LEO radiation environment: impacts on PROBA. Erwin De Donder BIRA-IASB Space Weather Section

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1 LEO radiation environment: impacts on PROBA Erwin De Donder BIRA-IASB Space Weather Section Brussels, 2014 March 31 STCE Workshop: PROBA science operations 1

2 Introduction BIRA-IASB Space Weather Section: Host and developer of Space Environment Information System (SPENVIS) since 1996 ( ESA s operational software to simulate the space environment and effects Used for: Mission preparation e.g. PROBA-2, PROBA-V SEE rate and TID calculations (QinetiQ Space nv) Mission analysis e.g. PROBA-2/LYRA auroral perturbations Model comparisons with in-orbit data e.g. PROBA-1/SREM data (ESTEC) Participation in SSA program (SN-I, SSCC, portal, ) Brussels, 2014 March 31 STCE Workshop: PROBA science operations 2

3 Outline I. Space radiation environment at LEO PROBA-1/SREM data PROBA-V/EPT data see talk V. Pierrard et al. II. Space radiation effects at LEO PROBA-2/TDM data PROBA-2/LYRA auroral perturbations Brussels, 2014 March 31 STCE Workshop: PROBA science operations 3

4 I. Space radiation environment at LEO PROBA-1/SREM data (1): introduction Brussels, 2014 March 31 STCE Workshop: PROBA science operations 4

5 I. Space radiation environment at LEO PROBA-1/SREM data (2): SAA, horns, equator, GCR (D. Marinov et al., 2008) Brussels, 2014 March 31 STCE Workshop: PROBA science operations 5

6 Map in invariant coordinates (R,λ) of the radiation-belt omnidirectional integral fluxes for protons > 10 MeV and electrons > 1 MeV, respectively (model: AP8-AE8) horns SAA SPENVIS-4: AP8/AE8 Brussels, 2014 March 31 STCE Workshop: PROBA science operations 6

7 I. Space radiation environment at LEO PROBA-1/SREM data (3): solar proton events Flare No Flare No (D. Marinov et al., 2008) Brussels, 2014 March 31 STCE Workshop: PROBA science operations 7

8 I. Space radiation environment at LEO PROBA-1/SREM data (4): geomagnetic shielding during SPE (coinc. p+) (p+) (p+) (H.D.R. Evans et al., 2008) Brussels, 2014 March 31 STCE Workshop: PROBA science operations 8

9 I. Space radiation environment at LEO PROBA-1/SREM data (5): variation radiation belts outer belt outer belt (e-) (H.D.R. Evans et al., 2008) inner belt fast wind injection (p+) Brussels, 2014 March 31 STCE Workshop: PROBA science operations 9

10 I. Space radiation environment at LEO PROBA-1/SREM data (7): model comparisons (p+) (coinc. p+) (p+) (p+) (H.D.R. Evans et al., 2008) Brussels, 2014 March 31 STCE Workshop: PROBA science operations 10

11 I. Space radiation environment at LEO PROBA-1/SREM data (8): anisotropy (H.D.R. Evans et al., 2008) Brussels, 2014 March 31 STCE Workshop: PROBA science operations 11

12 Summary PROBA-1/SREM data are useful to study radiation environment as function of time and space study directionality of radiation environment at low altitude correlate data with on-board degradations caused by radiation Brussels, 2014 March 31 STCE Workshop: PROBA science operations 12

13 II. Space radiation effects at LEO Introduction (1): overview various effects Brussels, 2014 March 31 STCE Workshop: PROBA science operations 13

14 II. Space radiation effects at LEO Introduction (2): altitude effect SPENVIS-4: SHIELDOSE with AP-8 input. Brussels, 2014 March 31 STCE Workshop: PROBA science operations 14

15 II. Space radiation effects at LEO PROBA-2/TDM data (1): SEL experiment Technology Demonstrator Module study differences between in-flight data and predictions input for improvement modelling, predicting and testing Brussels, 2014 March 31 STCE Workshop: PROBA science operations 15

16 II. Space radiation effects at LEO PROBA-2/TDM data (2): SEU mapping (M. D Alessio, 2013) Brussels, 2014 March 31 STCE Workshop: PROBA science operations 16

17 II. Space radiation effects at LEO PROBA-2/TDM data (3): SEU rates Overall rates are dominated by protons and are within a factor 2 of the inflight rates (M. D Alessio, 2013) Brussels, 2014 March 31 STCE Workshop: PROBA science operations 17

18 II. Space radiation effects at LEO PROBA-2/LYRA data (1): auroral perturbations when cover open in EUV/X-ray channel (Al, Zr) in auroral zones (~ 70 lat) after geomagnetic storm (Kp 4) no correlation with SPE Which mechanism? Which particles? Brussels, 2014 March 31 STCE Workshop: PROBA science operations 18

19 II. Space radiation effects at LEO PROBA-2/LYRA data (2): localisation Perturbations trajectories 2011/05/1,2,29 Perturbations Centers in North pole 2011/05/01 J-P Iraguha (ULB student) Brussels, 2014 March 31 STCE Workshop: PROBA science operations 19

20 II. Space radiation effects at LEO PROBA-2/LYRA data (3): an approach Reconstructing particle environment (i.e. flux) by using e.g. MetOpA data ~ km, LTAN = 21h30) finding similar (B,L) pairs for a = K p Propagation of flux through detector using GEANT4 software (available in SPENVIS) Comparing detector response with observations Brussels, 2014 March 31 STCE Workshop: PROBA science operations 20

21 Space radiation effects at LEO PROBA-2/LYRA data (4) METOP-A trajectories Perturbations trajectories PROBA-2 trajectories J-P Iraguha (ULB student) Brussels, 2014 March 31 STCE Workshop: PROBA science operations 21

22 General conclusion PROBA provides data on the radiation environment (fluxes, directionality, species, ) DIRECTLY through radiation measurements INDIRECTLY through radiation effect measurements that allows us to improve environment models and eventually create new models Brussels, 2014 March 31 STCE Workshop: PROBA science operations 22

23 Thank you for your attention. Brussels, 2014 March 31 STCE Workshop: PROBA science operations 23

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