ISON: Exis+ng Structure, Tasks, Characteris+cs and Further Development
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1 Russian Academy of Sciences Keldysh Ins+tute of Applied Mathema+cs ISON: Exis+ng Structure, Tasks, Characteris+cs and Further Development Molotov I., Agapov V., Akim E., Sukhanov S. Keldysh Ins+tute of Applied Mathema+cs, RAS 8 th US/Russian Space Surveillance Workshop April 2010, Wailea, Maui
2 ISON: Interna+onal scien+fic op+cal network - main goal is providing an open source of informa+on about space objects accessible for scien+fic analysis Current primary tasks: - regular GEO monitoring, new objects discovering and tracking, maintenance as complete GEO objects database as possible - new objects on GTO and other HEO regimes discovering and individual tracking, special HEO surveys will start soon - determining of possible origin of the discovered objects - analysis of poten+ally dangerous situa+ons in GEO
3 ISON milestones:
4 Interna+onal scien+fic op+cal network Green and Blue circles ISON observatories Orange circles other Russian observatories providing follow up observations Red circles foreign observatories collaborating with the ISON Yellow and White circles ISON observatories in preparation
5 Interna+onal scien+fic op+cal network
6 ISON structure network of op+cal facili+es: - search and survey subsystem for surveys of the GEO region (par+ally opera+onal) - subsystem for high orbit faint (fainter than 15.5 m ) space debris tracking (opera+onal) - subsystem for tracking of bright GEO and HEO objects (in development) network opera+on suppor+ng groups: - electric and so\ware engineering (Pulkovo observatory) - op+cal and mount engineering (SPE Project- Technics ) - observa+on planning and data processing (KIAM, Vympel and KMZ) - network development (KIAM) 20 new telescopes and 35 GPS- based +ming devices are produced, 30 CCD cameras are purchased, standard so\ware for CCD frames reduc+on and telescope equipment control is elaborated
7 Search and survey subsystem for the GEO region: nine cm telescopes with FOV of degree
8 Subsystem for tracking of bright GEO and HEO objects: Ussuriysk, Uzhgorod, Abastumani, Artem, Lesosibirsk, Nauchny- 2, TamDao
9 Subsystem for faint debris tracking: AT- 64 Nauchny- 1, RC- 600 Mayaki, S- 600 Andrushivka, ZIMLAT Zimmerwald, AZT- 14 Mondy, AS- 32 Abastumani, Zeiss- 600 Arkhyz, AZT- 8 Gissar
10 Subsystem for very faint debris tracking down to 21m: 2.6 m ZTSh Nauchny- 1, Zeiss Teide, Zeiss Terskol, 1.7 m AZT- 33IK Mondy, 1.25 m ZTE Nauchny- 2
11 Total (all objects) GEO Debris
12
13 Observed HEO Objects Number (by day, Jan- Nov 2009 г.)
14 Distribu+on of discovered 556 fragments by telescopes (341 objects / 215 uncorrelated tracks)
15 Current ISON performances more 30 telescopes in 20 observatories of 10 countries Control of full GEO arc uncatalogued GEO debris search (using different strategies, limi+ng magnitude 19 m ) and tracking (limi+ng magnitude 21 m ) measurements with precision of to determine the high accuracy orbits for close encounters analysis GTO and other HEO objects observa+ons including faint space debris observa+ons of new lunches at GEO and HEO Third switching on of DM- SLB Telstar- 11N
16 Future ISON development improving of the faint fragment search and tracking ability across full GEO arc pumng into opera+on of series of 40- cm 80- cm telescopes improving of western hemisphere coverage - involving of observatories in Chile, Mexico, Brasilia, New Zealand is under considera+on upgrading 1- m Zeiss in Sanghlok, Tajikistan star+ng the special HEO surveys using lens objec+ves with FOV of degrees
17 Future development improving of the faint fragment search ability across full GEO arc
18 Future ISON development
19 Outlook ISON is obtaining large volume of measurements on high orbit space objects on regular basis about 15 addi+onal telescopes will be puned into opera+on during it will allow independent con+nuous tracking of all objects larger than 1 m in size and about 90% of objects larger than 0.5 m in size along all GEO arc and improved capability to detect and to track faint GEO and HEO objects with magnitude down to 21 m next stage of ISON development foresees monitoring of GTO, Molniya and other types of HEO
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