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91探花
Black Hole

Lensing of space time around a black hole. At 91探花 we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Jay Sahota

Project Portfolio Manager

Sub department

  • Astrophysics
jay.sahota@physics.ox.ac.uk
Telephone: 01865 273319
Denys Wilkinson Building, room 603A
  • About
  • Publications

Rock鈥恗agnetic characterization of early, redoxomorphic diagenesis in turbiditic sediments from the Madeira Abyssal Plain

Sedimentology Wiley 47:2 (2000) 367-394

Authors:

Simon G Robinson, John TS Sahota

Early diagenesis in North Atlantic abyssal plain sediments characterized by rock-magnetic and geochemical indices

Marine Geology Elsevier 163:1-4 (2000) 77-107

Authors:

Simon G Robinson, John TS Sahota, Frank Oldfield

Magnetic measurements of Greenland and Himalayan ice-core samples

Holocene SAGE Publications 6:4 (1996) 477-480

Authors:

JTS Sahota, PA Mayewski, F Oldfield, Et al.

Abstract:

This paper summarizes Isothermal Remanence (IRM300mT) measurements from Holocene ice-core samples from two contrasting glaciological regimes: (i) the Greenland ice sheet and (ii) a Himalayan glacier. Cores had been previously characterized in terms of chronologies, geochemistry and, for the Himalayan core, microparticle concentrations. Six samples from the Greenland 20-D ice core from the time period AD 1876-1983 did not yield magnetic measurements above instrumental noise-level. Significant Isothermal Remanence measurements (IRM300mT) were obtained from some levels in the Himalayan ice core. Scanning electron microscopy and EDAX analyses indicate weathered crustal material. The techniques used require ice-core samples with relatively high dust loadings and/or larger volume ice samples.

Magnetic measurements used to identify paleoxidation fronts in deep鈥恠ea sediments from the Madeira Abyssal Plain

Geophysical Research Letters American Geophysical Union (AGU) 22:15 (1995) 1961-1964

Authors:

JTS Sahota, SG Robinson, F Oldfield

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OX1 3PU

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