Edge Rewrite
// HTMLRewriter · presentation

This page was redesigned at the edge.

Cloudflare fetched the original article and streamed it through HTMLRewriter to apply an entirely new visual system without rebuilding the source page.

// request.cf · coarse context

A page that knows where it met you.

Only coarse request metadata is shown. This demo does not display or persist visitor IP addresses.

Country
US
Cloudflare location
CMH
Connection
HTTP/2
Language
Not provided

Ray ID: a22e553c4984879c

Jump to content

// Workers AI · dad joke modeWho's Ray Weymann? A ray of hope in a mann's world.

From Wikipedia, the free encyclopedia
Ray Weymann
Alma materCalifornia Institute of Technology, Princeton University
Scientific career
ThesisHeating of stellar chromospheres by shock waves and coronal evaporation as a possible mechanism for mass loss in red giants. (1960)

Ray Weymann is a retired astronomer and astrophysicist, associated with the Carnegie Institution of Washington. His PhD is from Princeton University. He is a founder of the Climate Science Rapid Response Team, a member National Academy of Sciences (1984),[1] and past president of the Astronomical Society of the Pacific 1973-1975.

He has made notable contributions to astronomy in the areas of the evolution of high redshift galaxies, and mass ejection from active galaxies. He was part of the team that first observed a gravitationally lensed quasar in 1979.

References

[edit]
  1. NAS Directory of members