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 [email protected] post-éclipse meeting, IAP 30.9.2010 ICRA and solar physics www.icra.it/solar 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) Classification of Solar diameter measurements 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 Baily’s beads – problem: scintillation, signal to noise, filter, FSR Last solar cycle XXIII: SOHO data (June 2010) Calibrating eclipses for studying secular variations Eclipse Problem 1: scintillation Problem 2: Flash Spectrum Region Flash Spectrum (1905) Problem 3: lunar profile Watts (1962) σ>0.2” random Kaguya (2009) σ<<0.01” sampling each 0.5”-5” Sampling 1-10 km Real lunar limb vs Watts profile (Kilcic, Sigismondi, Rozelot & Guhl, So. Phys. 2009) Locarno Solar Obsevratory IRSOL Istituto Ricerche Solari di Locarno 10 km 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 LIMB DARKENING FUNCTION WITH BAILY’S BEADS ANALYSIS Andrea Raponi and C. Sigismondi Sapienza University of Rome Total Solar Irradiance changed in the past, so also the diameter? Hendrick Avercamp (1585-1643), Amsterdam Eclipses Beads of 15/01/2010 by R. Nugent with Kaguya profile; software Occult Solar Limb and LDF seeing and inflection point Baily’s bead light curve depends on scintillation Valley’s profile + real LDF LDF and Flash Spectrum Region? computing LDF from light curve and Kaguya lunar profile LDF from 2 different beads x:units of 6 mas Synthetic LDF from Poissonian noise 2.50 2.00 CONTEGGI / PIXEL 1.50 1.00 0.50 0.00 0 -0.50 0.1 0.2 0.3 0.4 0.5 0.6 0.7 SECONDI D'ARCO DAL SOLE STANDARD 0.8 0.9 1 Notes: quartz oscillators physics Thewlis Enc. Dictionary of Physics, Pergamon Press 1962 Quartz, the preparation and use of, oscillators Annular Eclipse of 22/9/2006 2 watches: SONY e CASIO in French Guyana the temperature was > 8 °C than in Rome Roman tradition in solar diameter ….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…