Atmospheric fluctuations below 0.1 Hz during drift-scan solar diameter measurements

C sigismondi; A Raponi; G De Rosi; M Bianda; R Ramelli; M Caccia; Matteo Maspero; L Negrini; X Wang

doi:10.1051/eas/1255054

Atmospheric fluctuations below 0.1 Hz during drift-scan solar diameter measurements

C sigismondi, A Raponi, G De Rosi, M Bianda, R Ramelli, M Caccia, Matteo Maspero, L Negrini, X Wang

Research output: Contribution to journal › Article › Academic

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.

Original language	English
Article number	0
Pages (from-to)	381-383
Number of pages	3
Journal	EAS Publications Series
Volume	55
Early online date	27 Jun 2012
DOIs	https://doi.org/10.1051/eas/1255054
Publication status	Published - 27 Jun 2012

Keywords

Solar activity
solar diameter

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10.1051/eas/1255054

http://dx.doi.org/10.1051/eas/1255054

Cite this

@article{307c45502b0a46d99138bd26d149b3a5,

title = "Atmospheric fluctuations below 0.1 Hz during drift-scan solar diameter measurements",

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.",

keywords = "Solar activity, solar diameter",

author = "C sigismondi and A Raponi and {De Rosi}, G and M Bianda and R Ramelli and M Caccia and Matteo Maspero and L Negrini and X Wang",

year = "2012",

month = jun,

day = "27",

doi = "10.1051/eas/1255054",

language = "English",

volume = "55",

pages = "381--383",

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T1 - Atmospheric fluctuations below 0.1 Hz during drift-scan solar diameter measurements

AU - sigismondi, C

AU - Raponi, A

AU - De Rosi, G

AU - Bianda, M

AU - Ramelli, R

AU - Caccia, M

AU - Maspero, Matteo

AU - Negrini, L

AU - Wang, X

PY - 2012/6/27

Y1 - 2012/6/27

N2 - 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.

AB - 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.

KW - Solar activity

KW - solar diameter

U2 - 10.1051/eas/1255054

DO - 10.1051/eas/1255054

M3 - Article

VL - 55

SP - 381

EP - 383

JO - EAS Publications Series

JF - EAS Publications Series

M1 - 0

ER -

Atmospheric fluctuations below 0.1 Hz during drift-scan solar diameter measurements

Abstract

Keywords

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