Re: Seventy-Day Jupiter Movie Pulls Patterns Out Of Chaos 4

Planetary rotation has been explained by the Zetas (previous post 2) as
due to lack of homogeneity in a mobile or liquid core, parts of which
chase or retreat from elements they are attracted to or repulsed from
OUTSIDE of the planet. The question raised by the NASA post (previous
post 1) is why their model does not work, as the movies made of the pole
shots show that the poles, and not just the equatorial latitudes, also
rotate. If the NASA model no longer works, then what IS causing the
alternating east-west motion (previous post 3) within Jupiter's latitude
bands?  And why the longevity of the storms produced? The Zetas will
explain.

    On Earth, these same patterns exist, but due to the
    buffering action of the crust the atmosphere operates
    independently. Where the Earth moves under the 
    atmosphere, the drag is from east to west, and as the 
    atmosphere is not so inclined, eddy currents, the prevailing
    westerlies, are created.  Storms on Earth, created due to
    unequal pressure of air masses and their relative humidity,
    last only as long as equalizing the factors takes - a matter
    of days.  Storms on a gaseous planet, noted by NASA in
    July, 2001 from recent images taken by a fly-by probe,
    seem to last for long periods.  This is because they are
    NOT driven simply by a thin and highly mobile air mass,
    but by elements disbursed in the entire core of the planet.
    Equalization is not in a thin layer, but as deep as the
    planet itself, so the drama takes longer to resolve.
        ZetaTalk™

PIA-03452
Jupiter Polar Winds Movie
July 16, 2001, http://www.nasa.gov

    Bands of eastward and westward winds on Jupiter
    appear as concentric rotating circles in this movie ...
    What is surprising in this view is the coherent nature
    of the high-latitude flows, despite the very chaotic,
    mottled and non-banded appearance of the planet's
    polar regions.  This is the first extended movie
    sequence to show the coherence and longevity of
    winds near the pole and the features blown around
    the planet by them. ... There are thousands of spots,
    each an active storm similar to the size to the largest
    of storms on Earth.  Large terrestrial storms usually
    last only a week before they dissolve and are replaced
    by other storms. But many of the Jovian storms seen
    here, while occasionally changing latitute or merging
    with each other, persist for the entire 70 days. Until
    now, the lifetime of the high-latitude features was
    unknown. Their longevity is a mystery of Jovian weather.