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Atmospheric fluctuations below 0.1 Hz during drift-scan solardiameter measurements

Published online by Cambridge University Press:  27 June 2012

M. Faurobert ,
C. Fang ,
T. Corbard ,
C. Sigismondi ,
A. Raponi ,
G. De Rosi ,
M. Bianda ,
R. Ramelli ,
M. Caccia  and
M. Maspero
...Show all authors
C. Sigismondi
Affiliation:
Sapienza University of Rome and ICRA, Italy; University of Nice-Sophia Antipolis, France; IRSOL and GPA-Observatorio Nacional Rio de Janeiro, Brazil. e-mail: sigismondi@icra.it
A. Raponi
Affiliation:
Sapienza University of Rome, Italy
G. De Rosi
Affiliation:
Sapienza University of Rome, Italy
M. Bianda
Affiliation:
IRSOL, Locarno, Switzerland
R. Ramelli
Affiliation:
IRSOL, Locarno, Switzerland
M. Caccia
Affiliation:
Como University, Italy
M. Maspero
Affiliation:
Como University, Italy
L. Negrini
Affiliation:
Como University, Italy
X. Wang
Affiliation:
Huairou Solar Observing Station, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China
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Abstract

Measurements of the power spectrum of the seeing in the range 0.001–1 Hz have beenperformed in order to understand the criticity of the transits method for solar diametermonitoring.

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References

Cuevas, S., Qualgliata, N., Sigismondi, C., et al., 2011, in 22nd General Congress of the International Commission for Optics, ed. R. Rodriguez-Vera & R. Diaz-Uribe (Puebla, Mexico), Abstract No. 2285348
Gething, P.J.D., 1955, Mon. Notes Roy. Astron. Soc., 115, 558 CrossRef
Sigismondi, C., 2010, in IAGA-II Proc., ed. L. Damé & A. Hady (Cairo University Press), 207
Wittmann, A.D., & Bianda, M., 2000, ESA SP, 463, 113