NOSCI Infrastructure for Lunar Observatories Bremen, Germany March 22 – 24, 2005 NanOspace-1...
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Transcript of NOSCI Infrastructure for Lunar Observatories Bremen, Germany March 22 – 24, 2005 NanOspace-1...
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NOSCIInfrastructure for Lunar Observatories Bremen, Germany March 22 24, 2005NanOspace-1 SCientific InstrumentsJan Bergman Swedish Institute of Space Physics Uppsala, Sweden
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NanoSpace-1Mass < 10 kgIonospheric orbit, 400-1000 km
1 Mbps S-bandColdgas precision attitude control < 10mMassive use of Micro and Nano-TechnologyJan Bergman
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NOSCIEFVS Electric Field Vector SensorLP Langmuir ProbeARM Anisotropic magnetoResistive MagnetometerFGM FluxGate MagnetometerAB Antennas & Booms
Bremen, March 22 24, 2005Jan Bergman
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OrganizationJan BergmanBremen, March 22 24, 2005
InstrumentsContributorsInvestigatorsElectric Field Vector Sensor EFVSPhysics in space IRF, Uppsala, SwedenBo Thid Jan Bergman, Project managerLamgmuir Probe LPSpace plasma physics IRF, Uppsala, SwedenMats Andr Jan-Erik WahlundAnisotropic magnetoResistiv Magnetometer ARMSpace plasma physicsIRF, Uppsala, SwedenAnders Eriksson Lennart hlnFlux Gate Magnetometer FGMAlfvn Laboratory KTH, Stockholm, SwedenLars Blomberg Nickolay IvchenkoAntennas & Booms ABCBK, Warsaw, Poland IRF, Uppsala, Sweden STC, Uppsala, SwedenZbigniev Kos & Hanna Rotkael Jerzy Grygorczuk Lars StenmarkSpacecraft Interfaces CAN & SpaceWireSTC, Uppsala, Sweden IRF, Uppsala SwedenLars StenmarkJohan Khler, Project Manager Fredrik Bruhn
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Qualify micro and nanotechnology components Major step forward in the technical development of instrumentation for space science research.Qualify new sensors and boom systemsShrinking the electronics is not sufficient, sensors and boom systems must also follow suit.Test and verify new measurement methodsNew questions in space science, inspires the need to find new measurement methods. ObjectivesJan BergmanSpace science objectives are secondary
Bremen, March 22 24, 2005
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Unique capabilitiesDynamic 3D E-field vector, up to 20 MHzUnambiguous 3D wave polarization characteristicsStatistical properties, such as wave entropy, can be derived Major challengeAmount of Signal processing capabilities versus spacecraft heat and power requirementsThree different digital implementations are studiedLow mass1000 mm long extendible antenna, 2.7 gram
Electric Field Vector SensorJan BergmanBremen, March 22 24, 2005
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Langmuir ProbeUnique CapabilityPlasma density, n, and temperature, T, from DC to 10 kHzDigital signal generator makes it possible to measure local temperature (up to 10 kHz)Ion masses can be derivedDual probe experimentSimultanous measurements of electrons and ionsInterferometryTests of two different probe surface coatings (BepiColombo)Low mass273 mm long deployable boom, 0.7 gram5 mm Titanium probe, 0.3 gramJan BergmanBremen, March 22 24, 2005
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Anisotropic magnetoResistive MagnetometerUnique Capabilities3D magnetic field vector, B, from DC to 10 kHzSmall size and low massVolume 483.8 mm3 One gram for the whole instrumentExtremely interesting technology for future satellite and Lunar missionsFrequencies up to 7 MHzBad sensitivity 5-10 nTPrototype AMR sensors aquire 0.1 nT sensitivityPrototype Spin Dependent Tunneling (SDT) sensors < 1 pTMounting on a solar panel frameJan BergmanBremen, March 22 24, 2005
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FluxGate MagnetometerUnique Capabilities3D magnetic field vector, B, from DC to 100 HzMajor challengeMiniaturization of the sensorMaximum mass 10 gMaximum volume 20 20 20 mm3 Possibilities to involve a partner are being investigatedMounting on a solar panel frame
Jan BergmanBremen, March 22 24, 2005
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Antennas & BoomsSix 1000 mm extendible EFVS antennasMetal foil antennasLow mass and smooth releaseAntenna element 2.7 gram (Titanium)Release mechanism 20 gramTwo 273 mm deployable rigid LP boomsNew boom design with a bellow hingeLow mass and smooth releaseBoom 0.7 gramRelease mechanism 10 gramJan BergmanBremen, March 22 24, 2005
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ResourcesJan Bergman
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Obstanovka-1 on ISSRFA, joint Polish Swedish experimentObstanvka means Environment in RussianLaunch at the beginning of 2007 with Progres and deployed by ISS crewJan Bergman
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Kompas satellitesKompas-2RFA joint Polish Swedish experiment Disaster warning satelliteLaunch in May June 2005 from Russian nuclear submarineKompas-2N Identical to Compass-2Launch in Sept Dec 2005Precursors to Vulkan fleet of up to 8 satelliteOne satellite per year in next 5 10 yearsMultiple Spacecraft, Multiple Instrument onboard data processingCollaboration with Uppsala DataBase LaboratoryJan BergmanBremen, March 22 24, 2005
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LOISLOIS (LOFAR Outrigger In Scandinavia)Receiver on-line for three years without failureFive receivers now on-line at the test stationJan BergmanBremen, March 22 24, 2005
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Chandrayaan-1Indian mission to the Moon 2008Invited to participate with EFVS but not yet formally selectedCollaboration between Sweden, Poland and IndiaJan BergmanBremen, March 22 24, 2005
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Thank you for listening!Jan BergmanBremen, March 22 24, 2005