Laser-interferometric strainmeters have several advantages over conventional quartz-tube and invar-rod strainmeters, such as high sensitivity, low drift, and expandability to long baseline measurements. Of these advantages, low-drift performance is the most significant if a frequency-stabilized laser is used as a light source for the strainmeter . Frequency stabilityreaches values better than 10
-1210
-13 ; the potential strain accuracy of the laser strainmetercorresponds to these figures. Because strainmeters have a flat response to ground strain change, very broadband observations, such as earth tides, strain steps, and small earthquakes, with a range of 10
6 -10 Hz, are possible. Strain measurements with reference to a quantum standard that has no drift in principle, such as the wavelength of a frequency-stabilized laser, are essential for the long-term strain measurement of secular and tectonic strain changes. In our observations with the laser strainmeter, however, secular and tectonic changes are unclear, even at a deep undergroundsite. On the other hand, GPS has observed secular and tectonic strain changes; the GPS uses the wavelength of an atomic clock as a reference, which is a quantum standard like a frequency-stabilized laser. After comparing the principle and data of the Kamioka laser strainmeter and other strain meters with those of GPS, we concluded that km-class laser strainmeters can realize long-term strain observations with a higher resolution than GPS. We propose that two-color interfer ometers be constructed in air as a reasonable solution to resolution and cost . With the use of ordinary laser strainmeters (10-100-m baselines), two-color laser strainmeters (1-10-km baselines), and GPS (10-100-km baselines), all of which are based on quantum standards, strain observations can cover a very broad range in both time and space.
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