Station

Star system
Station distance
869 Ls
Planet
BD-02 4304 AB 4 c
Landing pad
Large
Station type
Surface Port

Station services
Commodity marketOutfittingRearmRefuelRepairShipyard

Black marketContactsFleet carrier administrationFleet carrier servicesFleet carrier vendorInterstellar factorsMaterial traderPower contactRedemption officeSearch and rescueTechnology brokerUniversal CartographicsVendorsWorkshop

BartenderConcourseCrew loungeFrontline SolutionsMissionsPioneer SuppliesTuningVista Genomics


Economy
Colony
Wealth
Population
Government
Democracy
Allegiance
Federation

Station update
13 Nov 2024, 2:01pm
Location update
13 Nov 2024, 2:01pm
Market update
13 Nov 2024, 2:02pm
Shipyard update
10 Nov 2024, 7:59pm
Outfitting update
10 Nov 2024, 7:59pm

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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