The Observatorio Astronómico Nacional – San Pedro Márur Network
Transcription
The Observatorio Astronómico Nacional – San Pedro Márur Network
The Observatorio Astronómico Nacional – San Pedro Már;r Network Ba n d w i d t h Michael Richer Observatorio Astronómico Nacional-‐San Pedro Már;r Ins;tuto de Astronomía -‐ Ensenada Universidad Nacional Autónoma de México What/where is the OAN-‐SPM? • The observatory is basically a small village: – 4.5 hours from Ensenada – 20-‐25 people – food, water brought in – generates its own power – microwave internet link 11 October 2013 M. Richer -‐-‐ CICESE, Big Data Big Network 2 History • In the early 1990s, a satellite link was installed. • The bandwidth was 64 kbits/second. • Telephone service was half duplex. • Later, the bandwidth was doubled with full duplex telephone service. 11 October 2013 M. Richer -‐-‐ CICESE, Big Data Big Network 3 Today • In early 2003, a microwave link was installed by TelNor. • The bandwidth is 2 Mbits/second. • VOIP telephone service was installed. unknown photographer, provided by Urania Ceseña 11 October 2013 M. Richer -‐-‐ CICESE, Big Data Big Network 4 Today • Light use: – telephone service – general use • Intensive use: – data transmission • Only the RATIR instrument produces a large data volume. The condor’s view… • RATIR is a collabora;on unknown photographer, between UNAM, UC, ASU, provided by Urania Ceseña and NASA/Goddard. 11 October 2013 M. Richer -‐-‐ CICESE, Big Data Big Network 5 Today, RATIR • The RATIR instrument: – 4 channel imaging (2 in visible; 2 in the infrared) – robo;c telescope (1.5m telescope) – data volume: 22 Gbytes/night – the data are sent to Ensenada: • impossible without compression • with compression, 100% of the bandwidth for 10 hours/day • With the current microwave link, we cannot confront a substan;ally larger data volume. • An upgrade to 10 Mbits/second is planned within the next few months. 11 October 2013 M. Richer -‐-‐ CICESE, Big Data Big Network 6 Future (star;ng now) • TAOS II (under construc;on; ASIAA/Taiwan, Harvard/CfA) – 3 robo;c telescopes, advanced cameras (20 Hz frame readout) – 4 Tbytes/night – a fibre op;c link is needed • Boötes-‐5 (2014; Ins;tuto de Astroksica de Andalucía) – robo;c telescope with wide-‐field camera – 35 Gbytes/night – feasible with upgraded microwave link and compression • Flash (2015; French partners) – robo;c telescope, similar instrumenta;on as RATIR – 25 Gbytes/night – feasible with upgraded microwave link and compression? • SPMT (2014+?; INAOE and American partners): – 6.5m telescope, advanced instrumenta;on – 30-‐50 Gbytes/night, first genera;on instruments – probably requires a fibre op;c link (SASIR will, > 1Gbit/second) 11 October 2013 M. Richer -‐-‐ CICESE, Big Data Big Network 7 Future • Cherenkov Telescope Array (2015+?; Mexican, European, and American partners) – array of 25 Cherenkov telescopes – 10 Tbytes/observa;on (¡!), only reduced data will be transmired, – requires a fibre op;c link. • With CFE, we are planning to build an electricity line to connect the OAN-‐SPM to the na;onal electricity grid. • This connec;on will also include a fibre op;c link to Ensenada. • For now, the bandwidth specifica;on is 100 Mbits/second, but can be upgraded with signal repeaters (TAOS-‐II will need 410 Mbits/second). 11 October 2013 M. Richer -‐-‐ CICESE, Big Data Big Network 8 Ensenada’s Connec;vity • CICESE and UNAM share a 10 Gbits/second link from Ensenada to Tijuana/San Diego for na;onal/ interna;onal traffic. • This link will be important for the instruments that will come online at the OAN-‐SPM in the next few years. • This link is also important now for the compu;ng needs of the theore;cal astronomers in Ensenada, whose connec;vity to compu;ng resources in central Mexico have been limited. 11 October 2013 M. Richer -‐-‐ CICESE, Big Data Big Network 9 11 October 2013 M. Richer -‐-‐ CICESE, Big Data Big Network 10 11 October 2013 M. Richer -‐-‐ CICESE, Big Data Big Network 11