Station
Similar stations in BD-02 4304
Surface Port - 110 Ls
Democrats of BD-02 4304
Bean Enterprise
Starport (Coriolis) - 138 Ls
Social Eleu Progressive Party
Simak Town
Surface Port - 142 Ls
Democrats of BD-02 4304
Gell-Mann Dock
Starport (Coriolis) - 159 Ls
Social Eleu Progressive Party
Durrance Station
Starport (Coriolis) - 298 Ls
BD-02 4304 Gold Major Holdings
Tanner Installation
Surface Port - 877 Ls
Social Eleu Progressive Party
Brandenstein Enterprise
Outpost (Civilian) - 904 Ls
BD-02 4304 Gold Major Holdings
Currie Terminal
Outpost (Civilian) - 5,686 Ls
Social Eleu Progressive Party
Fabian Dock
Outpost (Civilian) - 5,688 Ls
Democrats of BD-02 4304
Newton Dock
Starport (Orbis) - 5,732 Ls
Social Eleu Progressive Party
Abbott Arsenal
Surface Port - 6,448 Ls
Social Eleu Progressive Party
Galpedia
Eugene Parker
Eugene N. Parker (born June 10, 1927) is an American solar astrophysicist who received his B.S. degree in physics from Michigan State University in 1948 and Ph.D. from Caltech in 1951. In the mid-1950s Parker developed the theory on the supersonic solar wind and predicted the Parker spiral shape of the solar magnetic field in the outer solar system. In 1987, Parker proposed that the solar corona might be heated by myriad tiny "nanoflares", miniature brightenings resembling solar flares that would occur all over the surface of the Sun.
Parker was elected to the National Academy of Sciences in 1967. As of early 2005, he was still engaged in active research at the University of Chicago. His daughter and son-in-law are both faculty members at Michigan State University.
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