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Concept

Geomagnetic pole

Publications associées (5)

Underwater propelling device for underwater vehicle

Felix Stephan Schill, Alexander Bahr

The present invention relates to an underwater propelling device (10) i a stator (20) comprising circumferential arrayed coils (35) and being adapted to generate a controlled electromagnetic field along an axial direction, a shaftless propellant rotor (30) ...

2016

Cold pulse and rotation reversals with turbulence spreading and residual stress

Ning Yan

Transport modeling based on inclusion of turbulence spreading and residual stresses shows internal rotation reversals and polarity reversal of cold pulses, with a clear indication of nonlocal transport effects due to fast spreading in the turbulence intens ...

American Institute of Physics (AIP)2016

Renormalization and blow up for wave maps from $S^2 \times \mathbb{R}$ to $S^2$

Sohrab Mirshams Shahshahani

We construct a one parameter family of nite time blow ups to the co-rotational wave maps problem from

S^2\times R

S^2

parameterized by

\nu \epsilon (\frac{1}{2},1]

. The longitudinal function

u(t,\alpha)

which is the main object of study will be ...

2016

Background studies for acoustic neutrino detection at the South Pole

Matthias Wolf, Xiaoxia Bai, Mathieu Ribordy, Shirit Cohen

The detection of acoustic signals from ultra-high energy neutrino interactions is a promising method to measure the flux of cosmogenic neutrinos expected on Earth. The energy threshold for this process depends strongly on the absolute noise level in the ta ...

2012

Search for relativistic magnetic monopoles with the AMANDA-II neutrino telescope

Matthias Wolf, Xiaoxia Bai, Mathieu Ribordy, Shirit Cohen

We present the search for Cherenkov signatures from relativistic magnetic monopoles in data taken with the AMANDA-II detector, a neutrino telescope deployed in the Antarctic ice cap at the Geographic South Pole. The non-observation of a monopole signal in ...

2010

Publications associées (5)

S^2\times R

S^2

parameterized by

\nu \epsilon (\frac{1}{2},1]

. The longitudinal function

u(t,\alpha)

which is the main object of study will be ...

2016

Background studies for acoustic neutrino detection at the South Pole

Matthias Wolf, Xiaoxia Bai, Mathieu Ribordy, Shirit Cohen

2012

Search for relativistic magnetic monopoles with the AMANDA-II neutrino telescope

Matthias Wolf, Xiaoxia Bai, Mathieu Ribordy, Shirit Cohen

2010