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The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and IRSOL Istituto Ricerche Solari di Locarno sigismondi@icra.it post-éclipse meeting, IAP 30.9.2010
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ICRA and solar physics www.icra.it/solar
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Participating institutions ICRA, International Center for Relativistic Astrophysics Sapienza University of Rome # IOTA ES and US * # Osservatorio Astronomico di Roma # Basilica di Santa Maria degli Angeli, Roma * Yale Astronomy Department # Université de Nice-Fizeau Dept. # Observatoire de la Cote d'Azur (Calern site PICARD Sol) * Institute d'Astrophysique de Paris * # IRSOL * # # data and analysis * observations (CLAVIUS)
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Classification of Solar diameter measurements
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Measuring radius from Earth Drift-scan: solar angular speed * transit time = diameter problem: seeing Angular direct measurements – problem: seeing, optical aberration Mercury and Venus transits: planetary speed * transit time = diameter - problem: scintillation, black drop Eclipses with Bailys beads – problem: scintillation, signal to noise, filter, FSR
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Last solar cycle XXIII: SOHO data (June 2010)
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Calibrating eclipses for studying secular variations
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Eclipse Problem 1: scintillation
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Problem 2: Flash Spectrum Region
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Flash Spectrum (1905)
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Problem 3: lunar profile Watts (1962) σ>0.2 random Kaguya (2009) σ<<0.01 sampling each 0.5-5 Sampling 1-10 km
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Real lunar limb vs Watts profile (Kilcic, Sigismondi, Rozelot & Guhl, So. Phys. 2009)
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10 km Locarno Solar Obsevratory IRSOL Istituto Ricerche Solari di Locarno
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δR =-0.41±0.05 (Kilcic et al. 2009) on 29 march 2006, in agreement with SOHO 2003 data preliminary:δR =-0.36±0.15 on 15 Jan 2010, based on 6 beads from R.Nugent
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LIMB DARKENING FUNCTION WITH BAILYS BEADS ANALYSIS Andrea Raponi and C. Sigismondi Sapienza University of Rome
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Total Solar Irradiance changed in the past, so also the diameter ? Hendrick Avercamp (1585-1643), Amsterdam
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Eclipses Beads of 15/01/2010 by R. Nugent with Kaguya profile; software Occult
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Solar Limb and LDF seeing and inflection point
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Bailys bead light curve depends on Valleys profile + real LDF scintillation
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LDF and Flash Spectrum Region?
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computing LDF from light curve and Kaguya lunar profile
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LDF from 2 different beads x:units of 6 mas
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Synthetic LDF from Poissonian noise
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Notes: quartz oscillators physics Thewlis Enc. Dictionary of Physics, Pergamon Press 1962 Quartz, the preparation and use of, oscillators
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Annular Eclipse of 22/9/2006 2 watches: SONY e CASIO
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in French Guyana the temperature was > 8 °C than in Rome
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Roman tradition in solar diameter
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….and in eclipses: In 1581 edition Clavius wrote: relinquebatur in Sole circulus quidam exilis undique totam lunam ambiens. He actually saw an annular eclipse. The Sun in 1567 was >2.5 arcsec larger than now ? Not possible for physical reasons…
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