| Issue |
EAS Publications Series
Volume 55, 2012
4th French-Chinese Meeting on Solar Physics - Understanding Solar Activity: Advances and Challenges
|
|
|---|---|---|
| Page(s) | 381 - 383 | |
| Section | Instrumentation | |
| DOI | https://doi.org/10.1051/eas/1255054 | |
| Published online | 27 June 2012 | |
M. Faurobert, C. Fang and T. Corbard (eds)
EAS Publications Series, 55 (2012) 381-383
Atmospheric fluctuations below 0.1 Hz during drift-scan solar diameter measurements
1
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
2
Sapienza University of Rome,
Italy
3
IRSOL, Locarno, Switzerland
4
Como University,
Italy
5
Huairou Solar Observing Station, National Astronomical
Observatories, Chinese Academy of Sciences, Beijing, China
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.
© EAS, EDP Sciences 2012