PIRSA:14110103 Conference

DOI10.48660/14110103

Conference/School: EHT 2014

Crew, G. (2014). EHT Correlation. Perimeter Institute. https://pirsa.org/14110103

Crew, Geoffrey. EHT Correlation. Perimeter Institute, Nov. 13, 2014, https://pirsa.org/14110103 

@misc{ pirsa_PIRSA:14110103,
  doi = {10.48660/14110103},
  url = {https://pirsa.org/14110103},
  author = {Crew, Geoffrey},
  keywords = {},
  language = {en},
  title = {EHT Correlation},
  publisher = {Perimeter Institute},
  year = {2014},
  month = {nov},
  note = {PIRSA:14110103 see, \url{https://pirsa.org}}
}

Abstract

Over the next few years the Event Horizon Telescope will greatly expand its capabilities from the current 8 Gbps at a few sites to 64 Gbps at a much larger number of sites. The good news is that this processing can proceed through 4 independent (16 Gbps) processing stages of 2 GHz of bandwidth. The bad news is that EHT stations come in multiple "flavors" each posing its own issues for correlation with DiFX (the current correlation option). This talk will discuss some of the issues and the road ahead.

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