Del Moro, D. and Criscuoli, S. and Bonet, J.A. and Berrilli, F. and Egidi, A. (2002) Evolution of solar granulation fields from THEMIS-IPM time series. Il nuovo cimento C, 25 (5\6). pp. 595-599. ISSN 1826-9885
|
Text
ncc8833.pdf - Published Version Download (137kB) | Preview |
Abstract
The temporal evolution of solar granulation has been investigated using a time series of high spatial and spectral resolution images acquired at the THEMIS solar telescope (Observatorio del Teide, Tenerife) using the IPM observing mode. In order to investigate different physical properties of solar granulation (associated horizontal velocity fields, lifetimes, intensity and geometry evolution), we identify and track solar granules automatically. We discuss the obtained results and compare them with results reported inthe literature. In order to overcome problems of atmospheric distortions, we also implement a FORTRAN95 code for the application of the Phase Diversity technique that is planned to be used at the THEMIS telescope.
Item Type: | Article |
---|---|
Additional Information: | Paper presented at the International Meeting on THEMIS and the New Frontiers of Solar Atmosphere Dynamics, Rome, Italy, March 19-21, 2001. Based on observations made with THEMIS-CNRS/INSU-CNR operated on the island of Tenerife by THEMIS S.L. in the Spanish Observatorio del Teide of the Instituto de Astrofisica de Canarias. |
Uncontrolled Keywords: | Photosphere, granulation ; Conference proceedings |
Subjects: | 500 Scienze naturali e Matematica > 530 Fisica |
Depositing User: | Marina Spanti |
Date Deposited: | 12 Mar 2020 14:41 |
Last Modified: | 12 Mar 2020 14:41 |
URI: | http://eprints.bice.rm.cnr.it/id/eprint/14851 |
Actions (login required)
View Item |