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Ionosphere: Difference between revisions
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Ionization depends primarily on the Sun and its activity. The amount of ionization in the ionosphere varies greatly with the amount of radiation received from the Sun. Thus there is a diurnal (time of day) effect and a seasonal effect. The local winter hemisphere is tipped away from the Sun, thus there is less received solar radiation. The activity of the Sun is associated with the sunspot cycle, with more radiation occurring with more sunspots. Radiation received also varies with geographical location (polar, auroral zones, mid-latitudes, and equatorial regions). There are also mechanisms that disturb the ionosphere and decrease the ionization. There are disturbances such as solar flares and the associated release of charged particles into the solar wind which reaches the Earth and interacts with its geomagnetic field.<ref>[https://en.wikipedia.org/wiki/Ionosphere Ionosphere]</ref> | Ionization depends primarily on the Sun and its activity. The amount of ionization in the ionosphere varies greatly with the amount of radiation received from the Sun. Thus there is a diurnal (time of day) effect and a seasonal effect. The local winter hemisphere is tipped away from the Sun, thus there is less received solar radiation. The activity of the Sun is associated with the sunspot cycle, with more radiation occurring with more sunspots. Radiation received also varies with geographical location (polar, auroral zones, mid-latitudes, and equatorial regions). There are also mechanisms that disturb the ionosphere and decrease the ionization. There are disturbances such as solar flares and the associated release of charged particles into the solar wind which reaches the Earth and interacts with its geomagnetic field.<ref>[https://en.wikipedia.org/wiki/Ionosphere Ionosphere]</ref> | ||
==Birkeland Current== | |||
A [[Birkeland current]] is a set of currents that flow along geomagnetic field lines connecting the Earth’s [[Magnetosphere]] to the Earth's high latitude [[Ionosphere]]. In the Earth’s magnetosphere, the currents are driven by the solar wind and interplanetary magnetic field and by bulk motions of plasma through the magnetosphere (convection indirectly driven by the interplanetary environment). | |||
==Particle Charge Ratio== | |||
The recent transmissions were a momentous event that has stabilized a different ratio of particle charge to the magnetic field layer, within our planetary ionosphere. The [[Ionosphere]] is the uppermost part of the planet’s atmosphere, distinguished because it is ionized by solar radiation. The [[Ionization]] levels depend primarily on the Sun and its activity. The amount of ionization in the ionosphere varies greatly with the amount of radiation received from the sun. We have recently had unprecedented massive solar flare activity and this is the associated release of charged particles into the solar wind, which reaches the Earth and interacts with its geomagnetic field. [[Ionization]] is the physical process of converting an atom or molecule into an ion, by adding or removing charged particles such as electrons or other ions. <ref>[https://energeticsynthesis.com/resource-tools/news-shift-timelines/149-newsletter-2008/1622-magnetic-change-of-the-global-brain Magnetic Change of Global Brain]</ref> | |||
==Organic Magnetism== | |||
The [[Solar Coding|solar streams]] in the form of solar winds enter the [[Magnetosphere]] which is located in the ultraviolet layer of the [[Ionosphere]] and directly control the planet’s internal magnetic field, which is currently being reconfigured into organic states of magnetism.<ref>[https://energeticsynthesis.com/resource-tools/news-shift-timelines/3716-solar-coding-crystal-body-and-dna Solar Coding, Crystal Body and DNA]</ref> | |||
==References== | ==References== | ||
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==See Also== | ==See Also== | ||
[[Geoengineering]] | |||
[[NET]] | [[NET]] | ||