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Oscillations, Waves, and Interactions - GWDG

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304 Schreiber<br />

7.2 The ring laser component<br />

In order to obtain a stable interferogram of the two laser beams the cavity length has<br />

to be kept constant to within a fraction of a wavelength. Therefore usually ring laser<br />

bodies are made from Zerodur, a glass ceramic which exhibits a very small relative<br />

thermal expansion of α = 5 · 10 −8 K −1 . Since a ring laser for seismic applications<br />

requires an enclosed area of more than 1 m 2 a monolithic ring construction would<br />

both be too expensive <strong>and</strong> not transportable.<br />

Figure 25 gives an impression of the actually realized ring laser hardware. Again<br />

the laser cavity has the shape of a square. The 4 turning mirrors are each located<br />

in a solid corner box. As shown on the right side of the plot, a folded lever system<br />

allows the alignment of each mirror to within ±10 seconds of arc. This high level of<br />

alignment is required to ensure lasing from an optically stable cavity. The mirrors<br />

are located inside steel containers which in turn are connected up with stainless steel<br />

tubes, forming a vacuum recipient around the laser beam path. In the middle of one<br />

side the steel tubes are reduced to a small glass capillary of 4 mm in diameter <strong>and</strong> a<br />

length of 10 cm, which is required for gain medium excitation. When operated, the<br />

ring laser cavity is first evacuated <strong>and</strong> then filled with a mixture of Helium <strong>and</strong> Neon<br />

reaching a total gas pressure of approximately 6 mbar. The left part of Fig. 25 gives<br />

an impression of the instrumental layout. The following two important considerations<br />

are unique for the GEOsensor design.<br />

• Since the ring laser is constructed from several components, it requires a stable<br />

concrete platform as a base at the location of deployment. Such a pad is simple<br />

to specifiy <strong>and</strong> can be prepared totally independent of the actual GEOsensor<br />

deployment.<br />

• The actual area of the ring laser component is not predetermined by the design.<br />

The instrument can be built according to the available space at the respective<br />

host observatory. Different GEOsensor realizations may therefore have different<br />

sizes <strong>and</strong> consequently different instrumental resolution. The length of the<br />

current instrument is 1.6 m on a side, which provides an area of 2.56 m 2 .<br />

Figure 25. The basic construction layout of the GEOsensor ring laser

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