SLAC Today is
available online at:
http://today.slac.stanford.edu
In this issue:
Making Heads or Tails of Comet Dust
Science Today: Towards a Global Effort on ILC Emittance Preservation Studies
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Thursday – March 9, 2006 |
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NASA's Stardust gathered material from the tail of a comet in January 2004
and returned to earth in January 2006. Making Heads or Tails of Comet DustLast week, a team of SSRL researchers began analyzing particles taken from the tail of a comet. The particles came from the Stardust NASA mission, which clipped the tail of comet Wild 2 (pronounced Vilt). Comet particles skidded through ultra-light aerogel and remained stuck there for the journey back to earth. SLAC is one of many laboratories identifying elements in the samples, which arrived from NASA in thin aerogel slices. “We are very excited to be mapping out the elemental abundance of the comet particles,” said SLAC's Sean Brennan. The purpose of the mission was to catch ancient unspoiled material from the tail of the Wild 2 comet that might tell about the birth of the solar system. As it is, scientists know very little about what makes up interplanetary material. Read more... |
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![]() Toward a Global Effort on ILC Emittance Preservation Studies
Therefore, more sophisticated methods called Beam-Based Alignment (BBA) must be used. In BBA, the beam itself is used as the diagnostic tool. BBA has been used extensively before, but the precision and lengths involved in the ILC are unprecedented. As a result, very detailed simulations are required to develop and confirm the performance of these BBA algorithms. A global effort has begun to critically analyze these BBA techniques and crosscheck their performance in the presence of both static and dynamic sources of misalignment. To do this, we are using various simulation codes from numerous laboratories from around the world including CERN, Cornell University, DESY, Fermilab and SLAC. These programs simulate the motion of the particle beam as it passes through the ILC. After various types of misalignments are introduced into the ILC computer model, the BBA algorithms are applied and the resultant beam size is calculated. We have currently completed a first stage of crosschecking and are beginning to get into the details of the various BBA algorithms. |
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