Dr Francesco Miniati: Publications

Contrasting environmental effects of astronomically driven climate change on three Eocene hemipelagic successions from the Basque–Cantabrian Basin

Sedimentology Wiley 64:4 (2017) 960-986

Authors:

Naroa Martínez‐Braceras, Aitor Payros, Francesco Miniati, Javier Arostegi, Gloria Franceschetti

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Numerical modeling of laser-driven experiments aiming to demonstrate magnetic field amplification via turbulent dynamo

PHYSICS OF PLASMAS 24:4 (2017) ARTN 041404

Authors:

P Tzeferacos, A Rigby, A Bott, AR Bell, R Bingham, A Casner, F Cattaneo, EM Churazov, J Emig, N Flocke, F Fiuza, CB Forest, J Foster, C Graziani, J Katz, M Koenig, C-K Li, J Meinecke, R Petrasso, H-S Park, BA Remington, JS Ross, D Ryu, D Ryutov, K Weide, TG White, B Reville, F Miniati, AA Schekochihin, DH Froula, G Gregori, DQ Lamb

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Enabling radiative transfer on AMR grids in crash

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 467:2 (2017) 2458-2475

Authors:

N Hariharan, L Graziani, B Ciardi, F Miniati, H-J Bungartz

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FARADAY ROTATION MEASURE SYNTHESIS OF INTERMEDIATE REDSHIFT QUASARS AS A PROBE OF INTERVENING MATTER

The Astrophysical Journal American Astronomical Society 829:2 (2016) 133

Authors:

Kwang Seong Kim, Simon J Lilly, Francesco Miniati, Martin L Bernet, Rainer Beck, Shane P O’Sullivan, Bryan M Gaensler

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Proton imaging of an electrostatic field structure formed in laser-produced counter-streaming plasmas

8th International Conference on Inertial Fusion Sciences and Applications (IFSA 2013) 8–13 September 2013, Nara, Japan IOP Publishing Ltd. 688:1 (2016) 012071-012071

Authors:

T Morita, NL Kugland, W Wan, R Crowston, RP Drake, F Fiuza, Gianluca Gregori, C Huntington, T Ishikawa, M Koenig, C Kuranz, MC Levy, D Martinez, J Meinecke, F Miniati, CD Murphy, A Pelka, C Plechaty, R Presura, N Quirós, BA Remington, B Reville, JS Ross, DD Ryutov, Y Sakawa, L Steele, H Takabe, Y Yamaura, N Woolsey, HS Park

Abstract:

We report the measurements of electrostatic field structures associated with an electrostatic shock formed in laser-produced counter-streaming plasmas with proton imaging. The thickness of the electrostatic structure is estimated from proton images with different proton kinetic energies from 4.7 MeV to 10.7 MeV. The width of the transition region is characterized by electron scale length in the laser-produced plasma, suggesting that the field structure is formed due to a collisionless electrostatic shock.

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Dr Francesco Miniati

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Contrasting environmental effects of astronomically driven climate change on three Eocene hemipelagic successions from the Basque–Cantabrian Basin

Authors:

Numerical modeling of laser-driven experiments aiming to demonstrate magnetic field amplification via turbulent dynamo

Authors:

Enabling radiative transfer on AMR grids in crash

Authors:

FARADAY ROTATION MEASURE SYNTHESIS OF INTERMEDIATE REDSHIFT QUASARS AS A PROBE OF INTERVENING MATTER

Authors:

Proton imaging of an electrostatic field structure formed in laser-produced counter-streaming plasmas

Authors:

Abstract:

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Dr Francesco Miniati

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Contrasting environmental effects of astronomically driven climate change on three Eocene hemipelagic successions from the Basque–Cantabrian Basin

Authors:

Numerical modeling of laser-driven experiments aiming to demonstrate magnetic field amplification via turbulent dynamo

Authors:

Enabling radiative transfer on AMR grids in crash

Authors:

FARADAY ROTATION MEASURE SYNTHESIS OF INTERMEDIATE REDSHIFT QUASARS AS A PROBE OF INTERVENING MATTER

Authors:

Proton imaging of an electrostatic field structure formed in laser-produced counter-streaming plasmas

Authors:

Abstract: