The top documents tagged [stored magnetic energy]

PED Syllabus Final
Documents PED Syllabus Final

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Approaching the Lower Bounds on Q for Electrically Small Electric-Dipole Antennas Using High Permeability Shells
Technology Approaching the Lower Bounds on Q for Electrically Small Electric-Dipole Antennas Using High Permeability Shells

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A giant flare from the magnetar SGR 1806-20 -- a tsunami of gamma-rays Søren Brandt Danish National Space Center
Documents A giant flare from the magnetar SGR 1806-20 -- a tsunami of gamma-rays Søren Brandt Danish National Space Center

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New Results for Minimum Q, Maximum Gain, and Polarization Properties of Electrically Small Arbitrary Antennas Professor David M. Pozar Electrical and Computer
Documents New Results for Minimum Q, Maximum Gain, and Polarization Properties of Electrically Small Arbitrary Antennas Professor David M. Pozar Electrical and Computer

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SDO Project Science Team 1 The Science of SDO. SDO Project Science Team 2 Sensing the Sun from Space High-resolution Spectroscopy for Helioseismology
Documents SDO Project Science Team 1 The Science of SDO. SDO Project Science Team 2 Sensing the Sun from Space High-resolution Spectroscopy for Helioseismology

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EEE340Lecture 261 Internal inductance versus external inductance Example. Magnetic-Head Connector (MHC) Configuration of high speed magnetic head connector
Documents EEE340Lecture 261 Internal inductance versus external inductance Example. Magnetic-Head Connector (MHC) Configuration of high speed magnetic head connector

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PIMS, July 2009 The Solar Dynamics Observatory:Waiting for a Launch Solar Cycle 24 Aleya Van Doren W. Dean Pesnell Steele Hill NASA, Goddard Space Flight
Documents PIMS, July 2009 The Solar Dynamics Observatory:Waiting for a Launch Solar Cycle 24 Aleya Van Doren W. Dean Pesnell Steele Hill NASA, Goddard Space Flight

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Switched Reluctance Motors
Documents Switched Reluctance Motors

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Hydrostatic model ling of active region EUV and X-ray emis sion
Documents Hydrostatic model ling of active region EUV and X-ray emis sion

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antennasfundamentalv2.pdf
Documents antennasfundamentalv2.pdf

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- Preliminary results from temperature modeling using the CIII 97.7 nm / CIV 155 nm line ratio give an average plasma temperature of 25 eV early in counter-helicity
Documents - Preliminary results from temperature modeling using the CIII 97.7 nm / CIV 155 nm line ratio give an average plasma temperature of 25 eV early in counter-helicity

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ILWS Workshop, Ubatuba, Brazil, October 2009 The Solar Dynamics Observatory:Waiting for a Launch Solar Cycle 24 W. Dean Pesnell NASA, Goddard Space Flight
Documents ILWS Workshop, Ubatuba, Brazil, October 2009 The Solar Dynamics Observatory:Waiting for a Launch Solar Cycle 24 W. Dean Pesnell NASA, Goddard Space Flight

214 views