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Electric solar wind sail - propelling the future
Pekka Janhunen Finnish Meteorological Institute, Helsinki Finnish Cospar 50 years anniversary seminar FMI auditorium, June 2, 2014
Electric solar wind sail - propelling the future Finnish Cospar 50 - - PowerPoint PPT Presentation
Electric solar wind sail - propelling the future Finnish Cospar 50 years anniversary seminar FMI auditorium, June 2, 2014 Pekka Janhunen Finnish Meteorological Institute, Helsinki 1 Contributors Petri Toivanen, Jouni Envall, Jouni Polkko,
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Pekka Janhunen Finnish Meteorological Institute, Helsinki Finnish Cospar 50 years anniversary seminar FMI auditorium, June 2, 2014
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Petri Toivanen, Jouni Envall, Jouni Polkko, Sini Merikallio, Henri Seppänen (Finnish Meteorological Institute), Pekka Salminen (SkyTron, Finland), Edward Haeggström, Timo Rauhala, Jukka Ukkonen, Göran Maconi (Univ. Helsinki, Finland), Sergiy Kiprich (NSC Kharkov Inst. Physics, Ukraine), Hannu Koivisto, Olli Tarvainen, Taneli Kalvas (Univ. Jyväskylä, Finland), Alexander Obraztsov (Univ. Eastern Finland at Joensuu, and Moscow State Univ.), Greger Thornell, Sven Wagner, Johan Sundqvist (ÅSTC, Uppsala, Sweden), Tor-Arne Grönland, Håkan Johansson, Kristoffer Palmer (Nanospace AB, Uppsala, Sweden), Emil Vinterhav (Swedish Space Corporation&ECAPS), Roland Rosta, Tim van Zöst (DLR-Bremen, Germany), Mart Noorma, Viljo Allik, Silver Lätt, Urmas Kvell (Univ. Tartu, Estonia), Giovanni Mengali, Alessandro Quarta, Generoso Aliasi (Univ. Pisa, Italy), Salvo Marcuccio, Pierpaolo Pergola, Nicola Giusti (Alta S.p.A., Pisa, Italy), Giuditta Montesanti (Univ. Roma Tre, Rome, Italy), Jose Gonzalez del Amo, Eduard Bosch- Borras (ESA/ESTEC)
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– Electron gun is simpler than ion gun – No limitation on voltage by electron field emission – No photoelectron emission
– Usually can use satellite body as balancing electrode – Negative tether gathers less plasma current (ions versus electrons) – Photoelectron current is much less than plasma current
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– Thrust 0.5 mN/km at 20 kV in average solar wind at 1 au – Thrust scaling ~1/r (r=solar distance) – Electron gun power consumption ~0.7 W/mN, scales ~1/r²
– Thrust ~0.05-0.1 mN/km at 1 kV at 800 km LEO – Power consumption ~2 W/mN – Thrust likes oxygen (Pdyn~mi where Pdyn=minov²)
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Remote Unit Auxiliary Tether
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– Voltage “low” (~1 kV), photoelectron current negligible ==> can use negative tether – Negative polarity uses less power than positive
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– Only needs solar wind to work – Thrust direction controllable 0-30° off radial – Thrust magnitude ~1/r, 100% throttling capability
– Multi-asteroid touring – Giant planet entry & flyby – Non-Keplerian orbits – “Data clippers” – Asteroid mining
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– Off-Lagrange point solar wind monitoring (space weather forecasting with longer than 1 hour warning time) – Watching Earth-approaching NEOs and pseudomoons – High elliptic orbit whose apogee is locked to morning sector – Various orbits having view to polar regions
– Lifted orbit above ecliptic plane (helioseismology of Sun's poles) – Jupiter aurora study: Stay above Jupiter-Sun Lagrange L1 point: continuous view to Jupiter's polar aurora and in-situ solar wind measurement (for other giant planets as well)
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– If one wants to have a Mars probe, one must buy an escape- capable launcher (and then one pays 40 Meur and gets >1 tonne) – One could add piggyback payloads, but they will all be destined to the same planet, e.g. Mars – One could use ion engine, but...
– Enables small and cheap planetary/solar system probes
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