ALL POINTS ALERT CERN LHC: The primary goal of CLOUD is to understand the influence of galactic cosmic rays

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ALL POINTS ALERT CERN LHC: The primary goal of CLOUD is to understand the influence of galactic cosmic rays

The primary goal of CLOUD is to understand the influence of galactic cosmic rays (GCRs) on aerosols and clouds, and their implications for climate.

Atmospheric aerosols and their effect on clouds are poorly understood and yet important for climate. Indeed, they are recognised by the Intergovernmental Panel on Climate Change (IPCC 2013 (link is external)) as the largest source of uncertainty in present radiative forcing and in climate projections over the 21st century.

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Although its design is optimised to address the cosmic ray question, CLOUD is the first experiment to reach the demanding technological performance and ultralow contaminant levels necessary to be able to measure aerosol nucleation and growth under controlled conditions in the laboratory. Consequently CLOUD has become the world’s leading laboratory experiment to address not only the influence of cosmic rays on aerosol-cloud processes but also more general and equally poorly understood aspects.

At the heart of the experiment is a stainless steel chamber of volume 26m3. This is surrounded by state of the art instrumentation measuring the gases and particles inside. The chamber is filled with synthetic air made from liquid nitrogen and liquid oxygen. Small quantities of other gases such as sulphur dioxide or organic compounds are added, and aerosol particles are formed and characterised.

Experiments often focus on measuring the rate of formation of aerosol particles with different mixtures of gases in the chamber, and investigating the effect of ionisation on this formation rate. The ionisation produced by cosmic rays can be enhanced with a high energy particle beam from the CERN Proton Synchrotron, or removed with a strong electric field. In addition, if the humidity inside the chamber is close to 100%, cooling achieved by fast adiabatic expansion can be used to make clouds in the chamber. At warm temperatures, this allows chemical processes inside cloud droplets to be studied and, at lower temperatures, experiments on ice microphysics are carried out.

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Supervolcano discovered at the North Pole — Mount Dutch undersea super volcano caldera

An earthquake swarm broke out near the North pole over the past few days (May 21-23, 2016).

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Upon inspection of the area, I found an UNNAMED supervolcano at the Northernmost portion of the Mid-Atlantic Ridge, at the tip of the North Pole.
Coordinates of the caldera here:

81 32 38.90 N , 119 48 1.02 E

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I hearby declare that the unnamed / undiscovered super-volcano at the North Pole, the location of the earthquake swarm currently happening… is now to be called Mount Dutch.

The supervolcano resides at the far North Tip of the North Mid-Atlantic ridge, and is not just a “volcanic field” like the professionals have reported.

A supervolcano caldera measuring 110km / 68 miles long, and 48km / 30 miles wide is at the location in question.

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In perspective, this supervolcano is larger than Toba Supervolcano in Indonesia, and greater than the overall size  of Yellowstone in Wyoming.

Toba Supervolcano is approximately 60 miles long and 25 miles wide.

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Yellowstone Supervolcano is approximately 60 miles across (100km).

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As the discoverer of this undersea supervolcano at the North Pole, I think it would be very prudent at this point to begin a study of the location in detail.

Hopefully we can find out much more about this location now that we’ve determined a super-volcano caldera is present.

The “Mount Dutch” North Pole supervolcano caldera needs MUCH more investigation.


Earthquake swarm information at the North Pole from the USGS:

http://earthquake.usgs.gov/earthquakes/eventpage/us10005j89#general

http://earthquake.usgs.gov/earthquakes/eventpage/us10005j67#general