Results 31 to 40 of about 124,500 (193)
The numerical study on active control strategies of T-foil
ObjectivesAn active control T-foil can effectively improve the longitudinal anti-rolling motion of the ship, but there is still no conclusion on what control strategy has the best anti-rolling effect.
Yichen JIANG +4 more
doaj +1 more source
The ULF wave foreshock boundary: Cluster observations [PDF]
The interaction of backstreaming ions with the incoming solar wind in the upstream region of the bow shock gives rise to a number of plasma instabilities from which ultra-low frequency (ULF) waves can grow.
Andres, Nahuel +4 more
core +2 more sources
The Martian bow wave—Theory and observation [PDF]
Refinement of the relationship between the trajectory of Mariner 4 in its fly-by of Mars and the calculated location of a proposed Martian bow arising from interaction of the solar wind and the ionosphere by inclusion of aberration effects of the planet's motion about the sun.
J.R. Spreiter, A.W. Rizzi
openaire +1 more source
The performance of bow foils in irregular and oblique waves
Bow foils are an emerging energy saving device that utilise wave energy to improve the efficiency of ships operating in waves, through both a reduction in ship motions and the generation of additional thrust.
J.A. Bowker, N.C. Townsend
doaj +1 more source
Planetary magnetosheaths are characterized by high plasma wave and turbulence activity. The Martian magnetosheath is no exception; both upstream and locally generated plasma waves have been observed in the region between its bow shock and magnetic ...
A. M. S. Franco +3 more
doaj +1 more source
Structural and Electronic Instabilities in Polyacenes: Density Matrix Renormalization Group Study of a Long--Range Interacting Model [PDF]
We have carried out Density Matrix Renormalization Group (DMRG) calculations on the ground state of long polyacene oligomers within a Pariser-Parr-Pople (PPP) Hamiltonian.
A. K. Bakshi +52 more
core +2 more sources
Mesoscale modeling of Venus' bow-shape waves [PDF]
The Akatsuki instrument LIR measured an unprecedented wave feature at the top of Venusian cloud layer. Stationary bow-shape waves of thousands of kilometers large lasting several Earth days have been observed over the main equatorial mountains. Here we use for the first time a mesoscale model of the Venus's atmosphere with high-resolution topography ...
Lefèvre, Maxence +2 more
openaire +4 more sources
Phase diagram of the one-dimensional half-filled extended Hubbard model
We study the ground state of the one-dimensional half-filled Hubbard model with on-site (nearest-neighbor) repulsive interaction $U$ ($V$) and nearest-neighbor hopping $t$.
D. Baeriswyl +5 more
core +1 more source
Recently it has been discussed whether a bow shock ahead of the heliospheric stagnation region does exist or not. This discussion was triggered by measurements indicating that the Alfv\'en speed and that of fast magnetosonic waves are higher than the ...
Fichtner, Horst, Scherer, Klaus
core +1 more source
Bow shocks, bow waves, and dust waves. IV. Shell shape statistics
21 pages, 16 figures.
Henney, William J. +3 more
openaire +2 more sources

