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Vamos: Velocity and Magnetic Observations of the Sun: Calibration and Data Analysis

Published online by Cambridge University Press:  08 February 2017

M. Oliviero
Affiliation:
Dipartimento di Scienze Fisiche dell'Università “Federico II”, Mostra D‘Oltremare Pad. 19, 80125 Napoli, Italy
G. Severino
Affiliation:
Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy
Th. Straus
Affiliation:
Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy
A. Cacciani
Affiliation:
Dipartimento di Fisica dell’Università “La Sapienza”, P.le A. Moro 2, 00185 Roma, Italy
M. Dolci
Affiliation:
Dipartimento di Fisica dell’Università “La Sapienza”, P.le A. Moro 2, 00185 Roma, Italy
P.F. Moretti
Affiliation:
Dipartimento di Fisica dell’Università “La Sapienza”, P.le A. Moro 2, 00185 Roma, Italy

Extract

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This poster illustrates the calibration procedure and the analysis pipeline developed for the helioseismology data acquired with the VAMOS (Velocity And Magnetic Observations of the Sun) instrument. The VAMOS, based on the MOF (Magneto-Optical Filter) technology, and its operation are discussed in detail elsewhere (Cacciani et al., 1997 and Moretti et al., 1997).

Type
I. Global Structure and Evolution of the Solar and Stellar Interior
Copyright
Copyright © Kluwer 1998 

References

Cacciani, A., Marmolino, C., Moretti, P.F., Oliviero, M., Severino, G., Smaldone, L.A.: 1997, Mem. SAIt. in press.Google Scholar
Moretti, P.F., Severino, G., Cauzzi, G., Reardon, K., and Straus, T., Cacciani, A., Marmolino, C., Oliviero, M., and Smaldone, L.A.: 1997, in Pijpers, F.P., Christensen-Dalsgaard, J., and Rosenthal, C.S. (eds.), “SCORe'96: Solar Convection and Oscillations and their Relationship”, Kluwer, Dordrecht, p. 293.CrossRefGoogle Scholar