WP5 Impact for Space exploration
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Transcript of WP5 Impact for Space exploration
WP5Impact for Space exploration
Progress report for 2nd yearLPI, KUL, SRC PAS, NOVELTIS, ROB
Sergey Kuzin (LPI)
Main goals• Exploring the heliospace with
multiple satellites, a data assimilation-based optimisation approach.
• Perils, threats, operation:• Missions to the Near Earth
Environment• Mission to Mars• Mission to the Moon• Variability of particle environment• Computer simulation of the
interaction of the space environment with spacecrafts
List of DeliverablesTask 5.1 (D 5.1) Exploring the heliospace with multiple satellites, a data assimilation-based optimisation approach. Lead – NOVELTIS, participating KUL. Period 1- 36 m.
Task 5.2. (D 5.2) Mission to Mars: perils and threats. Lead – KULeuven. Period 1-24months.
Task 5.3. (D 5.3) Mission to the Moon: perils and threats. Lead – KULeuven. Delivered in time.
Task 5.4 (D5.4) Computer Simulation of the Moon environment. Lead – KULeuven. Period – 19-36 months.
Task 5.5 (D 5.5) Particle environmental impacts on space-based instruments on LEO high-latitude orbits. Lead – SRC PAS, participants - LPI, ROB and outer partners. Period – 1-30 months.
Task 5.6 (D5.6) Effects of the upper atmosphere of the Earth on solar EUV observations from LEO satellites. Lead – LPI, participants – ROB. Period – 1-30 months
Task 5.7 (D5.7) Computer simulation of the interaction of the space environment with satellites under quiet and active conditions. Lead – KULeuven, Delivered in time
2012 2013 2014 2015
2012 2013 2014 2015
2012 2013 2014 2015
2012 2013 2014 2015
2012 2013 2014 2015
2012 2013 2014 2015
2012 2013 2014 2015
March 2014 in progress planned done
5 November 2003 22:46:39 UTRemaining tasks:
• Final comparison of obtained results with the SPENVIS and GEANT4 predictions.
• Final analysis of database content.
• Release of final database version.
D5.6 Effects of the Earth upper atmosphere on solar EUV observations
•Goal To reach: Study of atmosphere absorption effects in occultation data of the CORONAS/SPIRIT/TESIS and PROBA2/SWAP/LYRA solar experiments, comparison with models, dependence on solar and geomagnetic activity
• Progress So far:• Analysis of occultation data for max, min
and moderate solar activity in 175 and 304A
• Retrieval of the extinction coefficients by the Tikhonov’s generalized discrepancy method
• Comparison of the measured data with the NRLMSISE-00 and DTM 2013 atmosphere models
• The Deliverable report D5.6 is finishing
SPIRIT
SWAP&LYRA
TESIS
Max
Min Moderate
CONCLUSIONS• EUV absorption can be used for validation
of atmospheric models• EUV absorption at different levels of solar
activity much better agrees with the DTM 2013 model (FP7 ATMOP project ) than with the NRLMSISE-00 model
Comparison with atmosphere models
Retrieval of linear extinction coefficient by the Tikhonov’s regularization method
Increase of extinction during geomagnetic storm
NRLMSISE-00
Measurement
NRLMSISE-00Measurement
DTM 2013
Storm Kp=9
Quiet
Status of deliverables and milestones
Deliverable Milestone Collaboration
D5.1 36m - 70% done MS18 18m – done NOVELTIS+KUL
D5.2 24m - ready MS 4 7m –done KUL
D5.3 12m - done MS29 26m – done KUL
D5.4 36m – ready MS26 24m –ready KUL
D5.5 30m – 80% done MS19 18m – done SRC PAS+LPI+ROB
D5.6 30m - 90% done MS 9 12m – done LPI+ROB
D5.7 18m -done MS 3 6m – done KUL
Conclusion
1. Two of 7 deliverables have been done.
2. One deliverable is ready for submission
3. In all tasks progress (both milestones and deliverables) corresponds to the plan
4. In total prepared:
4 publications
6 talks, 4 posters