Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
I.N.A.F., Osservatorio Astronomico di Capodimonte, Via Moiarello 16, 80131 Napoli, Italy
Department of Physics, University of Rome `La Sapienza', P.le A. Moro 2, 00185 Rome, Italy
Osservatorio Astronomico di Capodimonte, I-80131 Napoli, Italy
Istituto Tecnico Industriale Statale E. Fermi, via Trionfale 8737, Roma 00133, Italy
INAF, Osservatorio Astronomico di Capodimonte, via Moiarello 16, 80131 Napoli, Italy
Department of Physics, University of Rome `La Sapienza', 00185 Rome, Italy Osservatorio Astronomico di Capodimonte, Via Moiariello 16, I-80131 Napoli, Italy
Osservatorio Astronomico di Capodimonte, Napoli
Roma I, Univ., Rome, Italy
I.T.I.S. G. Galilei, via Ponchielli, Latina 04100, Italy ; Department of Earth Sciences University of Rome La Sapienza, P.le A. Moro 2, 00185 Rome, Italy
Univ. La Sapienza di Roma
Universitàdegli Studi di Roma "La Sapienza", P.le A. Moro 5, 00185 Rome, Italy; Osservatorio Astronomico di Roma, Via Frascati 33, 00040, Monte Porzio Catone, Italy
Department of Earth and Environment, CNR
Headquarter of National Research Council, Piazzale Aldo Moro
Istituto Nazionale di Astrofisica, Osservatorio Astronomico di Capodimonte, Via Moiarello 16, I-80131 Naples, Italy Tecnico Industriale Statale "G. Galilei", via Ponchielli, I-04100 Latina, Italy
Department of Physics, University of Rome `La Sapienza', P. A. Moro 2, I-00185 Roma, Italy
INAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, I-80131 Naples, Italy.
University of Rome "La Sapienza
A model to interpret the intensity-velocity and velocity-velocity phase differences from solar observations obtained with magneto-optical filters
A new limit on the observed amplitude of Jovian global oscillations
A Search for Photospheric Sources of Coronal Longitudinal Oscillations
AFM, FE-SEM and Optical Imaging of a Shocked L/LL Chondrite: Implications for Martensite Formation and Wave Propagation
An interpretation of the I-V phase background based on observed plasma jets
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