Re: Honest Question...Poleshift and the Pyramids...Pole/Axis Shift in Cayce Quotes

In Article  <fc8f94e.0110241040.47383465@posting.google.com> Idon't wrote:
> Reviewed that link and some others. Thanks. I don't fully
> inderstand the technology used for detecting Solar 
> magnetism, but they certainly seem to be seeing it. 

Let's examine their claim in detail, of WHY solar flares et al have a
magnetic basis.  They measure x-rays, light rays, and all of this
somehow is supposed to be caused by magnetism.  Is this the case on
Earth?  We bend light rays with a magnetic field? Can we do this in the
lab?  X-rays are excited by an electrical flow, yes, but do we bend
x-rays in a direction with a magnetic field ALONE? Can we do this in the
lab?  We heat something to 1,800,000ºF in the lab to see how it
behaves?  What PROOF do they have that magnetism is involved in sun
cycles, is the driver?   None.

Sunspot Cycle Predictions, linked from ..
http://science.msfc.nasa.gov/headlines/y2001/ast15feb_1.htm
    MSFC Solar Physics Branch members Wilson, Hathaway,
    and Reichmann have studied the  sunspot record for 
    characteristic behavior that might help in predicting 
    future sunspot  activity. Our current predictions of solar 
    activity for the next few years can be found at  this link. 
    Although sunspots themselves produce only minor
    effects on solar emissions, the magnetic activity that 
    accompanies the sunspots can produce dramatic changes
    in the ultraviolet and soft x-ray emission levels. These 
    changes over the solar cycle have important consequences
    for the Earth's upper atmosphere.

The White-Light Corona, linked from ..
http://science.msfc.nasa.gov/headlines/y2001/ast15feb_1.htm
    The Corona is the Sun's outer atmosphere. It is visible 
    during total  eclipses of the Sun as a pearly white crown 
    surrounding the Sun. The corona displays a  variety of 
    features including streamers, plumes, and loops.
    These features change from eclipse to eclipse and the 
    overall shape of the corona changes  with the sunspot cycle.
    However, during the few fleeting  minutes of totality few, 
    if any, changes are seen in these coronal features.

The Emission Line Corona, linked from ..
http://science.msfc.nasa.gov/headlines/y2001/ast15feb_1.htm
    Early observations of the visible spectrum of the corona 
    revealed bright emission lines at wavelengths that did not
    correspond to any known materials. This led astronomers
    to propose the existence of coronium as the principal gas 
    in the corona. The true nature of the corona remained a 
    mystery until it was determined that the coronal gases are 
    super-heated to temperatures greater than 1,000,000ºC 
    (1,800,000ºF). At these high temperatures both hydrogen
    and helium (the two dominant elements) are completely 
    stripped of their electrons. Even minor elements like 
    carbon, nitrogen, and oxygen are stripped down to bare 
    nuclei. Only the heavier trace elements like iron and
    calcium are able to retain a few of their electrons in this 
    intense heat. 

The X-Ray Corona, linked from ..
http://science.msfc.nasa.gov/headlines/y2001/ast15feb_1.htm
    The corona shines brightly in x-rays because of its high 
    temperature. On  the other hand, the "cool" solar photosphere
    emits very few x-rays. This allows us to view the corona 
    across the disk of the Sun when we observe the Sun in X-rays.
    To do this we must first design optics that can image x-rays 
    and then we must get above the Earth's atmosphere. 

Chromosphere, linked from ..
http://science.msfc.nasa.gov/headlines/y2001/ast15feb_1.htm
    The chromosphere is an irregular layer above the photosphere
    where the temperature rises from 6000° C to about 20,000° C. 
    At these higher temperatures hydrogen emits light that 
    gives off a reddish color (H-alpha emission). This colorful 
    emission can be seen in prominences that project above the 
    limb of the sun during total solar eclipses. This is what gives 
    the chromosphere its name (color-sphere). When the Sun is 
    viewed through a spectrograph or a filter that isolates
    the H-alpha emission, a wealth of new features can be seen.
    These features include the chromospheric network of
    magnetic field elements, bright plage around sunspots,