INSTABILITY OF HIGHLY COLLISIONAL PLASMAS IN MAGNETIC FIELD: FROM THE LOWER EARTH’S IONOSPHERE AND METEORS TO SOLAR CHROMOSPHERE Y.S. Dimant and M.M. Oppenheim Center for Space Physics, Boston University - Jicamarca Radio Observatory - Document - PDFSEARCH.IO

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	INSTABILITY OF HIGHLY COLLISIONAL PLASMAS IN MAGNETIC FIELD: FROM THE LOWER EARTH’S IONOSPHERE AND METEORS TO SOLAR CHROMOSPHERE Y.S. Dimant and M.M. Oppenheim Center for Space Physics, Boston University Add to Reading List Document Date: 2014-01-24 14:14:55 Open Document File Size: 78,18 KB Share Result on Facebook Organization Boston University / LOWER EARTH’S IONOSPHERE AND METEORS TO SOLAR CHROMOSPHERE Y.S. Dimant and M.M. Oppenheim Center for Space Physics / / SocialTag Astrophysics Optical materials Plasma Ionosphere Electrojet Jicamarca Radio Observatory Astrophysical plasma Plasma physics Physics Space plasmas

INSTABILITY OF HIGHLY COLLISIONAL PLASMAS IN MAGNETIC FIELD: FROM THE LOWER EARTH’S IONOSPHERE AND METEORS TO SOLAR CHROMOSPHERE Y.S. Dimant and M.M. Oppenheim Center for Space Physics, Boston UniversityAdd to Reading List