F. Curtis Michel

Curt Michel

fcm@rice.edu

My Theory of Pulsars

What a great field to be in!

On a more positive note, try Family Stuff


Member of Scientia .

Spa 565 shows the class syllabus for spring 1998

What's New is available here.

Recent talk

Publication list is available here.

Biographical information is available here.

Proposals are available here.


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Interested in graduate work?


Work Address
Space Physics and Astronomy Dept.
Rice University  MS-108
P.O. Box 1892
Houston, Texas 77251
telephone: (713) 527-4925
fax: (713) 285-5143

Home Address
2101 University Blvd.
Houston, TX 77030
(713) 665-2974


Read "Theory of Neutron Star Magnetospheres" (Univ. Chicago 1991) - NOW!

"In conclusion, those interested in 
understanding how pulsars shine are
warned against taking seriously the
sweeping clains made in this book for 
the success of the authors' own model.
They would be better advised to turn 
to the observationally oriented book
Pulsar Astronomy by A. G. Lyne and 
F. G. Smith (Cambridge, 1990), and
to the very different theoretical biases
but much more complete attention to 
the facts found in Theory of Pulsar
Magnetospheres(sic) by F. Curtis Michel
(Chicago, 1991)."
			Jonathan Arons
	University of California, Berkeley
(Review of Physics of the Pulsar Magnetosphere
by Beskin, Gurevich and Istomin, Physics Today
October 1994, p. 71.)

Birkeland images from my book

Unfortunately these are hard to find. They are from pages 223, 254, and 257, respectively.

Above, we get an equatoral belt of trapped electrons.

Now we even get concentric Saturn-like rings.

The man in person, in his lab, inspecting one of his runs. The next is just a summary of what it is like to teach science to non scientists.