1. THEMIS time opportunities
Arturo López Ariste

3. THEMIS at short 90 cm Ø Ritchey-Chrétien telescope f/17 at F1 focus
Polarimetric analysis at F1 (no instrumental polarization at 2-3×10-5 level)
3 post-focal instruments:
MTR: Multiline spectropolarimetry. High-res double spectrograph allowing up to 10 (6) spectral domains observed simultaneously from 4000 – Å
MSDP: Spectro-imager.
IPM: Tunable imaging filter (UBF + etalon). High-spectral resolution (90 mÅ)

4. 4 cameras

6. Prominences I Q U V
He D3 Hα
Ca II

7. #4 #3 #1 #2 #5

8. #4 #3 #1 #2 #5

13. A. Sainz Dalda

14. A. Sainz Dalda

15. A. Sainz Dalda

16. 200-250 days allocated per year
Two different TACs:
Main TAC (80% of total time)
Spanish TAC (20%)

17. 200-250 days allocated per year
Two different TACs:
Main TAC (80% of total time)
5% International access
76% French time
19% Italian time
Spanish TAC (20%)

18. 200-250 days allocated per year
Two different TACs:
Main TAC (80% of total time)
5% International access
76% French time
19% Italian time
Spanish TAC (20%)
1.3 pressure factor

19. Easier ways to have access?
Include a Co-I from one of the participating countries
Find appropriate data in BASS2000 after a 1-year exclusive period.

20. Coordinated Campaigns
About one a year in the last few years:
2004/2005: JOP 175 (5 ground telescopes, 2 space instruments)
2006: VTT-Themis coordinated campaign

21. Coordinated Campaigns
About one a year in the last few years:
2004, 2005: JOP 175 (5 ground telescopes, 2 space instruments)
2006: VTT-Themis coordinated campaign

23. F1

24. F2