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The top documents tagged [magnetic field variation]
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magnetic field variation
March 2006 The International Linear Collider at the IP – from feedback hardware to electromagnetic backgrounds FONT collaboration P Burrows, G Christian,
213 views
R Scrivens, CERN, ABI Workshop, 12/2008 The Feschenko Bunch Shape Monitor User experience at CERN Developed by INR, Troitsk. High resolution bunch shape.
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Dissipation of Alfvén Waves in Coronal Structures Coronal Heating Problem T corona ~10 6 K M.F. De Franceschis, F. Malara, P. Veltri Dipartimento di Fisica.
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Characteristics of VLF Tweeks Nedra Tounsi & Hassen Ghalila Laboratoire de Spectroscopie Atomique Moléculaire et Applications 1 In this spectrogram recorded.
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March 25, 2004 IRIS Seismometer Workshop1 Testing & Testing Facilities – charge to breakout group nWho/where are current testing facilities? Do we need.
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Testing & Testing Facilities – charge to breakout group
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Solar Atmosphere as a Laboratory for Magnetic Reconnection Shinsuke Imada (ISAS/JAXA)
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Chapter Ⅰ USM. Definition Of USM USM is able to effectively machine all hard materials whether they are electrically conductive or not. USM is able to.
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Solar Atmosphere as a Laboratory for Magnetic Reconnection
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The Feschenko Bunch Shape Monitor User experience at CERN
77 views
Testing & Testing Facilities – charge to breakout group
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