A Beginner's View of Our Electric Universe - New
A Beginner's View of Our Electric Universe - New
A Beginner's View of Our Electric Universe - New
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The sensitive equipment we have can detect<br />
this radiation so images can then be constructed<br />
that let us understand the filamentary nature <strong>of</strong><br />
structures in space. One <strong>of</strong> the best sources for<br />
imagery has been the Chandra X-ray observatory<br />
launched in 1999. The X-ray detectors it carries<br />
have revealed to us not only wonderful structures<br />
in our own galaxy but many that lie billions <strong>of</strong><br />
light years further away.<br />
The Cygnus Loop. Credit: ESA & Digitised Sky Survey (Caltech)<br />
What appeared before to us as vast empty spaces are now showing up as regions that have within them filamentary<br />
networks that deliver power to galaxies and stars and to vast regions <strong>of</strong> dust and gas where the formation <strong>of</strong> new<br />
bodies is going on. Appreciating the pervasiveness and power <strong>of</strong> Birkeland currents on the grandest scales helps<br />
us understand how plasma networks have formed the universe and remain to dominate it.<br />
Stars again: With more now in place, we will go back to stars. We said they have solid cores and that, depending<br />
on the charge level they have, their plasmaspheres will extend sometimes to great distances. The size and colour<br />
<strong>of</strong> what appears to be their outer glowing or arcing<br />
surface is therefore no indication <strong>of</strong> the size <strong>of</strong><br />
the core, in fact, we have no way <strong>of</strong> telling much<br />
about a star’s solid core except that electric theory<br />
says it is cooler than the photosphere. A star’s<br />
appearance is also no indication <strong>of</strong> its age, as has<br />
been assumed for so long by astro-science. Rather,<br />
the apparent size and colour tells us about the<br />
physical dimensions <strong>of</strong> the plasmasphere around<br />
the core and the density <strong>of</strong> current flowing onto<br />
and into the star at this single point in time [6-21] .<br />
In terms <strong>of</strong> all low-energy stars that do not ‘shine’<br />
like typical stars, these bodies have until just a few<br />
decades ago, been very hard indeed to detect.<br />
A comparison <strong>of</strong> star and planet sizes to Earth<br />
Credit: NASAJPL-CaltechUCB<br />
110 | The <strong>Electric</strong> <strong>Universe</strong> answers I see