'Magnetic field measurements' presentation slideshows

Notes:

Notes: In many of the Fourier transforms the frequency is given in c/d = cycles per day. To convert to m Hz multiply numbers by 11.57 HD 101065 has a period of ~12 minutes. If you use Period04 on the data this corresponds to ~118 c/d. Rapidly Oscillating Peculiar Magnetic A stars.

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Lecture 12: Giant Planet Moons and Rings

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Hermean environment

BepiColombo : a tool for Hermean Environment investigation Anna Milillo ( INAF/ Istituto di Fisica dello Spazio Interplanetario ).

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ATST Science Requirements

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What Studies Have Been Done About AR 10930 ?

What Studies Have Been Done About AR 10930 ?. Presented by Sung-Hong Park NJIT / SWRL. Published Papers ( more than 27 ). Published Papers ( continued ). Overview of NOAA 10930. Hinode/FG/ G-band. Hinode/FG/ Ca II H. Hinode/FG/ Stokes-V. LASCO/C2. Hinode/ XRT. LASCO/C2.

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Satellite Missions and Observations

Satellite Missions and Observations. Dan Gershman SHINE Student Day 7/10/2011. This talk. Overview What makes each spacecraft dataset important? Where can you get all this data? Summary. Overview of current missions. http://science.nasa.gov/missions/.

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MICE project board IV response to charge and MPB questions

MICE project board IV response to charge and MPB questions. These questions have been answered by S. Gourlay and reproduced in the written document. See plan description in the report. It should be stressed that this requires 4 new people

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EXPERIMENTAL MAGNETS COMMISSIONING

EXPERIMENTAL MAGNETS COMMISSIONING. LAYOUT. About the magnets Status and plans Commissioning of the dipoles Commissioning of the solenoids Atlas toroids and end caps. About the magnets. All experimental magnets are driven by standard FGC and power converter

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Lattice structure and misfit between substrate/buffer/YBCO conductor

Lattice structure and misfit between substrate/buffer/YBCO conductor. Conductive buffer layers. Twisted conductor. - large circulating currents can exist among the filaments due to connections at the ends (in current leads)

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Space Weather: Magnetic Storms 31 October 2011

C/NOFS. DMSP. Space Weather: Magnetic Storms 31 October 2011. William J. Burke Air Force Research Laboratory/Space Vehicles Directorate Boston College Institute for Scientific Research. CRESS. Space Weather Course Overview. Lecture 1: Overview and Beginnings Lecture 2: The Aurorae

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Production schedule and cost estimation of the BINP full-scale prototype wiggler

Production schedule and cost estimation of the BINP full-scale prototype wiggler. Alexey Bragin, Budker Institute of Nuclear Physics, Novosibirsk, Russia December 2010. Tested short prototype. Review. Short prototype of NbTi wiggler was tested in August 2010. Its parameters are:

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Issues

Issues. A0 beam is 16 MeV. NML beam will be up to 50 MeV. Are the present set of A0 magnets adequate for the higher beam energy at NML? Limitations could be temperature, or fringe field, or ....

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Laser Magnetized Plasma Interactions for the Creation of Solid Density Warm (~200 eV) Matter

II. HOT ELECTRON CONFINEMENT. I. ABSTRACT.

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