2014.
  22. "2.1 Explosion - 1km NNE of West, Texas (BETA)". United States Geological Survey. June 19, 2013. Retrieved December 18, 2013.
  23. "The Tsar Bomba ("King of Bombs")". Retrieved July 6, 2014.
  24. Petraglia, M.; R. Korisettar, N. Boivin, C. Clarkson,4 P. Ditchfield,5 S. Jones,6 J. Koshy,7 M.M. Lahr,8 C. Oppenheimer,9 D. Pyle,10 R. Roberts,11 J.-C. Schwenninger,12 L. Arnold,13 K. White. (6 July 2007). "Middle Paleolithic Assemblages from the Indian Subcontinent Before and After the Toba Super-eruption". Science 317 (5834): 114–116. doi:10.1126/science.1141564. PMID 17615356.
  25. Bralower, Timothy J.; Charles K. Paull; R. Mark Leckie (1998). "The Cretaceous-Tertiary boundary cocktail: Chicxulub impact triggers margin collapse and extensive sediment gravity flows" (PDF). Geology. 26: 331–334. Bibcode:1998Geo....26..331B. doi:10.1130/0091-7613(1998)026<0331:TCTBCC>2.3.CO;2. ISSN 0091-7613. Retrieved September 3, 2009.
  26. Klaus, Adam; Norris, Richard D.; Kroon, Dick; Smit, Jan (2000). "Impact-induced mass wasting at the K-T boundary: Blake Nose, western North Atlantic". Geology. 28: 319–322. Bibcode:2000Geo....28..319K. doi:10.1130/0091-7613(2000)28<319:IMWATK>2.0.CO;2. ISSN 0091-7613.
  27. Busby, Cathy J.; Grant Yip; Lars Blikra; Paul Renne (2002). "Coastal landsliding and catastrophic sedimentation triggered by Cretaceous-Tertiary bolide impact: A Pacific margin example?". Geology. 30: 687–690. Bibcode:2002Geo....30..687B. doi:10.1130/0091-7613(2002)030<0687:CLACST>2.0.CO;2. ISSN 0091-7613.
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  29. Simkin, Tom; Robert I. Tilling; Peter R. Vogt; Stephen H. Kirby; Paul Kimberly; David B. Stewart (2006). "This dynamic planet. World map of volcanoes, earthquakes, impact craters, and plate tectonics. Inset VI. Impacting extraterrestrials scar planetary surfaces" (PDF). U.S. Geological Survey. Retrieved September 3, 2009.
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External links

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