Results 1 to 10 of about 124,500 (193)
Experimental studies of air entrainment by breaking waves are essential for advancing the understanding of these flows and creating valid models.
Brennen, C. E. +2 more
core +2 more sources
Bow shape has been recognized as an important factor influencing the seakeeping performance and added resistance of ships. This paper presents a numerical comparative study on added resistance and seakeeping of model ships with ‘X-bow’ and a wave ...
Shuling Chen +3 more
doaj +3 more sources
Mirror waves and mode transition observed in the magnetosheath by Double Star TC-1 [PDF]
The Double Star TC-1 magnetosheath pass on 26 February 2004 is used to investigate magnetic field fluctuations. Strong compressional signatures which last for more than an hour have been found near the magnetopause behind a quasi-perpendicular bow ...
J. Du +4 more
doaj +4 more sources
Treatment outcomes of two surgical techniques in secondary reconstruction of unilateral cleft lip and ala nasi utilizing anthropometry assessment: a randomized controlled trial [PDF]
Background An orofacial cleft significantly impacts the oral health-related quality of life of children and teenagers. Secondary reconstruction is a more complex procedure due to tissue deficiency and scarring.
Ebrahim Humadi +2 more
doaj +2 more sources
Investigation of An Inverted Bow on Frigate Hull Resistance [PDF]
This study discusses the inverted bow design on the combatant hull form. Changes in the shape of the stem angle and flare bow are used as analytical parameters to investigate the ship's performance.
S. Samuel +6 more
doaj +1 more source
Bow shocks, bow waves, and dust waves – III. Diagnostics [PDF]
ABSTRACT Stellar bow shocks, bow waves, and dust waves all result from the action of a star’s wind and radiation pressure on a stream of dusty plasma that flows past it. The dust in these bows emits prominently at mid-infrared wavelengths in the range 8 to 60 $\mu$m.
Henney, William J., Arthur, S. J.
openaire +2 more sources
Bow shocks, bow waves, and dust waves – I. Strong coupling limit [PDF]
Dust waves and bow waves result from the action of a star's radiation pressure on a stream of dusty plasma that flows past it. They are an alternative mechanism to hydrodynamic bow shocks for explaining the curved arcs of infrared emission seen around some stars.
Henney, William J., Arthur, S. J.
openaire +2 more sources
Bow shocks, bow waves, and dust waves – II. Beyond the rip point [PDF]
20 pages, 15 figures, MNRAS submitted (revised to correct arXiv links in reference list)
Henney, William J., Arthur, S. J.
openaire +2 more sources
Electron Acceleration by Magnetosheath Jet‐Driven Bow Waves [PDF]
AbstractMagnetosheath jets are localized fast flows with enhanced dynamic pressure. When they supermagnetosonically compress the ambient magnetosheath plasma, a bow wave or shock can form ahead of them. Such a bow wave was recently observed to accelerate ions and possibly electrons. The ion acceleration process was previously analyzed, but the electron
Terry Z. Liu +4 more
openaire +5 more sources
Statistical Study of Magnetosheath Jet‐Driven Bow Waves [PDF]
AbstractWhen a magnetosheath jet (localized dynamic pressure enhancements) compresses ambient magnetosheath at a (relative) speed faster than the local magnetosonic speed, a bow wave or shock can form ahead of the jet. Such bow waves or shocks were recently observed to accelerate particles, thus contributing to magnetosheath heating and particle ...
Terry Z. Liu +5 more
openaire +4 more sources

