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The so-called Richter magnitude scale - more accurately, Richter's magnitude scale, or just Richter magnitude - for measuring the strength ("size") of earthquakes refers to the original "magnitude scale" developed by Charles F. Richter and presented in his landmark 1935 paper, and later revised and renamed the Local magnitude scale, denoted as "ML" or "M_L". Because of various shortcomings of the ML scale most seismological authorities now use other scales, such as the moment magnitude scale (M_w), to report earthquake magnitudes, but much of the news media still refers to these as "Richter" magnitudes. All magnitude scales retain the logarithmic character of the original, and are scaled to have roughly comparable numeric values.

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Development

Prior to the development of the magnitude scale the only measure of an earthquake's strength or "size" was a subjective assessment of the intensity of shaking observed near the epicenter of the earthquake, categorized by various seismic intensity scales such as the Rossi-Forel scale. In 1883 John Milne surmised that the shaking of large earthquakes might generate waves detectable around the globe, and in 1899 E. Von Rehbur Paschvitz observed in Germany seismic waves attributable to an earthquake in Tokyo. In the 1920s Harry O. Wood and John A. Anderson developed the Wood-Anderson seismograph, one of the first practical instruments for recording seismic waves. Wood then built, under the auspices of the California Institute of Technology and the Carnegie Institute, a network of seismographs stretching across Southern California. He also recruited the young and unknown Charles Richter to measure the seismograms and locate the earthquakes generating the seismic waves.

In 1931 Kiyoo Wadati showed how he had measured, for several strong earthquakes in Japan, the amplitude of the shaking observed at various distances from the epicenter. He then plotted the logarithm of the amplitude against the distance, and found a series of curves that showed a rough correlation with the estimated magnitudes of the earthquakes. Richter resolved some difficulties with this method, then, using data collected by his colleague Beno Gutenberg, produced similar curves, confirming that they could be used to compare the relative magnitudes of different earthquakes.

To produce a practical method of assigning an absolute measure of magnitude required additional developments. First, to span the wide range of possible values Richter adopted Gutenberg's suggestion of a logarithmic scale, where each step represents a ten-fold increase of magnitude, similar to the magnitude scale used by astronomers. Second, he wanted a magnitude of zero to be around the limit of human perceptibility. Third, he specified the Wood-Anderson seismograph as the standard instrument for producing seismograms. Magnitude was then defined as "the logarithm of the maximum trace amplitude, expressed in microns", measured at a distance of 100 km. The scale was calibrated by defining a magnitude 3 shock as one that produces (at a distance of 100 km) a maximum amplitude of 1 micron (1 µm, or 0.001 millimeters) on a seismogram recorded by a Wood-Anderson torsion seismograph. Finally, Richter calculated a table of distance corrections, in that for distances less than 200 kilometers the attenuation is strongly affected by the structure and properties of the regional geology.

When Richter presented the resulting scale in 1935 he called it (at the suggestion of Harry Wood) simply a "magnitude" scale. "Richter magnitude" appears to have orginated when Perry Byerly told the press that the scale was Richter's, and "should be referred to as such." In 1956 Gutenberg and Richter, while still referring to "magnitude scale", labelled it "local magnitude", with the symbol M_L, to distinguish it from two other scales they had developed, the surface wave magnitude (M_S) and body wave magnitude (M_B) scales.

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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, symbol M_w); for earthquakes adequately measured by the Richter scale, numerical values are approximately the same. Although values measured for earthquakes now are ${\displaystyle M_{w}}$ (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 ${\displaystyle M_{\text{L}}}$ and the surface wave ${\displaystyle M_{\text{s}}}$ scale. In addition, the body wave magnitude, ${\displaystyle m_{\text{b}}}$, and the moment magnitude, ${\displaystyle M_{\text{w}}}$, 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 ${\displaystyle M_{\text{L}}}$, ${\displaystyle M_{\text{s}}}$, and ${\displaystyle M_{\text{w}}}$.> The ${\displaystyle m_{\text{b}}}$ 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.

${\displaystyle M_{\text{L}}}$ 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 ${\displaystyle M_{\text{s}}}$ is also reported frequently.

The seismic moment, ${\displaystyle M_{o}}$, 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. ${\displaystyle M_{\text{w}}}$ is derived from it empirically as a quantity without units, just a number designed to conform to the ${\displaystyle M_{\text{s}}}$ scale. A spectral analysis is required to obtain ${\displaystyle M_{o}}$, whereas the other magnitudes are derived from a simple measurement of the amplitude of a specifically defined wave.

All scales, except ${\displaystyle M_{\text{w}}}$, 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 ${\displaystyle M_{L}}$ is about 7 and about 8.5 for ${\displaystyle M_{\text{s}}}$.

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 (${\displaystyle =({10^{1.0}})^{(3/2)}}$) in the energy released; a difference in magnitude of 2.0 is equivalent to a factor of 1000 (${\displaystyle =({10^{2.0}})^{(3/2)}}$) 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 ${\displaystyle m_{\text{b}}}$ because most energy is carried by the high frequency waves.

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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:

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

(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 frequently 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).

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Magnitude empirical formulae

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

The Lillie empirical formula:

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

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

and for distances between 200 km and 600 km,

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

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

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

The Tsumura empirical formula:

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

The Tsuboi, University of Tokyo, empirical formula:

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

Source of the article : Wikipedia