The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi...

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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 [email protected] post-éclipse meeting, IAP 30.9.2010

Transcript of The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi...

Page 1: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

The solar limb during eclipses: Flash Spectrum Region and Baily beads

Costantino SigismondiICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis

and IRSOL Istituto Ricerche Solari di Locarno

[email protected]

post-éclipse meeting, IAP 30.9.2010

Page 2: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

ICRA and solar physicswww.icra.it/solar

Page 3: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

Participating institutions

ICRA, International Center for Relativistic AstrophysicsSapienza 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)

Page 4: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

Classification of Solar diameter measurements

Page 5: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

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

Page 6: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

Last solar cycle XXIII: SOHO data (June 2010)

Page 7: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

Calibrating eclipses for studying secular variations

Page 8: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.
Page 9: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

Eclipse Problem 1: scintillation

Page 10: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.
Page 11: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

Problem 2: Flash Spectrum Region

Page 12: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

Flash Spectrum (1905)

Page 13: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

Problem 3: lunar profile

Watts (1962) σ>0.2” randomKaguya (2009) σ<<0.01” sampling each 0.5”-5”

Sampling 1-10 km

Page 14: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

Real lunar limb vs Watts profile (Kilcic, Sigismondi, Rozelot &

Guhl, So. Phys. 2009)

Page 15: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

10 km

Locarno Solar Obsevratory IRSOL Istituto Ricerche Solari di Locarno

Page 16: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.
Page 17: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

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

Page 18: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

LIMB DARKENING FUNCTION WITH BAILY’S BEADS ANALYSIS

Andrea Raponi and C. SigismondiSapienza University of Rome

Page 19: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

Total Solar Irradiance changed in the past, so also the diameter?

Hendrick Avercamp (1585-1643), Amsterdam

Page 20: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

Eclipses

Beads of 15/01/2010 by R. Nugent with Kaguya profile; software Occult

Page 21: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

Solar Limb and LDF

seeing and inflection point

Page 22: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

Baily’s bead light curve

depends on

Valley’s profile

+ real LDF

scintillation

Page 23: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

LDF and Flash Spectrum Region?

Page 24: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

computing LDF from light curve and Kaguya lunar profile

Page 25: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

LDF from 2 different beads x:units of 6 mas

Page 26: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

Synthetic LDF from Poissonian noise

Page 27: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

Notes: quartz oscillators physicsThewlis Enc. Dictionary of Physics, Pergamon Press 1962 Quartz, the

preparation and use of, oscillators

Page 28: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

Annular Eclipse of 22/9/2006 2 watches: SONY e CASIO

Page 29: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

in French Guyana the temperature was > 8 °C than in Rome

Page 30: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

Roman tradition in solar diameter

Page 31: The solar limb during eclipses: Flash Spectrum Region and Baily beads Costantino Sigismondi ICRA-Sapienza, Roma; Université de Nice-Sophia Antipolis and.

….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…