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From: "Alexander Kosovichev" <sasha@khors.Stanford.EDU>
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Date: Thu, 19 Dec 1996 17:50:34 -0800
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To: local@quake.Stanford.EDU, jkuhn@solar
Subject: Satellite Images Show Our 'Round' Sun to be a Bit Knobby
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	The Christian Science Monitor
	SAN FRANSICO -- Astronomers who study the sun have a new image to
contemplate - a knobby star.
	Early data from a new European-American orbiting solar observatory
show our star is covered with knob-like features. They measure about
60,000 miles across (five Earth diameters) and a half-mile high. On a
solar scale, that makes them too small to have been seen by any Earth-
or space-based solar observatory before.
	Shown for the first time at the fall meeting here of the American
Geophysical Union, the knobs appear to be a significant feature of the
sun's outer layer. Ed Rhodes of the University of Southern California
at Los Angeles told a press conference that theorists had predicted
such features should exist. If the knobs prove to be a permanent solar
element, he says, it is reasonable to think they play a significant
role in the mechanisms that bring energy from the interior to power
solar activity and sunshine.
	Meanwhile, the sharp view of the new, $1.1 billion satellite may
have settled a debate over whether the sun's shape is inconsistent
with Einstein's general theory of relativity, and how fast the sun's
core region rotates. Jeff Kuhn of Michigan State University reported
that new observations show the sun, instead of having a slightly
squashed shape, is essentially a perfect sphere ``and Einstein's
theory is safe.`` He added that some theorists suggested that the core
region rotates quite rapidly compared with the rest of the sun. The
fact that the sun shows so little flattening rules that out.


