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Atmospheric fluctuations below 0.1 Hz during drift-scan solar diameter 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: [email protected]
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 been performed in order to understand the criticity of the transits method for solar diameter monitoring.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 55: 4th French-Chinese Meeting on Solar Physics - Understanding Solar Activity: Advances and Challenges , 2012 , pp. 381 - 383
Copyright
© EAS, EDP Sciences 2012

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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