[net.astro] Size and shape of our sun, and relativity: Thank you, Bob Dicke!

abeles@mhuxm.UUCP (abeles) (07/03/84)

As mentioned in the previous article by P. Wyant, Dicke has studied the
question of non-sphericalness of the sun.  To add to this, I point out
that research by Dicke's Princeton group on the subject of what is known
now as "solar oblateness" has continued at least until recently.  The
interested parties may consult the Science Citation Index for references
under the names of Dicke, R., Kuhn, J., and Libbrecht, K.  The latter
two are former graduate students of Dicke, now faculty, I believe, at 
Princeton and Caltech respectively.

Incidentally, Bob Dicke is probably the most accomplished physicist alive
who has not received the Nobel Prize in Physics.  He has had remarkable
achievements both as a theorist and as an experimentalist, in areas of
physics both incredibly applied and equally pure.  His early work at
the MIT Radiation Laboratory during WWII (the lab which developed radar)
is amply detailed in the famous MIT Radiation Lab series of books,
now out of print, but among the most referenced out-of-print works in
physical science.  The series comprises all original work on microwave
circuitry, detection by semiconductor devices, microwave tubes, etc.,
as developed for the war effort.

Dicke is also known as the founder of Princeton Applied Research corporation,
which is now a subsidiary of EG&G, Inc.  He started PAR with his invention
of the Lock-in Amplifier.

Dicke extended his microwave achievements to create the "Dicke radiometer"
which enables the most sensitive possible measurements of microwave
radiation and is used to this day in frontier experiments to determine
the physics of the famous 3-degree "isotropic" background radiation of
the universe, now accepted as being the remaining heat left over from
the big bang which started the universe, now distributed over the entire
universe and considerably cooler.  I put the term "isotropic" in quotes
because current measurements of the anisotropy indicate movement
of the earth and the solar system through the 3-degree background radiation.
These measurements also depend on the Dicke radiometer.

In fact, Dicke's historically verifiable involvement with the discovery
of the 3-degree background radiation led many to expect that he would
be among those to receive any Nobel Prize given for it.  As you know,
Arno Penzias and Robert Wilson did receive the Nobel Prize for their
experimental observation of a then-unexplained extra-galactic microwave
signal during the early sixties.

As mentioned in the previous article, Dicke also developed what is known
as the Brans-Dicke theory which is an alternative to the particular form
chosen by Einstein for the formulation of his General Theory of Relativity,
but which at the time predicted identical experimental results to the
Einsteinian formulation.  Today the consensus indeed is that the Einstein
formulation, which is more elegant and intuitive, is correct.  Nevertheless,
the importance of this work is not to be understated.

Finally, Dicke is responsible for the building up of experimental physics
other than nuclear and particle physics at Princeton through his strong
influence on the department over many years; a listing of the other
projects which have been associated with him would be impossible here.

--J. H. Abeles
  Bell Communications Research, Inc.
  Murray Hill, NJ