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The Sudbury Neutrino Observatory (SNO) was a neutrino observatory located 2100 m underground in Vale's Creighton Mine in Sudbury, Ontario, Canada.The detector was designed to detect solar neutrinos through their interactions with a large tank of heavy water.
APEX-CAMBIUM - Advanced Plant Experiments on Orbit [2] Funded by the Canadian Space Agency (CSA), APEX-Cambium will help determine the role gravity plays in trees forming different kinds of wood. BCAT-5 - Binary Colloidal Alloy Test [3] BISE - Bodies In the Space Environment [4] CCISS - Space travel can be dizzying [5]
SNOLAB is a Canadian underground science laboratory specializing in neutrino and dark matter physics. Located 2 km below the surface in Vale's Creighton nickel mine near Sudbury, Ontario, SNOLAB is an expansion of the existing facilities constructed for the original Sudbury Neutrino Observatory (SNO) solar neutrino experiment.
In addition, a liquid scintillator experiment can detect anti-neutrinos like those created in nuclear fission reactors and the decay of thorium and uranium in the earth. SNO+ uses 780 tonnes of linear alkylbenzene as the scintillator (the detector started to be filled with the scintillator at the end of 2018 [ 3 ] ) and will be filled with 130
A FACE experiment began at Duke University in June 1994. The Blackwood Division of the Duke Forest contains the Forest-Atmosphere Carbon Transfer and Storage facility. This consists of four free-air CO 2 enrichment plots which provide higher levels of atmospheric CO 2 concentration and four plots that provide ambient CO 2 control. [ 5 ]
The experiment is designed for a 20-year period of data collection. [4] The primary science objectives of DUNE are [4] [5] Investigation of neutrino oscillations to test CP violation in the lepton sector, which explores why the universe is made of matter. [6] Determination of the ordering of the neutrino masses. [7]
The Canadian Hydrogen Intensity Mapping Experiment (CHIME) is an interferometric radio telescope at the Dominion Radio Astrophysical Observatory in British Columbia, Canada which consists of four antennas consisting of 100 x 20 metre cylindrical parabolic reflectors (roughly the size and shape of snowboarding half-pipes) with 1024 dual-polarization radio receivers suspended on a support above ...
The symmetry of a carbon dioxide molecule is linear and centrosymmetric at its equilibrium geometry. The length of the carbon–oxygen bond in carbon dioxide is 116.3 pm, noticeably shorter than the roughly 140 pm length of a typical single C–O bond, and shorter than most other C–O multiply bonded functional groups such as carbonyls. [19]