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Atomic and Laser Physics
Credit: Jack Hobhouse

Dr Francesco Miniati

Researcher in Computational Physics

Sub department

  • Atomic and Laser Physics

Research groups

  • Quantum high energy density physics
francesco.miniati@physics.ox.ac.uk
Clarendon Laboratory, room Simon room
  • About
  • Publications

THE ZURICH ENVIRONMENTAL STUDY (ZENS) OF GALAXIES IN GROUPS ALONG THE COSMIC WEB. II. GALAXY STRUCTURAL MEASUREMENTS AND THE CONCENTRATION OF MORPHOLOGICALLY CLASSIFIED SATELLITES IN DIVERSE ENVIRONMENTS**Based on observations collected at the European Southern Observatory, La Silla Chile, Program ID 177.A-0680.

The Astrophysical Journal American Astronomical Society 776:2 (2013) 72

Authors:

A Cibinel, CM Carollo, SJ Lilly, F Miniati, JD Silverman, JH van Gorkom, E Cameron, A Finoguenov, P Norberg, Y Peng, A Pipino, CS Rudick
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THE ZURICH ENVIRONMENTAL STUDY OF GALAXIES IN GROUPS ALONG THE COSMIC WEB. I. WHICH ENVIRONMENT AFFECTS GALAXY EVOLUTION?**Based on observations collected at the European Southern Observatory, La Silla Chile. Program ID 177.A-0680.

The Astrophysical Journal American Astronomical Society 776:2 (2013) 71

Authors:

C Marcella Carollo, Anna Cibinel, Simon J Lilly, Francesco Miniati, Peder Norberg, John D Silverman, Jacqueline van Gorkom, Ewan Cameron, Alexis Finoguenov, Yingjie Peng, Antonio Pipino, Craig S Rudick
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THE EXTENT OF MAGNETIC FIELDS AROUND GALAXIES OUT TO z ∼ 1**Based on observations made with the ESO Telescopes at the La Silla Observatories under program 082.A-0917 and 085.A-0417.

The Astrophysical Journal Letters American Astronomical Society 772:2 (2013) l28

Authors:

ML Bernet, F Miniati, SJ Lilly
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RELAXATION OF BLAZAR-INDUCED PAIR BEAMS IN COSMIC VOIDS

The Astrophysical Journal American Astronomical Society 770:1 (2013) 54

Authors:

Francesco Miniati, Andrii Elyiv
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Visualizing electromagnetic fields in laser-produced counter-streaming plasma experiments for collisionless shock laboratory astrophysics

Physics of Plasmas 20:5 (2013)

Authors:

NL Kugland, JS Ross, PY Chang, RP Drake, G Fiksel, DH Froula, SH Glenzer, G Gregori, M Grosskopf, C Huntington, M Koenig, Y Kuramitsu, C Kuranz, MC Levy, E Liang, D Martinez, J Meinecke, F Miniati, T Morita, A Pelka, C Plechaty, R Presura, A Ravasio, BA Remington, B Reville, DD Ryutov, Y Sakawa, A Spitkovsky, H Takabe, HS Park

Abstract:

Collisionless shocks are often observed in fast-moving astrophysical plasmas, formed by non-classical viscosity that is believed to originate from collective electromagnetic fields driven by kinetic plasma instabilities. However, the development of small-scale plasma processes into large-scale structures, such as a collisionless shock, is not well understood. It is also unknown to what extent collisionless shocks contain macroscopic fields with a long coherence length. For these reasons, it is valuable to explore collisionless shock formation, including the growth and self-organization of fields, in laboratory plasmas. The experimental results presented here show at a glance with proton imaging how macroscopic fields can emerge from a system of supersonic counter-streaming plasmas produced at the OMEGA EP laser. Interpretation of these results, plans for additional measurements, and the difficulty of achieving truly collisionless conditions are discussed. Future experiments at the National Ignition Facility are expected to create fully formed collisionless shocks in plasmas with no pre-imposed magnetic field. © 2013 AIP Publishing LLC.
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