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helium I

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helium I

[′hē·lē·əm ′wən]
(cryogenics)
The phase of liquid helium-4 which is stable at temperatures above the lambda point (about 2.2 K) and has the properties of a normal liquid, except low density.
McGraw-Hill Dictionary of Scientific & Technical Terms, 6E, Copyright © 2003 by The McGraw-Hill Companies, Inc.
References in periodicals archive
While it's all over the universe, there are only a few places on Earth where helium is regularly extracted.
Helium is a byproduct of natural gas and the current crisis is one of supply and demand, with the global demand for helium for everything from balloons to MRI machines far outpacing the noble gas' scarce supply.
Helium is the second element of the periodic table and is one of the most abundant elements in the universe, yet it is fairly rare on Earth.
A world shortage of liquid helium is expected to remain severe at least until the second half of 2013.
That is, although helium is typically regarded as a nonpsychoactive gas (an issue we discuss below), these decedents were nonetheless attempting to get high using helium and suffocated in consequence.
Helium is the only element that can remain at a sufficiently cold temperature to allow for the stable and uniform magnetic field the MRI scanners need to work.
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