November 1960 Electronics World
Wax nostalgic about and learn from the history of early electronics. See articles
Electronics World, published May 1959
- December 1971. All copyrights hereby acknowledged.
Being the birthday of
W. Wilson, there is no better occasion to post this article about the "sugar-scoop"
antenna used by the two Bell Telephone Labs engineers (the other being
Dr. Arno A. Penzias) who serendipitously discovered the cosmic
microwave background radiation (CMBR)
believed to be a signature of "The Big Bang." The pair were investigating an unexplained
hiss in the background of the very low noise receiver attached to the antenna. That microwave
energy was constant and came from all areas of the sky, regardless of where the antenna
was pointed. They eventually deduced that the signature was consistent with the
theoretical energy level of the primordial "soup" that was our universe a short time
after expansion began. Although this piece was published in 1960, it was not until 1964 that the
discovery was made.
Articles here on RF Cafe which mention the Dr. Robert W. Wilson and Dr. Arno
A. Penzias are The Maser & Sugar
Scoop Antenna: Receiver for Signals from Space,
Laboratories Project Echo,
The Amazing Maser: The Jewel That Conquers Space,
Signals from Sun and Stars, and
High on a hill in the New Jersey Highlands near
the birthplace of radio astronomy is the unusual-looking antenna that appears on our
cover this month. This antenna, shaped like a giant sugar scoop, is Bell Telephone Laboratories'
low-noise horn-reflector antenna. Already having been used to receive ultra-weak voice
signals from California, after these signals have been bounced off the moon, the antenna
is playing a star's role in NASA's project "Echo." In this project, a 100-foot aluminized
balloon, launched by rocket, served as a reflector for coast-to-coast radio signals.
According to Frederick R. Kappel, President of American Telephone and Telegraph Co.,
the type of research that is being done by telephone scientists today in space communications
is aimed at creating thousands of high-quality voice channels and, ultimately, television
channels, that would interconnect all parts of the globe by way of satellites.
The unusual shape of the antenna is required not only to obtain very high gain (about
43 db) and a narrow beam width (1 1/4°) but also to eliminate any side or rear lobes
from the antenna's directional pattern. Even with large and highly directive parabolic-reflector
antennas, some undesired lobes are directed toward the ground and the sky. These produce
some noise in a system that cannot be tolerated because of the extremely weak signals.
The entire structure, made largely from aluminum, is about 50 feet long and about
35 feet high. The horn opening measures around 20 by 20 feet. The entire assembly can
be rotated through 360 degrees on its circular track, and the large upright wheel allows
it to be oriented at any vertical angle.
The output signals from the horn are applied through a rotary joint and some r.f.
plumbing to the ruby maser amplifier located in the small cab at the end of the antenna.
The maser maintains the high sensitivity and extremely low noise characteristics that
are so essential in working with very weak signals.
The maser employed is a two-channel device operating at a signal frequency of 2400
mc. The two channels are useful in picking up signals having either clockwise or counterclockwise
circular polarization. The heart of the maser, a slab of ruby crystal, is kept at a temperature
just a few degrees above absolute zero (-460°F), by being submerged in a container of
liquid helium. This, in turn, is submerged in liquid nitrogen to prevent heat losses.
The two tanks of helium and nitrogen are located underneath the cabin that houses the
maser. Together with the horn-reflector antenna and an FM demodulation system, the maser
makes the system the most sensitive voice radio receiver yet built. (Cover photo by Bell
Posted January 10, 2018