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USING THE SCINTILLATION OF EXTENDED OBJECTS TO PROBE LOWER ATMOSPHERIC TURBULENCE Concept & First Results Published in: Experimental Astronomy 12, 1, 2001 Jacques M. Beckers US National Solar Observatory “SHADOW BANDS” DURING SOLAR ECLIPSE Images taken by Franz Kerschbaum (Vienna) during 2006 eclipse ~ 60 cm ¾ CLOSE TO “TOTALITY” AT A TOTAL ECLIPSE OF THE SUN RAPIDLY VARYING, LOW CONTRAST LIGHT PATTERNS ARE SEEN ON THE GROUND OR BUILDINGS.THESE ARE REFERRED TO AS “SHADOW BANDS”. IT IS THE SAME AS SOLAR SCINTILLATION. ¾ SHADOW BAND PATTERN IS ELONGATED IN THE DIRECTION OF THE CRESCENT ¾ CONTRAST APPEARS TO VARY FROM ECLIPSE TO ECLIPSE AND PROBABLY WITH LOCATION ¾ IT IS CLEARLY A PHENOMENON ASSOCIATED WITH ATMOSPHERIC TURBULENCE ¾ ED SEYKORA DETERMINED IN 1993 THAT PHENOMENON IS ALSO PRESENT OUTSIDE SOLAR ECLIPSE BUT WITH MUCH LOWER CONTRAST ( ≤ 0.1 % RMS) ¾ HE ALSO FOUND AT SAC PEAK A STRONG CORRELATION BETWEEN CONTRAST AND SEEING CORRELATION OF SOLAR SCINTILLATION & SOLAR LIMB MOTION Seykora CORRELATION OF SOLAR SCINTILLATION & GRANULATION CONTRAST Rimmele NOTE: AT SAC PEAK SEEING IS DOMINATED BY BOUNDARY LAYER TURBULENCE ATMOSPHERIC OPTICS (using Roddier, Progress in Optics XIX, 283, 1981) Notations: σI2 = (ΔIRMS/I)2 = Scintillation Index r0 = Fried Parameter at 500 nm ζ = Zenith Distance Cn2(h) = Refractive Index Structure Constant σI2 (for Stars) = 19.2*λ-7/6*cos-11/6ζ*,h+5/6*Cn2(h)dh LOOKING AT THE SUN ONE RECEIVES A CONE OF LIGHT ~ 0.01 RADIAN IN WIDTH Ö ONE AVERAGES THE ATMOSPHERIC EFFECTS OVER AN AREA WHICH INCREASES WITH INCREASING DISTANCE Ö HIGHER LAYERS CONTRIBUTE LESS TO SCINTILLATION INDEX σI2 (for Sun) = 0.955x106*cos-2/3ζ*,h-1/3*Cn2(h)dh (independent of λ!) ALSO: r0-5/3 = 0.060*λ2*cosζ*,Cn2(h)dh (:) FWHMseeing5/3 ⇒ σI(Sun)2/FWHM5/3 = const.* ,h-1/3*Cn2(h)dh/ ,Cn2(h)dh THIS RATIO IS DOMINATED BY BOUNDARY LAYER OPTICAL TURBULENCE. WHEN IT DOMINATES (as it does in daytime) THIS RATIO DOES NOT VARY MUCH WITH TIME AND LOCATION Ö EXPLAINS SEYKORA RELATION EARLY “ADVANCED TECHNOLOGY SOLAR TELESCOPE” SITE SURVEY Used Single Scintillometers Pointed at Meridional Transit of Sun Sites Tested: Big Bear Lake,CA Lake Heron,NM La Palma/ORM Mauna Loa,HI Sac Peak,NM “lakeshine” SHABAR = SHAdow BAnd Ranger NON-REDUNDANT SOLAR SCINTILLOMETER ARRAY Correlation of ► SHABAR pairs SHABAR Pair Light Path DIMM Yunnan’s Fuxian Hu Seeing Monitor Correlation Coefficient vs Separation 16 cm 2 cm 20 cm 6 cm 4 cm SHABAR 100 cm 200 cm S-DIMM PANEL SHABAR PANELS CCD IMAGE OF SLITS ACROSS SOLAR LIMB INTERPRETATION OF THE ATST SHABAR DATA DEVELOPED BY P. HICKSON, F. HILL, M. COLLADAS & H. SOCAS-NAVARRO USE: H. Socas-Navarro, J. Beckers, et al. PASP 117, 1296, 2005 CVobs(d) “missing scintillation” (due to L0 & time filtering) constant*CVtheory(h,d) d=0 mm h-1/3 curve d=12mm d=12mm ¾ Inversion of Equation ⇒ Cn2(h) ¾ Inclusion of DIMM Results (r0) ⇒ ∆s d=468mm 16 curves corresponding to 16 spacings ¾ Since 10 mm < d < 500 mm Height Range is Limited to ~ 0.2m< h < 500m TEST OF SHABAR Cn2(h) DETERMINATIONS USING 100+ METER DASH TOWER IN ERIE, COLORADO NEXT TO AN ATST SEEING MONITOR FINAL ATST SITE SURVEY INCLUDED 6 SITES IN USA, MEXICO AND EUROPE Big Bear, CA Haleakala, HI La Palma, Spain Panguitch Lake (UT) Sacramento Peak, NM San Pedro Martir, MX LAKE SITES LAND SITES HEIGHT VARIATION OF Cn2 AND SEEING (r0) Collados Socas-Navarro STATISTICAL RESULTS OF TWO INVERSION PROGRAMS (full: Collados analysis; dashed: Socas-Navarro analysis) CONCLUSIONS: • Place Telescope at h > 25m • Haleakala is best site • Conclusion based also on number of periods with continuous very good seeing THE SCINTILLATION OF MOON AND PLANETS FULL MOON ONLY (= like Sun) PLANETS AT OPPOSITION ONLY DO NOT INCLUDE SATURN BECAUSE OF ITS RINGS PLANETS: URANUS (dia 3.60 arcsec,; mV = 5.5) MARS (dia 17.9 arcsec.; mV = -2.0) JUPITER (dia 46.9 arcsec.: mV = -2.6) 0 arcsec. 3.6 arcsec. h+5/6 17.9 arcsec. 46.9 arcsec. h-1/3 1920 arcsec. • SCINTILLATION OF MARS IS ALMOST PROPORTIONAL TO THE SEEING • L0 (Ö “missing scintlillation ∆s”) IS OF NO CONCERN FOR STARS & PLANETS SUN/ MOON 100 m 1000 m m 0000 h =1 h= h= 0m h=1 STARS JUPITER MARS URANUS THANK YOU