Strategy for Space Physics in Uppsala: Swedish Institute of Space Physics (IRF) [Department of Astronomy - PowerPoint PPT Presentation

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Strategy for Space Physics in Uppsala: Swedish Institute of Space Physics (IRF) [Department of Astronomy

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Rosetta (aie) Magnum/Solaris? /Exo-Mars? (jwe) JME? (jwe,aie) VEP? ... Cometary environment (Rosetta) Jupiter dust rings (JME?) Modelling: Currently lacking! ... – PowerPoint PPT presentation

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Title: Strategy for Space Physics in Uppsala: Swedish Institute of Space Physics (IRF) [Department of Astronomy


1
Strategy forSpace Physics in UppsalaSwedish
Institute of Space Physics (IRF)Department of
Astronomy Space Physics (UU)Jan-Erik
Wahlundwww.irfu.se
To boldly go, to seek out new worlds....
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IRF-U Activities (not only Analysis/Publications)
  • We are humans with special knowledge resources
  • Experienced Team Needed for Experimental
    Activities!
  • Scientists
  • (development initiatives, contacts, analysis,
    databases, operations, methodology, education,
    PR, political support for science education)
  • Administrators
  • (management, economy)
  • Engineers
  • (development, electronics, mechanics, tests,
    contacts, methodology, industrial support for
    space engineering)
  • Computer specialists
  • (instrument S/W, DBH)
  • Strategy remark
  • All aspects of an experimental science group need
    be provided in a long term planning
  • Ex Lennart soon near pension
  • Modellers, theorists only if resources allow it

5
Planetary Space Physics
  • Dust-plasma physics
  • Observations
  • Saturn E-ring (Cassini discovery with IRF-U
    instrument!)
  • Cometary environment (Rosetta)
  • Jupiter dust rings (JME?)
  • Modelling Currently lacking!
  • How do T-Tauri accretion discs evolve?
  • origin of planetary system
  • Atmospheric/Ionospheric escape processes
  • Observations
  • Saturn Magn. - Titan ionosphere interactions
    (Cassini)
  • SW - Mars ionosphere interactions
    (Solaris?/Exo-Mars?/MEMO?)
  • SW - Venus ionosphere interactions (VEP?)
  • Modelling Hybrid-code
  • How do flowing plasma erode planetary
    atmospheres?
  • Atmospheric evolution

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Planetary Space Physics (cont)
  • Ionospheric organic chemistry
  • Observations
  • Titan ionosphere (Cassini)
  • Modelling
  • Earths early ionosphere
  • Chirality production in ionosphere?
  • Did ionospheric organic molecule production lead
    to pre-biotic chemistry?
  • Origin of life (Astrobiology)

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Development of Methods Instruments(1)
  • Restrictions
  • Instrument Heritage (our history matters!)
  • Instruments should have flown (tested) before in
    some sense
  • Instrument development occurs in small steps
    (like science), usually based on earlier
    designs/methods (know how)
  • Ex Analysis of current data operations often
    leads to insights on new methodology
  • International Contacts must be in place
  • Diplomacy, Administration, Presentations
    Travels
  • Good Science Arguments/Objectives must exist (of
    course)
  • The proposed instrument must be shown to meet the
    objectives/goals
  • Instrument simulations/demonstrators
  • examples next page ?

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Diplomacy Administration!
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Development of Methods Instruments(2)
  • Science goals determine which parameters we need
    measure
  • Fast Te-tracking with LP (up to 16 Hz)
  • Swarm testing
  • LP active chirp-technique at ion frequencies (Ti,
    ion composition)
  • Perhaps Swarm testing
  • New Ti-Al-N probe surfaces that stand high
    temperatures good performance
  • MexRus testing, BepiColombo to Mercury
  • Topside Sounder Ground Penetrating Radar
    (GPR)
  • Ionospheric profiles
  • Broaden to planetary sciences?
  • Complement with planetary radar (EISCAT)
  • Plasma Radio Tomography
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