1 / 4

Earth, Lunar and Planetary Environments (Session D)

Earth, Lunar and Planetary Environments (Session D). Key questions: -What we know -What we don’t know (and need to know for VSE) -How do we address the above? For: -Earth environment -Lunar Orbit and Surface -Mars Orbit and Surface. *Radiation Belts -LEO and GEO models

leone
Download Presentation

Earth, Lunar and Planetary Environments (Session D)

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Earth, Lunar and Planetary Environments (Session D) Key questions: -What we know -What we don’t 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. *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. Earth, Lunar and Planetary Environments-Earth Environment Issues Outline WHAT WE KNOW WHAT WE DON’T KNOW (AND NEED TO KNOW)

  3. *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 Earth, Lunar and Planetary Environments-Lunar Orbit and Surface Issues Outline WHAT WE KNOW WHAT WE DON’T KNOW (AND NEED TO KNOW) 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 * EarthRad 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)

More Related