Earth, Lunar and Planetary Environments Session D - PowerPoint PPT Presentation

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Earth, Lunar and Planetary Environments Session D

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Title: Earth, Lunar and Planetary Environments Session D


1
Earth, Lunar and Planetary Environments (Session
D)
  • Key questions
  • -What we know
  • -What we dont know (and need to know for VSE)
  • -How do we address the above?
  • For
  • -Earth environment
  • -Lunar Orbit and Surface
  • -Mars Orbit and Surface

2
Earth, Lunar and Planetary Environments-Earth
Environment Issues Outline
WHAT WE KNOW
WHAT WE DONT KNOW (AND NEED TO KNOW)
  • Radiation Belts
  • -LEO and GEO models
  • -Observational archives
  • -COSPAR reference list
  • Plasma Environment
  • -Observational Archives
  • -spacecraft charging models
  • Upper atmosphere, ionos.
  • -var. statistical models
  • -Observational archives
  • Rad Belts, Plasma, Atmos,Ionos
  • -dynamical models (validated)
  • -extremes models and predictive models (incl.
    heavy ions)
  • HOW DO WE ADDRESS THE ABOVE?
  • Data resource mining tools
  • Model-targeted missions (e.g. LWS RBMP, ITMP),
    with continued L1 monitor
  • dynamical/extremes model devel., coupled system
    models devel.

3
Earth, Lunar and Planetary Environments-Lunar
Orbit and Surface Issues Outline
WHAT WE KNOW
WHAT WE DONT KNOW (AND NEED TO KNOW)
  • Mission results from
  • -Explorer 35 and Apollo (data lost? docs only on
    SEP events and event shadows, dosimetry from
    Apollo, mag fields, dust, meteors)
  • -Clementine (SEP events and shadows, dosimetry,
    surface composition-data are limited, access not
    gen. open)
  • -Lunar Prospector (SEP events in ER backgrounds,
    shadowing, mag fields, surface composition,
    neutrons, alphas)
  • -Geotail (SEP events below a few MeV in transits
    of Lunar orbit)
  • -WIND (few flybys- plasmas, mag fields)
  • Models- surface neutrons based on measured
    surface composition
  • How different is lunar space environment from
    interplanetary?
  • Comprehensive lunar surface environment
    measurements and models
  • Details of surface composition
  • Need to revisit lessons learned from
  • Expl. 35, Apollo, Clementine
  • Relevant data sets restoration and mining
  • LRO and dedicated lunar space environment
    orbiter
  • Lunar Lander measurements of radiation, dust,
    micrometeorites, E fields/surfaces charging,
    gases
  • Solar wind/Sheath/Magnetosphere Interaction with
    Moon models
  • Samples for rad history analysis

HOW DO WE ADDRESS THE ABOVE?
4
Session D Meeting Plans
  • Today (Tues) PM session- outline/discussion of
    Mars orbit and surface environment and other
    planets and asteroids environments issues
  • Wed- brief presentations aimed toward the 3 key
    questions from session participants, discussion,
    and draft report/input for steering committee
    any desired combined session splinters
  • Earth Rad belts (Reeves), Earth Upper
    Atmosphere (Lu, Woods), LRO (Spence), surface
    neutrons (Clowdsley), Mars surface rad (Hassler),
    Lunar rad env (Lee), Lunar Electric
    fields/dust/charging (Guild, Delory), SEPs in
    Mars orbit env (Delory, Luhmann), Earth and Mars
    SEP predictions (Turner, Fry)
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