NASA Ulysses Data
Launched in 1990 from the space shuttle Discovery’s STS-41 mission, the Ulysses spacecraft would be going on a mission that lasted till 2009 and for
which we can attribute most of the Sun’s heliosphere data available nowadays.
The primary mission of the Ulysses spacecraft was to characterize the heliosphere as a function of solar latitude. The heliosphere is the vast
region of interplanetary space occupied by the Sun's atmosphere and dominated by the outflow of the solar wind. The periods of primary scientific
interest is when Ulysses was at or higher than 70 degrees latitude at both the Sun's south and north poles. Ulysses launched on October 6, 1990 and
in June 1994 it began a four-month observation from high latitudes of the complex forces at work in the Sun's outer atmosphere-the corona.
Originally, Ulysses was to provide data regarding the heliosphere, the solar winds, the Sun’s magnetic field, plasma waves and galactic cosmic rays
but it turned out to do more than that, measuring solar wind fields, particles and cosmic rays along with gas and dust particles.
As early as 1992, data was flowing in regarding stardust:
The stardust is embedded in the local galactic cloud through which the Sun is moving at a speed of 26 kilometres every second. As a result of
this relative motion, a single dust grain takes twenty years to traverse the Solar System. Observations by the DUST experiment on board Ulysses have
shown that the stream of stardust is highly affected by the Sun's magnetic field.
Curiously, it was found that during the 90’s, the field was keeping most of this dust out. Reports from 2002 however, showed that the shield had
lost most of its power during the solar maximum and more dust was getting through, as much as three times more.
Here is a graphic showing where the dust flows, whether we are at a solar maximum or a solar minimum:
The pictures above show cut-aways of where interstellar dust is concentrated in the Solar System - high concentration: red/yellow, low
concentration: blue/green (the planets are not shown). During solar minimum (top picture) most interstellar dust can be found above or below the Sun,
while at the solar maximum (bottom picture) the dust is concentrated close to the Sun in the plane of the planets' orbits.
Heading for a maximum again, in 2005 they proclaimed that we could expect to see more of this interstellar dust coming through. Interesting to note
that each year, we have roughly 40000 tons of dust showering on us, from asteroids and comets.
It is possible that the increase of stardust in the Solar System will influence the amount of extraterrestrial material that rains down to
Earth.
Cool stuff huh?
Then in 2008...it breaks the news...
Ulysses spacecraft data indicate solar system shield lowering.
23 September 2008: Data from the joint ESA/NASA Ulysses mission show that the Sun has reduced its output of solar wind to the lowest levels since
accurate readings have become available. This current state of the Sun could reduce the natural shielding that envelops our Solar System.
Again, it is interesting to note that such an event had never occurred since space age exists. Consequences of this shield lowering are simple. More
dust is flowing in; more cosmic rays are coming through.
The more constant cosmic rays coming through means more particles being hit within our atmosphere, which could explain the increase in the Beryllium
data provided in this research.
Now from what we know, from what the current data is providing, we could be entering a zone where the cloud is denser. We could also be entering a
zone of our galaxy where the space is denser. As the bowshock has turned into a bow wave, as the heliosphere is weakened, as more cosmic rays and
interstellar dust are getting through to us, it is far from insane to think that we might be heading for a new ice age or at the very least, a mini
ice age.
It becomes more and more factual and this does affect us all.
Sources
www.nasa.gov...
science.nasa.gov...
sci.esa.int...
sci.esa.int...
www.esa.int...