The solar I-V cross-spectrum: A powerful diagnostic for Helioseismology

Severino, G. and Magrì, M. and Oliviero, M. and Straus, Th. and Jefferies, S.M. (2002) The solar I-V cross-spectrum: A powerful diagnostic for Helioseismology. Il nuovo cimento C, 25 (5\6). pp. 529-533. ISSN 1826-9885

[img]
Preview
Text
ncc8824.pdf - Published Version

Download (133kB) | Preview
Official URL: https://www.sif.it/riviste/sif/ncc/econtents/2002/...

Abstract

We discuss results and limitations of a new model for the components of the solar intensity (I) an d velocity (V ) photospheric fluctuations. The model is able to take into account the complex behavior of a low-frequency p-mode, as observed inall the four I and V spectra. We also demonstrate that the solar I-V cross-spectrum provides a sensitive diagnostic for the interaction between the oscillatory and non-oscillatory components of the solar velocity and intensity signals.

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.
Uncontrolled Keywords: Oscillations and waves; helioseismology ; Conference proceedings
Subjects: 500 Scienze naturali e Matematica > 520 Astronomia e scienze connesse
Depositing User: Marina Spanti
Date Deposited: 12 Mar 2020 14:22
Last Modified: 12 Mar 2020 14:22
URI: http://eprints.bice.rm.cnr.it/id/eprint/14834

Actions (login required)

View Item View Item