• Non ci sono risultati.

From solar physics to astrophysics: the Sun as Rosetta stone for understanding astrophysical processes & The

N/A
N/A
Protected

Academic year: 2022

Condividi "From solar physics to astrophysics: the Sun as Rosetta stone for understanding astrophysical processes & The"

Copied!
3
0
0

Testo completo

(1)

MEMORIE DELLA SOCIET ` A ASTRONOMICA ITALIANA

Vol.84 n.2 2013

From solar physics to astrophysics: the Sun as Rosetta stone for understanding astrophysical processes & The

Sun: new tools and ideas in observational solar astrophysics

European week of Astronomy and Space Science

Rome, July 3, 2012 and Rome, July 5-6, 2012 editors:F. Berrilli, I. Ermolli, F. Zuccarello

TABLE OF CONTENTS

Index 281

Foreword 284

Plenary talk

S.K. Solanki, L. Teriaca, P. Barthol, W. Curdt B. Inhester

European Solar Physics: moving from Soho to Solar Orbiter and beyond 286

Special Session - From Solar Physics to Astrophysics: The Sun as Rosetta Stone for understanding astrophysical processes

A. Bonanno

The solar-stellar connection: new insights from the Kepler mission 315 M. P. Di Mauro

From Helio- to Asteroseismology and the progress in stellar physics 325 S. Criscuoli, I. Ermolli, H. Uitenbroek F. Giorgi

On the sensitivity of FeI 617.3 and 630.2 nm line shapes to unresolved magnetic

fields 335

A. Cristaldi, S.L. Guglielmino, F. Zuccarello, I. Ermolli, M. Falco S. Criscuoli

Small-scale brightenings observed in active regions with SST and Hinode 339 M. Falco, F. Zuccarello, S. Criscuoli, A. Cristaldi, S.L. Guglielmino I. Ermolli

Sunspot evolution observed with SST 345

F. Giannattasio, M. Stangalini, D. Del Moro, F. Berrilli

Velocity oscillation amplitude in bipolar active regions through SDO observations 351

(2)

282

S.L. Guglielmino, V. Mart´ınez Pillet, B. Ruiz Cobo, J.C. del Toro Iniesta, L.R. Bellot Rubio, S.K. Solanki and the Sunrise/IMaX team

Inversions of L12-2 IMaX data of an emerging flux mantle 355 M. Massi, E. Ros,D. Boboltz, K. M. Menten, J. Neidh¨ofer, G. Torricelli-Ciamponi J.

Kerp

Interacting coronae of two T Tauri stars 359

P. Romano and F. Zuccarello

Spatial distribution of the magnetic helicity flux measured with SDO/HMI in active

regions hosting flares and CMEs 363

H. Uitenbroek S. Criscuoli

A novel method to estimate temperature gradients in stellar photospheres 369 F. Zuccarello S. L. Guglielmino

An orphan penumbra observed with Hinode and DOT 375

Symposium - The Sun: New tools and ideas in observational solar astrophysics

M. Collados, F. Bettonvil, L. Cavaller, I. Ermolli, B. Gelly, A. P´erez, H. Socas-

Navarro, D. Soltau, R. Volkmer, the EST Team

The European Solar Telescope 379

E. Landi Degl’Innocenti

Spectropolarimetry with new generation solar telecopes 391 D. M¨uller, R.G. Marsden O. C. St. Cyr

Scientific synergy between Solar Orbiter and other new observatories 396 G. Trottet K.-L. Klein

Far infrared solar physics 405

M. Bianda, R. Ramelli, J. Stenflo, S. Berdyugina, D. Gisler I. Defilippis

The project of installing a ZIMPOL 3 polarimeter at GREGOR in Tenerife 413 A. Calcines, M. Collados, R. L. L´opez

An integral field spectrograph for the 4-m European Solar Telescope 416 S. Fabiani, R. Bellazzini, F. Berrilli, A. Brez, E. Costa, F. Muleri, M. Pinchera, A.

Rubini, P. Soffitta G. Spandre

A solar flares X-ray polarimeter 422

R. Gafeira, C.C. Fonte, M.A. Pais J. Fernandes

Variation rate of sunspot area 428

L. Giovannelli, F. Berrilli, M. Cocciolo, D. Del Moro, A. Egidi, R. Piazzesi M.

Stangalini

Preliminary test results of the UTOV Fabry-P´erot interferometer prototype 432 C. J. Nelson, J. G. Doyle, R. Erd´elyi, M. Madjarska S. J. Mumford

Ellerman Bombs: Small-Scale Brightenings in the Photosphere 436

(3)

283 S. Scardigli, D. Del Moro F. Berrilli

The multiscale nature of magnetic pattern on the solar surface 440 M. Stangalini, S. K. Solanki R. Cameron

MHD waves in small magnetic elements: comparing IMaX observations to simula-

tions 444

Riferimenti

Documenti correlati

Figure 38 Theoretical (solid curve) and measured (cir- cles) reflectance versus angle at 121, 6nm line for ML0 overcoated by Tungsten capping- layer CL4 58.. Figure 39

In conclusion, our data show that a structured physical activity intervention that includes, along with aerobic training, also specific exercises for strength, flexibility, balance

È plausibile, essendo i Conser vatori a gestire il flusso di denaro più rilevante (fra le entrate, quelle connesse all’appalto dei diritti di pesca sul Lago Trasimeno e al

- mandatory regional registration in order to have ac- cess to contracts with public agencies and tax breaks. Based on what has been illustrated up to now, Italian VOs

The EWASS 2012 conference held in Rome, July 1-6, 2012, hosted two events on solar physics research, the Special Session “From Solar Physics to Astrophysics: The Sun as Rosetta

At the spatial resolution that is now achiev- able the Sun has revealed to us a rich variety of structures and phenomena that include gran- ules and supergranules, convection cells

In this scenario, it is es- sential to understand: how do coronal mass ejections evolve through the corona and inner heliosphere and perturb the solar wind, how these

Preliminary results of this study suggest, for instance, that there may be an analogy between blobs created by tearing instability in current sheets (CSs) associated with solar