Publications based on hydrodynamic and MHD models using either the FLASH or the PLUTO code. The numerical simulations have been performed on a variety of supercomputers, including the IBM Sp5, Sp6, and the Linux clusters CLX and BCX hosted at CINECA (Italy), the Linux clusters hosted at the HPC facility SCAN of INAF-OAPA (Italy), and the Grid Infrastructure of Consorzio COMETA (Italy).

• SOLAR PHYSICS

  • MHD-modeling of the propagation of a coronal mass ejection
    Pagano P., Reale F., Orlando S., Peres G. 2007, A&A 464, 753

  • Modeling magnetohydrodynamics and non-equilibrium SoHO/UVCS line emission of CME shocks
    Pagano P., Raymond J.C., Reale F., Orlando S. 2008, A&A 481, 835

  • Nonequilibrium of Ionization and the Detection of Hot Plasma in Nanoflare-heated Coronal Loops
    Reale F., Orlando S. 2008, ApJ 684, 715

  • Post-flare UV light curves explained with thermal instability of loop plasma
    Reale F., Landi E., Orlando S. 2012, ApJ 746, 18

• YOUNG STELLAR OBJECTS AND PROTOSTELLAR JETS

  • The X-ray Emission Mechanism in the Protostellar Jet HH 154
    Bonito R., Orlando S., Peres G., Favata F., Rosner R. 2004, A&A 424, L1

  • X-rays from protostellar jets: emission from continuous flows
    Bonito R., Orlando S., Peres G., Favata F., Rosner R. 2007, A&A 462, 645

  • Generation of radiative knots in a randomly pulsed protostellar jet I. Dynamics and energetics
    Bonito R., Orlando S., Peres G., Eisloffel J., Miceli M., Favata F. 2010, A&A 511, A42

  • Generation of radiative knots in a randomly pulsed protostellar jet II. X-ray emission
    Bonito R., Orlando S., Miceli M., Eisloffel J., Peres G., Favata F. 2010, A&A 517, A68

  • X-ray emission from protostellar jet HH 154: the first evidence of a diamond shock?
    Bonito R., Orlando S., Miceli M., Peres G., Micela G., Favata F. 2011, ApJ 737, id. 54

  • X-ray emitting MHD accretion shocks in classical T Tauri stars. Case for moderate to high plasma-beta values
    Orlando S., Sacco G.G., Argiroffi C., Reale F., Peres G., Maggio A. 2010, A&A 510, A71

  • Mass accretion to young stars triggered by flaring activity in circumstellar disks
    Orlando S., Reale F., Peres G., Mignone A. 2011, MNRAS 415, 3380

  • X-ray emission from dense plasma in CTTSs: Hydrodynamic modeling of the accretion shock
    Sacco G.G., Argiroffi C., Orlando S., Maggio A., Peres G., Reale F. 2008, A&A 491, L17

  • On the observability of T Tauri accretion shocks in the X-ray band
    Sacco G.G., Orlando S., Argiroffi C., Maggio A., Peres G., Reale F., Curran R.L. 2010, A&A 522, A55

• NOVA OUTBURSTS

  • Three-dimensional modeling of the asymmetric blast wave from the 2006 outburst of RS Ophiuchi: Early X-ray emission
    Orlando S., Drake J.J., Laming J.M. 2009, A&A 493, 1049

  • The early blast wave of the 2010 explosion of U Scorpii
    Drake J.J., Orlando S. 2010, ApJ 720, L195

  • Modeling the 2010 blast wave of the symbiotic-like nova V407 Cygni
    Orlando S., Drake J.J. 2012, MNRAS 419, 2329

• SUPERNOVA REMNANTS

  • Constraints on local interstellar magnetic field from non-thermal emission of SN1006
    Bocchino F., Orlando S., Miceli M., Petruk O. 2011, A&A 531, A129

  • Shock-cloud interaction in the Vela SNR II. Hydrodynamic model
    Miceli M., Reale F., Orlando S., Bocchino F. 2006, A&A 458, 213

  • Crushing of Interstellar Gas Clouds in Supernova Remnants I. The Role of Thermal Conduction and Radiative Losses
    Orlando S., Peres G., Reale F., Bocchino F., Rosner R., Plewa T., Siegel A. 2005, A&A 444, 505

  • Crushing of Interstellar Gas Clouds in Supernova Remnants II. X-ray Emission
    Orlando S., Bocchino F., Peres G., Reale F., Plewa T., Rosner R. 2006, A&A 457, 545

  • On the Origin of Asymmetries in Bilateral Supernova Remnants
    Orlando S., Bocchino F., Reale F., Peres G., Petruk O. 2007, A&A 470, 927

  • The importance of magnetic-field-oriented thermal conduction in the interaction of SNR shocks with interstellar clouds
    Orlando S., Bocchino F., Reale F., Peres G., Pagano P. 2008, ApJ 678, 274

  • Modeling SNR shock waves expanding through the magnetized inhomogeneous interstellar medium
    Orlando S., Bocchino F., Miceli M., Reale F., Peres G. 2009, Il Nuovo Cimento C 32, 45

  • Observability and diagnostics in the X-ray band of shock-cloud interactions in supernova remnants
    Orlando S., Bocchino F., Miceli M., Zhou X., Reale F., Peres G. 2010, A&A 514, A29

  • Effects of non-uniform interstellar magnetic field on synchrotron X-ray and inverse-Compton gamma-ray morphology of SNRs
    Orlando S., Petruk O., Bocchino F., Miceli M. 2011, A&A 526, A129

  • Role of Ejecta Clumping and Back-reaction of Accelerated Cosmic Rays in the Evolution of Type Ia Supernova Remnants
    Orlando S., Bocchino F., Miceli M., Petruk O., Pumo M.L. 2012, ApJ 749, 156

  • Unveiling the spatial structure of the overionized plasma in the supernova remnant W49B
    Zhou X., Miceli M., Bocchino F., Orlando S., Chen Y. 2011, MNRAS 415, 244