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JOSEPH AJELLO JPL MICHAEL STEVENS NRL ROBERT WEST JACQUES GUSTIN LPAP

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Presentation on theme: "JOSEPH AJELLO JPL MICHAEL STEVENS NRL ROBERT WEST JACQUES GUSTIN LPAP"— Presentation transcript:

1 Titan Airglow: FUV & EUV 2009 UVIS Spectra of Airglow During Day, Night & Eclipse :
JOSEPH AJELLO JPL MICHAEL STEVENS NRL ROBERT WEST JACQUES GUSTIN LPAP GREG HOLSCLAW CU TODD BRADLEY UCF agu: dEC 2011

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3 TITAN PROTON PLASMA (0.1 keV-4 MeV) & SOLAR XUV GENERATES 2-level IONOSPHERE (300-1500 KM)
Solar XUV Excitation –Strong Top Ionosphere -Magnetospheric: p and O+ Plasma (Cravens et al., 2008).

4 N2 Cross section Analysis for Dayglow VI (2)→UVIS (16)→Lab(e +N2 300 features)
V(z)=g(z) x w gj (z) = F (e) x n(z) x s(e) Dl=0.2Å Dl=30Å Dl=5Å DD

5 ISS & UVIS OBSERVATION OF TITAN SOLAR ECLIPSE @ 600K km
plasma + N2

6 FUV DARK SIDE LIMB & DISK SPECTRA DOY110-2009 @15K km

7 Laboratory Result: p + N2

8 ELECTRON CROSS SECTIONS FOR TITAN DAYGLOW UV EMISSION MODEL
Stevens et al., 2011 “Production of Titan’s Far ions Ultraviolet Nitrogen Airglow” AURIC Code Emission Cross Sections: N2 Carroll-Yoshino c4′—X system,b‘-X, b-X systems N I and N II multiplets the N2 Lyman-Birge-Hopfield a—X system (Young et al., 2010) the N2 Vegard-Kaplan A—X bands sLBHPK= 0.6 A&S (1985) sLBH=0.7 A&S (1985)

9 Pixel Center Ray Height (km)
Best (S/N) Titan Dayglow UVIS Limb Spectrum; 22June 2009: ‘800 km STARE’ –40 One hour EUV and FUV image of 15 – 4 minute records . –42 EUV –44 DEC (deg) –46 –48 4 2 –2 –4 RA (deg) 1500 1000 FUV Pixel Center Ray Height (km) 500 10 20 30 40 50 60 Pixel Number

10 AURIC MODEL FIT TO UVIS EUV SPECTRUM AT 1000 KM

11 AURIC MODEL FIT TO UVIS FUV SPECTRUM AT 1000 KM

12 AURIC MODEL OF FUV VERs AND COLUMN EMISSION RATES

13 The FUV Dayglow Limb Spectra of Titan
Surface to Exosphere: 13Dec04.

14 DARK SIDE OBSERVATION OF TITAN ON 25MARCH2008

15 FUV LIMB PROFILE INTENSITIES OF 25 MARCH2009

16 Model fit to UVIS Dark Limb (Twilight) EUV Spectrum from 25Mar08 with a Regression Model - 7-Vectors)

17 How to get a BRIGHT UV Airglow in 2009
BRIGHTEST LIMB AIRGLOW 22JUNE obs[14] SZA=53DEG, MRH =1000 km S/C ~60k KM BRIGHTEST DISK & 2ND LIMB 12OCT OBS[45-51] LIMB~ 1000KM SZA~95, S/C ~175k KM

18 SUMMARY OF 2009 ECLIPSE, LIMB, BRIGHT DISK AND DARK DISK UVIS OBSERVATIONS OF TITAN
Solar Driven processes on Dayside and Twilight Observed EUV and FUV Emissions during 1 of 3 Eclipses. Probably Plasma impact. Tentative Sporadic FUV Nightglow Spectra at 0.1 Intensity level of dayglow. Probably Plasma Impact (protons, O+, electrons). Twilight (Terminator) Glow-Solar XUV at deg Limb SZA ~ Dayside Intensity. N2 EUV (12R) /FUV (200R) dayglow structure similar to Earth

19 Elvis Lives (Titan Organic Chemistry-Biomarker
Elvis Lives (Titan Organic Chemistry-Biomarker! ) 45 years with my Honey


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