SETI Presentation - OSCON 2011
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Presentation by Avinash Agrawal (SETI Institute) and Francis Potter (The Hathersage Group) at OSCON 2011 about open source initiatives connected to the Search for Extraterrestrial Intelligence.
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SETI Presentation - OSCON 2011
- 1. Open Source SETI Avinash Agrawal, SETI Institute Francis Potter, The Hathersage Group
- 11. SETI Institute Founded 1984 150 Scientists, Researchers and Staff Mission: Explore, Understand and Explain the Origin, Nature and Prevalence of Life in the Universe.
- 12. SETI Institute Founded 1984 150 Scientists, Researchers and Staff Mission: Explore, Understand and Explain the Origin, Nature and Prevalence of Life in the Universe.
- 14. Kepler
- 15. Kepler
- 16. Kepler
- 17. Kepler
- 18. Kepler
- 20. Astrophysics vs. Technology Hydroxyl (OH) Maser IRC + 10420 1.0 MHz Spacecraft 0.1 MHz 924 channels Time 0.001 MHz
- 22. Allen Telescope Array Hat Creek Observatory
- 23. Allen Telescope Array Hat Creek Observatory
- 24. Allen Telescope Array Hat Creek Observatory
- 25. Allen Telescope Array Hat Creek Observatory
- 27. Wide Band Digitizer Wide Band Digitizer Data Archive 2 Wide Band Digitizer SonATA Wide Band Digitizer
- 28. Wide Band Digitizer Wide Band Digitizer Data Archive 2 Wide Band Digitizer SonATA Wide Band Digitizer Beamformer Data (new SETI algorithms and radio astronomy) - 100 MHz x 2 Pol. x 16 bits (complex) = 3 Gb/s - 1.4 TB per hour
- 29. Wide Band Digitizer Wide Band Digitizer Data Archive 2 Wide Band Digitizer SonATA Wide Band Digitizer Beamformer Data (new SETI algorithms and radio astronomy) - 100 MHz x 2 Pol. x 16 bits (complex) = 3 Gb/s - 1.4 TB per hour Raw Data (software beamformer and correlator) - 1.4 TB/hour x 42 antennas = 59 TB/hour
- 32. I wish that you would empower Earthlings everywhere to become active participants in the ultimate search for cosmic company. - Jill Tarter
- 33. I wish that you would empower Earthlings everywhere to become active participants in the ultimate search for cosmic company. - Jill Tarter
- 36. ATA Observing
- 37. ATA Observing SonATA
- 38. ATA Observing SonATA
- 39. ATA Observing SonATA
- 40. ATA Observing SonATA Explorer
- 41. ATA Observing SonATA Explorer
- 42. ATA Observing SonATA Data Explorer
- 43. ATA Observing SonATA Data Apps Explorer
- 44. ATA Observing SonATA Data Apps Explorer
- 45. SonATA SonATA SETI ON the ATA SETI ON the ATA
- 50. GSoC: Porting to Multiple Linux Platforms GSoC: Implementing new signal detection algorithms Telescope Simulator 3D Antenna Visualization
- 72. setiQuest Explorer Search “SETI” on Android Market Browse http://explorer.setiquest.org Check out code at https://github.com/hathersagegroup/seti SonATA / open data Download data from http://setiquest.org/getting-data Check out code at https://github.com/setiQuest/SonATA Contact Us Follow @francispotter or @setiinstitute Email francis@hathersagegroup.com or avinash@setiquest.org Browse http://www.setiquest.org
Hinweis der Redaktion
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- N = the number of civilizations in our galaxy with which communication might be possible;\n\nR* = the average rate of star formation per year in our galaxy\nfp = the fraction of those stars that have planets\nne = the average number of planets that can potentially support life per star that has planets\nfℓ = the fraction of the above that actually go on to develop life at some point\nfi = the fraction of the above that actually go on to develop intelligent life\nfc = the fraction of civilizations that develop a technology that releases detectable signs of their existence into space\nL = the length of time for which such civilizations release detectable signals into space.\n
- N = the number of civilizations in our galaxy with which communication might be possible;\n\nR* = the average rate of star formation per year in our galaxy\nfp = the fraction of those stars that have planets\nne = the average number of planets that can potentially support life per star that has planets\nfℓ = the fraction of the above that actually go on to develop life at some point\nfi = the fraction of the above that actually go on to develop intelligent life\nfc = the fraction of civilizations that develop a technology that releases detectable signs of their existence into space\nL = the length of time for which such civilizations release detectable signals into space.\n
- N = the number of civilizations in our galaxy with which communication might be possible;\n\nR* = the average rate of star formation per year in our galaxy\nfp = the fraction of those stars that have planets\nne = the average number of planets that can potentially support life per star that has planets\nfℓ = the fraction of the above that actually go on to develop life at some point\nfi = the fraction of the above that actually go on to develop intelligent life\nfc = the fraction of civilizations that develop a technology that releases detectable signs of their existence into space\nL = the length of time for which such civilizations release detectable signals into space.\n
- N = the number of civilizations in our galaxy with which communication might be possible;\n\nR* = the average rate of star formation per year in our galaxy\nfp = the fraction of those stars that have planets\nne = the average number of planets that can potentially support life per star that has planets\nfℓ = the fraction of the above that actually go on to develop life at some point\nfi = the fraction of the above that actually go on to develop intelligent life\nfc = the fraction of civilizations that develop a technology that releases detectable signs of their existence into space\nL = the length of time for which such civilizations release detectable signals into space.\n
- N = the number of civilizations in our galaxy with which communication might be possible;\n\nR* = the average rate of star formation per year in our galaxy\nfp = the fraction of those stars that have planets\nne = the average number of planets that can potentially support life per star that has planets\nfℓ = the fraction of the above that actually go on to develop life at some point\nfi = the fraction of the above that actually go on to develop intelligent life\nfc = the fraction of civilizations that develop a technology that releases detectable signs of their existence into space\nL = the length of time for which such civilizations release detectable signals into space.\n
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