Search Results - "VITICCHIE, B"

Imaging Spectropolarimetry with IBIS. II. On the Fine Structure of G-band Bright Features by Viticchié, B, Del Moro, D, Criscuoli, S, Berrilli, F

“…We present new results from first observations of the quiet solar photosphere performed through the Interferometric BIdimensional Spectrometer (IBIS) in…”
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Meteosat Third Generation (MTG): Continuation and Innovation of Observations from Geostationary Orbit by Holmlund, K., Grandell, J., Schmetz, J., Stuhlmann, R., Bojkov, B., Munro, R., Lekouara, M., Coppens, D., Viticchie, B., August, T., Theodore, B., Watts, P., Dobber, M., Fowler, G., Bojinski, S., Schmid, A., Salonen, K., Tjemkes, S., Aminou, D., Blythe, P.

“…Within the next couple of years, the European Organisation for the Exploitation of Meteorological Satellites (EUMETSAT) will start the deployment of its…”
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MODEL SELECTION FOR SPECTROPOLARIMETRIC INVERSIONS by ASENSIO RAMOS, A, MANSO SAINZ, R, MARTINEZ GONZALEZ, M. J, VITICCHIE, B, OROZCO SUAREZ, D, SOCAS-NAVARRO, H

“…Inferring magnetic and thermodynamic information from spectropolarimetric observations relies on the assumption of a parameterized model atmosphere whose…”
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Statistical Properties of Synthetic Nanoflares by Viticchié, B, Del Moro, D, Berrilli, F

“…Statistical properties of flares are a powerful tool for addressing the upper solar atmosphere heating problem. We simulate time series of synthetic flares by…”
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Quiet-Sun Magnetic Field Measurements Based on Lines with Hyperfine Structure by Sánchez Almeida, J, Viticchié, B, Landi Degl'Innocenti, E, Berrilli, F

“…The Zeeman pattern of Mn i lines is sensitive to hyperfine structure (HFS), and because of this, they respond to hectogauss magnetic field strengths…”
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A Comparative Analysis of Photospheric Bright Points in an Active Region and in the Quiet Sun by Romano, P., Berrilli, F., Criscuoli, S., Del Moro, D., Ermolli, I., Giorgi, F., Viticchié, B., Zuccarello, F.

“…We present a comparative study of photometric and dynamic properties of photospheric bright points (BPs) observed at the disk centre in the active region (AR)…”
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Imaging Spectropolarimetry with IBIS: Evolution of Bright Points in the Quiet Sun by Viticchié, B, Del Moro, D, Berrilli, F, Bellot Rubio, L, Tritschler, A

“…We present the results from first spectropolarimetric observations of the solar photosphere acquired at the Dunn Solar Telescope with the Interferometric…”
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ON THE POLARIMETRIC SIGNATURE OF EMERGING MAGNETIC LOOPS IN THE QUIET SUN by VITICCHIE, B

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Modeling the solar irradiance background via numerical simulation by Viticchié, B., Vantaggiato, M., Berrilli, F., del Moro, D., Penza, V., Pietropaolo, E., Rast, M.

“…Various small scale photospheric processes are responsible for spatial and temporal variations of solar emergent intensity. The contribution to total…”
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IMAGING SPECTROPOLARIMETRY WITH IBIS: EVOLUTION OF BRIGHT POINTS IN THE QUIET SUN by Viticchie, B., Del Moro, D., Berrilli, F., Bellot Rubio, L., Tritschler, A.

“…We present the results from first spectropolarimetric observations of the solar photosphere acquired at the Dunn Solar Telescope with the Interferometric…”
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On the polarimetric signature of emerging magnetic loops in the quiet-Sun by Viticchie, B

“…The abundance of Stokes V profiles dominated by one lobe at the locations of emergence of Omega-shaped magnetic loops is evaluated. The emergence events were…”
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Magnetic field distribution in the quiet Sun: a simplified model approach by Berrilli, F, Del Moro, D, Viticchie, B

“…We simulate the dynamics and the evolution of quiet Sun magnetic elements to produce a probability density function of the field strengths associated with such…”
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Magnetic bright points in the quiet Sun by Almeida, J. Sanchez, Bonet, J. A, Viticchie, B, Del Moro, D

“…Astrophys.J. 715 (2010) L26 We present a visual determination of the number of bright points (BPs) existing in the quiet Sun, which are structures though to…”
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Model selection for spectro-polarimetric inversions by Ramos, A. Asensio, Sainz, R. Manso, Gonzalez, M. J. Martinez, Viticchie, B, Suarez, D. Orozco, Socas-Navarro, H

“…Inferring magnetic and thermodynamic information from spectropolarimetric observations relies on the assumption of a parameterized model atmosphere whose…”
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Quiet Sun Magnetic Field Measurements Based on Lines with Hyperfine Structure by Almeida, J. Sanchez, Viticchie, B, Degl'Innocenti, E. Landi, Berrilli, F

“…The Zeeman pattern of MnI lines is sensitive to hyperfine structure (HFS) and, they respond to hG magnetic field strengths differently from the lines used in…”
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Asymmetries of the Stokes V profiles observed by HINODE SOT/SP in the quiet Sun by Viticchié, B, Almeida, J. Sánchez

“…We present the first classification of SOT/SP circular polarization measurements with the aim of highlighting exhaustively the whole variety of Stokes V shapes…”
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High cadence spectropolarimetry of moving magnetic features observed around a pore by Criscuoli, S, Del Moro, D, Giannattasio, F, Viticchié, B, Giorgi, F, Ermolli, I, Zuccarello, F, Berrilli, F

“…Moving magnetic features (MMFs) are small-size magnetic elements that are seen to stream out from sunspots, generally during their decay phase. Several…”
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Interpretation of HINODE SOT/SP asymmetric Stokes profiles observed in quiet Sun network and internetwork by Viticchié, B, J, Almeida, Sánchez, Del Moro, D, Berrilli, F

“…We present the first interpretation of the Stokes profile asymmetries measured in the FeI 630 nm lines by SOT/SP, in both quiet Sun internetwork (IN) and…”
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Imaging Spectropolarimetry with IBIS II: on the fine structure of G-band bright features by Viticchié, B, Del Moro, D, Criscuoli, S, Berrilli, F

“…We present new results from first observations of the quiet solar photosphere performed through the Interferometric BIdimensional Spectrometer (IBIS) in…”
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Properties of G-band Bright Points derived from IBIS observations by Criscuoli, S, Del Moro, D, Giorgi, F, Romano, P, Berrilli, F, Ermolli, I, Viticchié, B, Zuccarello, F

“…We have investigated properties of photospheric Bright Points (BPs) observed in an Active Region during its decay phase and in a quiet Sun region. We have…”
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