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All-sky camera of the ALFA project: common points and interests with the Wide Field Astronomical Observations E. Séran & M. Godefroy CETP, St-Maur. June 14, 2006 Paris. h, km. e. 300. ionosphere. 630nm (O). V. F. 200. 558nm (O). δn. 428nm (N 2 + ). E. 100. B.
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All-sky camera of the ALFA project: common points and interests with the Wide Field Astronomical Observations E. Séran & M. Godefroy CETP, St-Maur June 14, 2006 Paris
h, km e 300 ionosphere 630nm (O) V F 200 558nm (O) δn 428nm (N2+) E 100 B 1 10 electron E, keV Project ALFA (Auroral Light Fine Analysis) λ/2 844.6 (O) fpe hν λ λ/2 = 1-3 m SD • SCIENTIFIC OBJECTIVES • Study of the energy and material exchange inside the transpolar arcs • - Fine analysis of the light emissions in the ionosphere (altitude ~150-300 km) • Interaction of the energetic electrons with the ionosphere • Formation of the density irregularities in the regions of the precipitating electrons • Plasma motion associated with the field-aligned currents SD
Project ALFA (Auroral Light Fine Analysis) INSTRUMENTAL OBJECIVES “All-sky“ “High resolution” “All-sky“ Angular resolution : - 90° < φ < 90° Horizontal resolution : ~ 200 m Horizontal covering : ~ 3000 km Filters: large frequency band R-G-B “High Resolution” Angular resolution :- 9° < φ < 9° Horizontal resolution :~ 40 m Horizontal covering : ~ 50 km Filters: narrow band of ~ 2 nm à 200 km
All-sky S2 PRO Δt=6sec 1600 ISO W • Observations • - Emissions • - structure, dynamics, intensity • relative intensity in the RGB ranges • Absorption through the atmosphere (using stars) • Comets trails, moon, human activity etc. 500 350 800 km N 50 km E B G R hν 104 103 102 101 2-3 keV N2 427.8 R/(erg cm-2 s-1) O 844.6 427.8557.7 630777.4 844.6 nm N2+O (1S)O(1D) O/ O2 O/ O2 O 630 0. 1 1 10 E, keV
Common points with astronomical observations in Dôme C • Observations • survey of the ionospheric emissions • survey of the atmospheric absorption • Data transfer (rate: <400 Mb/day for all experiments) • - ALFA’s ”quick-look”+ few images (Mb/day ?) • ALFA’s whole data base (~Gb/day !) • Technical points related to the extreme conditions • choice of materials (domes, insulations) • protection against the ice • access during the winter • - stuff training • etc.
Proposal of installation in the SuperDarn shelter (1300m from the base) • Advantages • - Common scientific purposes • Minimum human light • Inconveniences • No access during the winter season (over 750 m)
Electrical concept • Tension : 12V • - Power : 220 V / 1500 W Specific requirements • Dôme heating • Distance Camera - PC: 5 m • Mounting on the roof • Easy access from outside/inside
St-Maur, 2006 Dôme C, 2008 Kiruna, 2005
Proposal: Electric field and ice particles measurements in the boundary layer in Dôme C • Measured parameters • Vertical electric field • (influence on the transport of charged ice particles?) • - Electric conductivity • Flow of charged ice particles and charge distribution eE mg Q+ φ Q+ Q - ~ e-σt/ε0 u ~ 1/|ut| σ ~ 0.5 10-13 Mo m-1 φ ~ Q/C t=0 t u ~ 3 m s-1 t (growth) ~ 10 ms
power Proposal: Electric field and ice particles measurements in the boundary layer in Dôme C Electrodes + electronics: Weight : ~ 500g Sizes: ~ 15x3cm electrodes ~ 0.7m each boom ~ 2.2L electronic box Power : ~ 0.2W + heating (TBD) ~30m TM/TC