October 6, 2010: Asteroid Impact | Oct. 5 | Oct. 7 | 2010 | FOTD Home |
Fractal
visionaries
and enthusiasts:
For some reason, the TV channels these days are filled with programs
about looming catastrophes and the end of civilization. So
why not have one of the looming catastrophes appear in fractal
form? This is just what happened in today's FOTD, which
captures the hypothetical asteroid-impact catastrophe at the moment of
impact.
Actually, the scene shows an order 1.15 minibrot in the parent fractal
that appears when the formula Z^(1.15)+C is iterated at the
MandelbrotBC3 formula's ground level. This parent is shaped
much like the minibrot in today's image, and is decorated on its
southwest side by a field of rather fantastic zigzagging
filaments. Today's image lies about halfway out in this field.
The name "Asteroid Impact" says it all.
The rating of a 7 might be a little overdone. The colors
appear a bit too brilliant to me.
The calculation time of 1-3/4 minutes is a lot shorter than the time it
took for the asteroid to reach the earth.
Chilly temperatures and occasional light rain kept activity suppressed
here at Fractal Central on Tuesday. The fractal cats leaped
to their shelf for joy when the sun briefly appeared in the afternoon,
taking the chill from the temperature of 54F 12C. Unfortunately, the
sun went behind the clouds after bringing only 5 minutes warmth, and
the cats were sorely disappointed. My day was slow and
routine. FL killed time watching those hot Latin soap
operas. The next FOTD will be posted in 24 hours.
Until then, take care, and when will we capture a live bigfoot?
Jim Muth
jamth@mindspring.com
START PARAMETER FILE=======================================
Asteroid_Impact { ; time=0:01:43.70-SF5
on P4-2000
reset=2004 type=formula formulafile=basicer.frm
formulaname=MandelbrotBC3 function=ident
center-mag=-5.61156103006634/-3.172542628607448/\
247530.1/1/-171.1/0 params=1.15/0/0/525 float=y
maxiter=32767 inside=0 logmap=102 periodicity=6
colors=0002AI4BK6CM8DOAEQCFSEGUGHWIIYKJ_MKaOLcQMeS\
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FUSEURDUQCTPBSOARNAQMAOLAMJAJIAIHAHGAGFAFcRccT`cWX\
cYUc_QcbNcdJcfGc_JcUMcOPcIScFRcBRc8Qc5Pc2zc4zc7zc9\
zAlsBwrBkrmjrmjrCwqmiqmiqDwqmhpmhpmhpmgpEwpmfoFwoF\
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tKmtNmuPmuSmuUmvXmvZmvamvdmwfmwimzkmznmzpmzsmzumzx\
mzzmzqmzmmzmmzmmzmmzmmzmmzmmzzzzzzzzzzzzzzzzzzzzzz\
zzzzzzzzzzzzzzzzzzzzzzzzzzzzzzzzzzzzzzzzzzzzzzzzzz\
zzzzzzzzzzzzzzzzzzzzzzzzz }
frm:MandelbrotBC3 { ; by several Fractint users
e=p1, a=imag(p2)+100
p=real(p2)+PI
q=2*PI*fn1(p/(2*PI))
r=real(p2)+PI-q
Z=C=Pixel:
Z=log(Z)
IF(imag(Z)>r)
Z=Z+flip(2*PI)
ENDIF
Z=exp(e*(Z+flip(q)))+C
|Z|<a }
END PARAMETER FILE=========================================