The structure and unsteadiness characteristics of a shock train in a constant-area ducted flow are studied experimentally as a function of duct back pressure, which is mechanically controlled by a valve. Increasing the back pressure pushes the shock train upstream where the approach conditions (including Mach number and boundary-layer momentum thickness) are different, as these quantities vary along the duct length. Despite nominally constant boundary conditions during a run, the shock train fluctuates about its time-averaged position. Schlieren imaging reveals that the unsteadiness characteristics, including the fluctuation amplitude and frequency content, are independent of back pressure. However, changes in the Mach stem length and shock angles demonstrate that the leading shock structure transitions from oblique to normal as back pressure increases. Time-averaged pressure profiles show that the shock train length decreases and the pressure rise across the shock train increases during this process, but these quantities are nominally constant when normalized by the approach conditions. Finally, stereo particle image velocimetry is used to study the three-dimensional structure of a normal leading shock. The velocity fields show a large separation region on the side-wall of the duct and a degree of axisymmetry that indicates a nominally conical shock structure.
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Imperial Coll London, Dept Phys, Blackett Lab, London SW7 2AZ, EnglandImperial Coll London, Dept Phys, Blackett Lab, London SW7 2AZ, England
Trotta, D.
Pezzi
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CNR, Ist Sci & Tecnol Plasmi ISTP, Via Amendola 122-D, I-70126 Bari, ItalyImperial Coll London, Dept Phys, Blackett Lab, London SW7 2AZ, England
Pezzi
Burgess, D.
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Queen Mary Univ London, Dept Phys & Astron, London E1 4NS, EnglandImperial Coll London, Dept Phys, Blackett Lab, London SW7 2AZ, England
Burgess, D.
Preisser, L.
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Austrian Acad Sci, Space Res Inst, A-8042 Graz, AustriaImperial Coll London, Dept Phys, Blackett Lab, London SW7 2AZ, England
Preisser, L.
Blanco-Cano, X.
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Univ Nacl Autonoma Mexico, Inst Geofis, Dept Ciencias Espaciales, Ciudad Univ, Ciudad De Mexico 0451, MexicoImperial Coll London, Dept Phys, Blackett Lab, London SW7 2AZ, England
Blanco-Cano, X.
Kajdic, P.
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Univ Nacl Autonoma Mexico, Inst Geofis, Dept Ciencias Espaciales, Ciudad Univ, Ciudad De Mexico 0451, MexicoImperial Coll London, Dept Phys, Blackett Lab, London SW7 2AZ, England
Kajdic, P.
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Hietala, H.
Horbury, T. S.
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Imperial Coll London, Dept Phys, Blackett Lab, London SW7 2AZ, EnglandImperial Coll London, Dept Phys, Blackett Lab, London SW7 2AZ, England
Horbury, T. S.
Vainio, R.
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Univ Turku, Dept Phys & Astron, FI-20014 Turku, FinlandImperial Coll London, Dept Phys, Blackett Lab, London SW7 2AZ, England
Vainio, R.
Dresing, N.
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Univ Turku, Dept Phys & Astron, FI-20014 Turku, FinlandImperial Coll London, Dept Phys, Blackett Lab, London SW7 2AZ, England
Dresing, N.
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Retino, A.
Marcucci, M. F.
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INAF Ist Astrofis & Planetol Spaziali, I-00133 Rome, ItalyImperial Coll London, Dept Phys, Blackett Lab, London SW7 2AZ, England
Marcucci, M. F.
Sorriso-Valvo, L.
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CNR, Ist Sci & Tecnol Plasmi ISTP, Via Amendola 122-D, I-70126 Bari, Italy
KTH Royal Inst Technol, Sch Elect Engn & Comp Sci, Space & Plasma Phys, SE-10044 Stockholm, Sweden
Swedish Inst Space Phys IRF, Angstrom Lab, Lagerhyddsvagen 1, SE-75121 Uppsala, SwedenImperial Coll London, Dept Phys, Blackett Lab, London SW7 2AZ, England