Meter water equivalent

In physics, the meter water equivalent (often m.w.e. or mwe) is a standard measure of cosmic ray attenuation in underground laboratories. A laboratory at a depth of 1000 m.w.e is shielded from cosmic rays equivalent to a lab 1000 m below the surface of a body of water. Because laboratories at the same depth (in meters) can have greatly varied levels of cosmic ray penetration, the m.w.e. provides a convenient and consistent way of comparing cosmic ray levels in different underground locations.[1]

Cosmic ray attenuation is dependent on the density of the material of the overburden, so the m.w.e. is defined as the product of depth and density (also known as an interaction depth). Because the density of water is 1 g/cm3, 1 m of water gives an interaction depth of 1 hectogram per square centimeter (hg/cm2). Some publications use hg/cm2 instead of m.w.e., although the two units are equivalent.[2]

Another factor that must be accounted for is the shape of the overburden. While some laboratories are located beneath a flat ground surface, many are located in tunnels in mountains. Thus, the distance to the surface in directions other than straight up is less than it would be assuming a flat surface.

Standard rock

In addition to m.w.e., underground laboratory depth can also be measured in meters of standard rock. Standard rock is defined to have mass number A = 22, atomic number Z = 11, and density 2.65 g/cm3.[3] Because most laboratories are under earth and not underwater, the depth in standard rock is often closer to the actual underground depth of the laboratory.

Existing underground laboratories

Underground laboratories exists at depths ranging from just below ground level to approximately 6000 m.w.e. at SNOLAB[4] and 6700 m.w.e. at the Jinping Underground Laboratory in China.[5]

References

  1. ↑ "Deep Science". National Science Foundation. Retrieved 2014-10-03.
  2. ↑ P. K. F. Grieder (2001). Cosmic Rays at Earth: Researcher's Reference Manual and Data Book. Gulf Professional Publishing. p. 482. ISBN 978-0-444-50710-5.
  3. ↑ K. A. Olive et al. (PDG) (2014). "Review of Particle Physics". Chinese Physics C. 38 (9): 090001. Bibcode:2014ChPhC..38i0001O. doi:10.1088/1674-1137/38/9/090001.
  4. ↑ Mei, D. -M.; Hime, A. (2006). "Muon-induced background study for underground laboratories". Physical Review D. 73 (5). arXiv:astro-ph/0512125Freely accessible. Bibcode:2006PhRvD..73e3004M. doi:10.1103/PhysRevD.73.053004.
  5. ↑ Wu, Yu-Cheng; Hao, Xi-Qing; Yue, Qian; Li, Yuan-Jing; Cheng, Jian-Ping; Kang, Ke-Jun; Chen, Yun-Hua; Li, Jin; Li, Jian-Min; Li, Yu-Lan; Liu, Shu-Kui; Ma, Hao; Ren, Jin-Bao; Shen, Man-Bin; Wang, Ji-Min; Wu, Shi-Yong; Xue, Tao; Yi, Nan; Zeng, Xiong-Hui; Zeng, Zhi; Zhu, Zhong-Hua (August 2013). "Measurement of cosmic ray flux in the China JinPing underground laboratory" (PDF). Chinese Physics C. 37 (8): 086001. arXiv:1305.0899Freely accessible. Bibcode:2013ChPhC..37h6001W. doi:10.1088/1674-1137/37/8/086001.
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