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I worked in physics a few more years, then worked with the new architecture computers, rebuilding scientific simulation codes for parallel machines, and making new codes with unstructured meshes and dynamic load balancing (see 1993 below). I was co-author of a book Parallel Computing Works!. There was a lot of fluid-flow simulation on parallel computers, inculuding a simulation of the hypersonic flow around the Huygens space probe that landed on Saturn's moon Titan (paper).
The world-wide web arrived in the early 1990's, where I was an early adopter. In 1995, I gave a lecture and wrote an article about its potential. I was building web applications in 1996, delivering Earth remote-sensing data over the internet, where I wrote about what I called Hypermaps, a prequel to Google Maps.
I worked with the LIGO (gravitational waves) project in the late 1990's, introducing them to databases and XML, and built science gateways for the US Teragrid project. I was with the Virtual Observatory from the start, as architect, also creating in large part the VOTable and VOEvent standards, now widely used. There was a lot of work on astronomical transients, leading up to the Palomar Transient Factory and preliminary work on LSST, realizing that soon the transient detections would overwhelm the ability of telescopes to observe them all. I worked again for the LIGO group from 2010, developing the Gravitational Wave Open Science Center. I was lucky enough to be at Caltech when the first detection happened, with all its excitement, and I wrote this account of LIGO is Awesome and This is Why.
The world-wide web arrived in the early 1990's, where I was an early adopter. In 1995, I gave a lecture and wrote an article about its potential. I was building web applications in 1996, delivering Earth remote-sensing data over the internet, where I wrote about what I called Hypermaps, a prequel to Google Maps.
I worked with the LIGO (gravitational waves) project in the late 1990's, introducing them to databases and XML, and built science gateways for the US Teragrid project. I was with the Virtual Observatory from the start, as architect, also creating in large part the VOTable and VOEvent standards, now widely used. There was a lot of work on astronomical transients, leading up to the Palomar Transient Factory and preliminary work on LSST, realizing that soon the transient detections would overwhelm the ability of telescopes to observe them all. I worked again for the LIGO group from 2010, developing the Gravitational Wave Open Science Center. I was lucky enough to be at Caltech when the first detection happened, with all its excitement, and I wrote this account of LIGO is Awesome and This is Why.
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Roy D. Williams, Gareth P. Francis,Andy Lawrence, Terence M. Sloan, Stephen J. Smartt,Ken W. Smith,David R. Young
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