6 December, 2000
The magic that makes AST/RO work.
Like most things, the processes that allow AST/RO to collect and analyze
light from molecular clouds are hidden, and can seem like magic. This
magic happens inside the dewars and computers that first analyze the
light.
From the sky, the light gets reflected into one of four dewars. Inside
the dewar, the light from the skys first stop is into a feedhorn which then
directs the light into a mixer.
Since the signals from the sky are extremely weak, we need to amplify the
signal. To do this, we need mix it with another known signal. But before
we can do this, we need to change the light into an electrical signal that
we can easily manipulate. This is done with a SIS junction- two
superconductors sandwiching an insulator. Superconductors are substances
that have no electrical resistance, and thus transmit an electrical signal
very well. With the SIS junction set up correctly, an incoming photon will
cause an electron to cross this junction, thus creating an electrical
current.
Once we have an electrical signal, we amplify and combine it with a known
signal. We can change this combined signal so that it is in a frequency
range that is easily analyzed by our computers, changing the signal from
hundreds of gigahertz to tens of Hertz. Then, the known signal can be
taken away, leaving our original signal from the sky in a frequency range
that we can analyze easily.
It is important to mention that the superconductors need to be kept cold
very cold in order for them to be a superconductor. Typically, this is
only a few Kelvin, a few degrees above absolute zero. This is
accomplished by keeping liquid helium in the dewar, which boils at a
temperature of 4 Kelvin (4K).
AST/RO has four receivers: Major Dobbins (230 Gigahertz, GHz), FLaMR (490
GHz), Wanda (490 GHz and 810 GHz), and PoleSTAR (4-channel 810 GHz). More
detailed information about how the receivers work can be found at the
University of Arizona, where they are built: http://soral.as.arizona.edu
-- the overview section is a good place to start.
Contact the TEA in the field at
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If you cannot connect through your browser, copy the
TEA's e-mail address in the "To:" line of
your favorite e-mail package.
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