Thursday, August 11, 2011

The Alpha Magnetic Spectrometer Experiment )02

Credit: NASA/JSC, NASA

During the 14-day mission, Endeavour delivered the Alpha Magnetic Spectrometer (AMS) and spare parts including two S-band communications antennas, a high-pressure gas tank and additional spare parts for Dextre. This was the 36th shuttle mission to the International Space Station. STS-134 Mission Information



See:

HOW LONG – THE STORY OF AMS-02

July 31st, 2011 
In this video 16 years of preparation of AMS-02 become few blinks. The construction of AMS-02 is the result of a  worldwide effort undertaken by scientists from 16 different countries who now started analyzing the wealth of data downlinked from the ISS, looking for new, unexpected phenomena.

For me, following the story "on land"  by our own  innovators to understanding the energy valuations outputs and the many tree designs as Feynman pathways of particulate expressions has been very interesting. The pathways are designated motivation-ally and expressively, to see and reveal the level of experimental verification needed in looking at the results for confirm hypothesis and theoretical expectations. Proposals on what we might find. In AMS case and in Fermi,  we are counting these motivations from not only our sun , but from deep space as well.

See: BaBar: evidence for a charged Higgs boson

So in a sense should one also collaborate with what one can evaluate out in space with what one is evaluating on the ground with regard to Babar and LHC?

Any thoughts or opinions on that?

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