Station

Star system
Power
-
Station distance
1,237 Ls
Landing pad
Large
Station type
Starport (Orbis)

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
Agriculture
Wealth
Population
Government
Corporate
Allegiance
Empire
Minor faction

Station update
15 Dec 2024, 11:54pm
Location update
13 Dec 2024, 2:58pm
Market update
21 Oct 2024, 2:25pm
Shipyard update
21 Oct 2024, 2:25pm
Outfitting update
08 Dec 2024, 2:10am

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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