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GENESIS and the Future

This instrument flew on three missions SOHO, WIND, and ACE, where it has returned information about solar wind isotopes confirming the meteoritical abundances for the proto-solar nebulae [27], as well as identifying boundaries in the solar wind. With more than enough resolution to detect 170, why then was the GENESIS mission funded to return samples of the solar wind [22] Well, the problem turned out to be the C-foil once again. [Pg.264]

Neugebauer and R. von Steiger. The Solar Wind, in The Century of Space Science, J. A. M. Bleeker, M. Huber, J. Geiss (eds.), Springer, 2001. [Pg.264]

Newell, E. Homer. Beyond the Atmosphere Early Years of Space Science, 1980. [Pg.264]

Associations of Geomagnetic Activity with Plasma Sheet Thinning and Expansion—A Statistical Study, J. Geophy. Res., 89(1984) 5471-5478. [Pg.264]

Klecker, E. Moebius, D. Hovestadt, M. Scholer, and G. Gloeckler. Discovery of Energetic Molecular Ions (NO+ and 02+) in the Storm Time Ring Current, Geophys. Res. Lett., 13(1986) 632-635. [Pg.264]


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