Station

Star system
Station distance
699 Ls
Landing pad
Large
Station type
Starport (Coriolis)

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
Industrial
Wealth
Population
Large population
Government
Patronage
Allegiance
Empire

Station update
04 Nov 2024, 10:24pm
Location update
04 Nov 2024, 10:24pm
Market update
04 Nov 2024, 10:25pm
Shipyard update
04 Nov 2024, 10:24pm
Outfitting update
04 Nov 2024, 10:24pm

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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