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STAFF-SC / FGM Comparison. Cross_Calibration Workshop ESTEC, Noordwijk, 2-3 february 2006. P. Robert, CETP. A. Reminder on old comparisons (IC, London, February 2001). B. New comparisons. I. Spectrograms comparison. II. Average spectra comparison. III. Wave Forms comparison.
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STAFF-SC / FGM Comparison Cross_Calibration Workshop ESTEC, Noordwijk, 2-3 february 2006 P. Robert, CETP A. Reminder on old comparisons (IC, London, February 2001) B. New comparisons I. Spectrograms comparison II. Average spectra comparison III. Wave Forms comparison IV. Noise Level Conclusions
A. Old comparisons (IC, London, February 2001) A.1 Spectrogram Original FGM High res. Files provided by M. Dunlop Already STFF-FGM difference on perp. DC field P. Robert, Croos Cal WS, 2006-02-02, ESTEC
A. Old comparisons (IC, London, February 2001) A.2 Average Spectra Original FGM High res. Files provided by M. Dunlop Rather good agreement Between STFF-FGM Sensitivity differs beyond 1 Hz P. Robert, Croos Cal WS, 2006-02-02, ESTEC
B. New comparisons(February 2006) All following result has done with FGM high res. Data Provided by FGM Dapclus software, using cal tables downloaded from I.C. P. Robert, Croos Cal WS, 2006-02-02, ESTEC
P. Robert, Croos Cal WS, 2006-02-02, ESTEC I. Spectrograms comparison I.1 Bx,By,Bz SC1 Rest of spin effect, OK OK
Position in space 18:00 24:00 21:00 22:00 Tetrahedron size about 1200 km P. Robert, Croos Cal WS, 2006-02-02, ESTEC
P. Robert, Croos Cal WS, 2006-02-02, ESTEC I.2 Bz ALL S/C OK Pb !
I.3 Bperp ALL S/C 1) STAFF < FGM, FGM 2) STAFF Pb on S/C # 1 Sometimes up to 20% When strong DC field STAFF P. Robert, Croos Cal WS, 2006-02-02, ESTEC
I.3 Bperp SC1 and SC2 1) STAFF < FGM, Diff=1 nT or 16% on SC1, Diff=0.5 nT or 8% on SC2 FGM 2) STAFF Pb on S/C # 1 Sometimes up to 20% When strong DC field STAFF P. Robert, Croos Cal WS, 2006-02-02, ESTEC
P. Robert, Croos Cal WS, 2006-02-02, ESTEC Fs Fs II. Average spectra comparison II.1 Bx,By,Bz SC1 Fs STAFF FGM STAFF < FGM Sensitivity loss Sensitivity loss
II.2 Bz SC1 II.2 Bz SC2 Fs Fs Fs Some differences, as Bperp: Staff < FGM, Best fit with SC2 FGM STAFF Parasite spikes P. Robert, Croos Cal WS, 2006-02-02, ESTEC
P. Robert, Croos Cal WS, 2006-02-02, ESTEC Fs Fs II.3 Bz All S/C Parasite spikes different between STAFF and FGM Parasite spikes different on each SC Fs
III. Wave Forms comparison III.1 Filtered Bx,By,Bz, Bperp SC1 STAFF bug, offset NE 0 STAFF/FGM : difference about 0.5 nT P. Robert, Croos Cal WS, 2006-02-02, ESTEC
III.2 ZOOM on Filtered Bx,By,Bz, SC1 Looks the same, but STAFF < FGM About 20% at 2 Hz P. Robert, Croos Cal WS, 2006-02-02, ESTEC
III.3 ZOOM on Filtered Bx,By,Bz, SC2 Best fit: About 5 % But not everywhere P. Robert, Croos Cal WS, 2006-02-02, ESTEC
Fs Fs IV. Background noise Level IV.1 Bx,By,Bz SC1 Starting Time 09:02:00.029 Starting Time 09:02:00.486 Fs No reliable measurement P. Robert, Croos Cal WS, 2006-02-02, ESTEC
Fs IV. Background noise Level Fs IV.2 Bz SC1 No hurried conclusion ! Must be re-computed For other events P. Robert, Croos Cal WS, 2006-02-02, ESTEC
(from B. Grison) FGM - STAFF-SC P. Robert, Croos Cal WS, 2006-02-02, ESTEC
PRELIMINARY CONCLUSION - This work has be done too quickly: We have to take care with too fast conclusions - Two basic problems has been identified: a) Why perp DC. Field estimated from STAFF SC1 is less that SC2,3,4 ? b) Why perp DC field estimated from STAFF is less than FGM measurement ? . True for perp. DC field, . But also true on the entire spectra, . And also true on the filtered waveforms We have to look on the 4 transfer functions, and carrefully study the onboard calibration - A large amount of work remain to be done: a) Study other cases, in other regions of space in other epochs With or without strong DC field b) See if preliminary conclusions remains the same ; see also HBR mode c) Introduce the new despin utility software, and restart all… P. Robert, Croos Cal WS, 2006-02-02, ESTEC
STAFF SC - SA (B. Grison)
FGM - STAFF - EFW (B. Grison)