BEGIN:VCALENDAR VERSION:2.0 PRODID:-//Drupal iCal API//EN X-WR-CALNAME:Events items teaser X-WR-TIMEZONE:America/Toronto BEGIN:VTIMEZONE TZID:America/Toronto X-LIC-LOCATION:America/Toronto BEGIN:DAYLIGHT TZNAME:EDT TZOFFSETFROM:-0500 TZOFFSETTO:-0400 DTSTART:20230312T070000 END:DAYLIGHT BEGIN:STANDARD TZNAME:EST TZOFFSETFROM:-0400 TZOFFSETTO:-0500 DTSTART:20221106T060000 END:STANDARD END:VTIMEZONE BEGIN:VEVENT UID:683b3dab2defb DTSTART;TZID=America/Toronto:20231019T160000 SEQUENCE:0 TRANSP:TRANSPARENT DTEND;TZID=America/Toronto:20231019T170000 URL:/institute-for-quantum-computing/events/optical-gro und-station-oberpfaffenhofen-next-generation SUMMARY:Optical Ground Station Oberpfaffenhofen Next Generation: first\nsat ellite link tests with 80 cm telescope and AO system CLASS:PUBLIC DESCRIPTION:Summary \n\nIQC SEMINAR - JOHANNES PRELL\, INSTITUTE OF COMMUNI CATION AND\nNAVIGATION\, OSL GERMAN AEROSPACE CENTER (DLR) OBERPFAFFENHOFE N\,\nGERMANY\n\nQuantum Nano Centre (QNC) Room 0101 200 University Ave Wes t\, ݮƵ\nOntario\n\nSatellite based laser communication technology bo th classical and QKD\n(Q uantum K ey D istribution is gaining popularity a nd being\nincreasingly commercial i zed . Optical ground stations serve as the\nreceiv ing station in satellite to ground scenarios. The DLR institu te\nof Communications and Navigation hosts an experimental optical ground\ nstation for research and demonstration purpose. Supporting\nincreasingly demanding technical requirements from current and futu re\nmissions and te chnology demonstrations\, it was decided to replace the\n40cm Cassegrain t elescope an equip the new one with Nasmyth Ports for\ndirect experiments\, a Coudé Path to the lab and an Adaptive Optics\nSystem . This new 80cm ( 31.5inch) main apertur e diameter i nstrument\nis a Nasmyth Design Ritchey Chretien telescope The special feature is\nthe C oudé P ath which is gui ding the received light onto an optical\ntable in a lab oratory room below the telescope mount (see figure 1\nThe usage of the Coudé Path is new im plemented at DLR and offers a\nwide possibility for several different expe riments with the same setup\nThe optical propaga tion through a custom des igned lens system inside\nthe coudé path is optimized for wavelength s us ed for optical\ncommunication\, like 589nm\, 850nm\, 1064nm and 1550nm. It is possible to\nuse the setup as a receiving station and also as a transm itting\nfacility f or beacon lasers . The transmitt ing system ca n be\nin stalled either beside the telescope as a side installation or even\nlaunch ed from the optical table through coudé path and telescope\ndirectly\n\nT he optical Experiment table in the lab is equipped with an Adaptive\nOptic s ( System including fibe r coupling. This system uses a Shack\nHartmann W ave front sensor\, designed to match a deformable mirror in\nthe “ f rie d g eometry”. The system couples the light into a\nsingle mode fibe r \, which can be con nected to a coherent or Quantum\nencrypted communication s system. [ The telescope itself has four\nusable Nasmyth ports The first one is reserved for the coudé pa th\, t\nwo others are equipped with opti cal benches directly on the telescope\,\nand on the last one has a fixed c lassical laser communication\nreceiving setup including two cameras one vi sible light and one infra\nred and a signal receiving united is installed References\n\n[1] Andrew Paul Reeves\, Ilija R. Hristovski\, Alexandru Oct avian Duliu\,\nStefanie H äu sler\, Hela Friew Kelemu\, Pia Lützen\, Flo rian Moll\,\nEltimir Peev\, Juraj Poliak\, Amita Shrestha\, Joana Sul Torr es\; Adaptive\nOptics Corrected Bi Directional Links with a Geo Stationary Satellite\nfrom the DLR KN Optical Ground Station Figure 1 OGSOP System O vervi ew\n DTSTAMP:20250531T173435Z END:VEVENT END:VCALENDAR