Magnetic field strength of earth at equator,power blackout tweed heads,emergency preparedness plan template for home 3d - For Begninners

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It was in 2002-2003 that BibleSearchers Reflections began to investigate the role of the earth’s geo-magnetic field in relationships to future biblical prophetic envisioned catastrophes. Second, when the geomagnetic field diminishes, it allows unhindered solar energies to flow in unimpeded into the earth’s crust, creating extremely low frequency waves, associated with large air pressure changes, can create a electrical stimulation that can bring on a seismic event in the form of an earthquake. Updated to the year of 2010, we are now in the midst of progressive weather changes; earthquakes, typhoons, hurricanes, increasing solar flares, and evidence of the fragmentation of our crustal tectonic plates as we head towards 2012 and the End of the Mayan World Age. During the crossing, the Moon comes in contact with a gigantic "plasma sheet" of hot charged particles trapped in the tail. On the Moon's dayside this effect is counteracted to a degree by sunlight: UV photons knock electrons back off the surface, keeping the build-up of charge at relatively low levels.
Walking across the dusty charged-up lunar terrain, astronauts may find themselves crackling with electricity like a sock pulled out of a hot dryer. The best direct evidence comes from NASA's Lunar Prospector spacecraft, which orbited the Moon in 1998-99 and monitored many magnetotail crossings. The roller coaster of charge would be at its most dizzying during solar and geomagnetic storms.
A newly published study uses IBEX data and simulations of the interstellar boundary to better describe space in our galactic neighborhood. Immediately after its 2008 launch, NASA’s Interstellar Boundary Explorer, or IBEX, spotted a curiosity in a thin slice of space: More particles streamed in through a long, skinny swath in the sky than anywhere else. A new paper, published in The Astrophysical Journal Letters, precisely determines the strength and direction of the magnetic field outside the heliosphere.
This simulation shows the origin of ribbon particles of different energies or speeds outside the heliopause (labeled HP).
The new paper is based on one particular theory of the origin of the IBEX ribbon, in which the particles streaming in from the ribbon are actually solar material reflected back at us after a long journey to the edges of the sun’s magnetic boundaries.
Outside the heliosphere lies the interstellar medium, with plasma that has different speed, density, and temperature than solar wind plasma, as well as neutral gases.
Some solar wind protons that flow out from the sun to this boundary region will gain an electron, making them neutral and allowing them to cross the heliopause.
The IBEX ribbon is a relatively narrow strip of particles flying in towards the sun from outside the heliosphere. The directions of different ribbon particles shooting back toward Earth are determined by the characteristics of the interstellar magnetic field.

For the recent study, such observations were used to seed simulations of the ribbon’s origin.
But that difference may be accounted for by considering a stronger influence from the solar cycle, which can lead to changes in the strength of the solar wind and thus change the distance to the termination shock in the directions of Voyager 1 and 2. The Southwest Research Institute leads IBEX with teams of national and international partners. This generation will no doubt be “chosen” to experience the great transition as the Great Exodus of the Lost Tribes of Israel begin returning home as our earth prepares for the revealing of the Age of the Messiah. Ancient craters and frozen lava seas lie motionless under an airless sky of profound quiet. NASA-supported scientists have realized that something does happen every month when the Moon gets a lashing from Earth's magnetic tail. It is an extension of the same familiar magnetic field we experience when using a Boy Scout compass.
The lightest and most mobile of these particles, electrons, pepper the Moon's surface and give the Moon a negative charge.
But on the nightside, in the cold lunar dark, electrons accumulate and voltages can climb to hundreds or thousands of volts.
Touching another astronaut, a doorknob, a piece of sensitive electronics"”any of these simple actions could produce an unwelcome zap.
Drawn by differences in global charge accumulation, floating dust would naturally fly from the strongly-negative nightside to the weakly-negative dayside.
No one can say for sure what happens on the Moon when the magnetotail hits, because no one has been there at the crucial time. During some crossings, the spacecraft sensed big changes in the lunar nightside voltage, jumping "typically from -200 V to -1000 V," says Jasper Halekas of UC Berkeley who has been studying the decade-old data. The origin of the so-called IBEX ribbon was unknown – but its very existence opened doors to observing what lies outside our solar system, the way drops of rain on a window tell you more about the weather outside. Such information gives us a peek into the magnetic forces that dominate the galaxy beyond, teaching us more about our home in space. The IBEX ribbon particles interact with the interstellar magnetic field (labeled ISMF) and travel inwards toward Earth, collectively giving the impression of a ribbon spanning across the sky.
A giant bubble, known as the heliosphere, exists around the sun and is filled with what’s called solar wind, the sun’s constant outflow of ionized gas, known as plasma. These materials interact at the heliosphere’s edge to create a region known as the inner heliosheath, bounded on the inside by the termination shock – which is more than twice as far from us as the orbit of Pluto – and on the outside by the heliopause, the boundary between the solar wind and the comparatively dense interstellar medium.

Once in the interstellar medium, they can lose that electron again, making them gyrate around the interstellar magnetic field. A new study corroborates the idea that particles from outside the heliosphere that form the IBEX ribbon actually originate at the sun – and reveals information about the distant interstellar magnetic field. For instance, simulations show that the most energetic particles come from a different region of space than the least energetic particles, which gives clues as to how the interstellar magnetic field interacts with the heliosphere. Not only do these simulations correctly predict the locations of neutral ribbon particles at different energies, but the deduced interstellar magnetic field agrees with Voyager 1 measurements, the deflection of interstellar neutral gases, and observations of distant polarized starlight. Those pre-IBEX estimates were based largely on two data points – the distances at which Voyagers 1 and 2 crossed the termination shock. The two Voyager spacecraft made their measurements almost three years apart, giving plenty of time for the variable solar wind to change the distance of the termination shock.
NASA Goddard manages the Explorers Program for the agency’s Heliophysics Division within the Science Mission Directorate in Washington.
The forces of the universe are changing as our world is moving from a long era of Uniformitarianism to a world of Catastrophism.
Our entire planet is enveloped in a bubble of magnetism, which springs from a molten dynamo in Earth's core. This could create a temporary nighttime atmosphere of dust ready to blacken spacesuits, clog machinery, scratch faceplates (moondust is very abrasive) and generally make life difficult for astronauts. This "dust storm" effect would be strongest at the Moon's terminator, the dividing line between day and night.
NASA is returning to the Moon in the decades ahead and plans to establish an outpost for long-term lunar exploration. When these particles reach the edges of the heliosphere, their motion becomes more complicated.
If those particles pick up another electron at the right place and time, they can be fired back into the heliosphere, travel all the way back toward Earth, and collide with IBEX’s detector.
Out in space, the solar wind presses against this bubble and stretches it, creating a long "magnetotail" in the downwind direction: diagram. The particles carry information about all that interaction with the interstellar magnetic field, and as they hit the detector they can give us unprecedented insight into the characteristics of that region of space.

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