Rendezvous in planar environments with obstacles and unknown initial distance

2019 ◽  
Vol 273 ◽  
pp. 19-36 ◽  
Author(s):  
Deniz Ozsoyeller ◽  
Andrew Beveridge ◽  
Volkan Isler
Keyword(s):  
1972 ◽  
Vol 47 ◽  
pp. 402-404
Author(s):  
E. L. Ruskol

According to the Radzievskij-Artemjev hypothesis of the ‘locked’ revolution of the circumplanetary swarms around the Sun, the initial Moon-to-Earth distance and the angular momentum acquired by the Earth through the accretion of the inner part of the swarm can be evaluated. Depending on the concentration of the density to the centre of the swarm we obtain the initial distance for a single protomoon in the range 15–26 Earth radii R and for a system of 3-4 protomoons in the range 3–78 R, if the outer boundary of the swarm equals to the radius of the Hill's sphere (235 R). The total angular momentum acquired by the primitive Earth-Moon system through the accretion of the swarm particles is ½–⅔ of its present value. The rest of it should be acquired from the direct accretion of interplanetary particles by the Earth. The contribution of satellite swarms into the rotation of other planets is relatively less.


1997 ◽  
Vol 29 (4) ◽  
pp. 379-383 ◽  
Author(s):  
Geir Hestmark

AbstractThe pustules on the surface of the umbilicate lichen Lasallia pustulata are moved away from the centre and towards the thallus margins with an average speed of 1.8 mm per year, revealing a growth pattern organized radially and flowing from the centre of the thallus. Pustules close to the margin move substantially faster than those close to the centre; for each 10 mm added to the initial distance from the centre, the speed of outward movement is about doubled. This suggests that intercalary growth over the entire thallus is displaced outwards in an accumulating manner, accelerating the pustules. Moving away from the centre the pustules expand, often collapse in the middle, and mature by developing isidia. In the less active (senescent ?) margins the pustules are eroded away and the supplementary intercalary growth seems insufficient to keep the outflowing thallus intact. Thus the margins are disrupted into irregular lobes.


1993 ◽  
Vol 334 ◽  
Author(s):  
Che-Chen Chang ◽  
Jung-Yen Yang ◽  
Jaw-Chang Shieh

AbstractThe state of the surface after energetic keV particle bombardment is investigated using molecular dynamics. The model utilizes a Ag{110} microcrystallite which is statically bombarded by Ar particles at normal incidence. After being bombarded at incident energy of 1 keV, the relocation probability is <0.3 for all the surface atoms initially residing within four lattice spacings from the target. The probability decreases exponentially as the initial distance of the substrate atom from the target is increased. The most probable distances of displacement from the lattice site also vary with the initial atomic distance from the target atom. The probable displacement of the surface atom, except the target atom, is less than one twentieth of the surface lattice spacing. An analytical formulae for the initial-distance dependence of the relocation probability is also proposed. The formula has three adjustable parameters which are determined by the least-squares method.


2015 ◽  
Vol 771 ◽  
pp. 564-594 ◽  
Author(s):  
Hyeonju Jeong ◽  
Hyungmin Park

The dynamics of a large deformable bubble ($\mathit{Re}\sim \mathit{O}(10^{3})$) rising near a vertical wall in quiescent water is experimentally investigated. The reference (without the wall) rising path of the considered bubble is a two-dimensional zigzag. For a range of wall configurations (i.e. initial wall distance and boundary condition), using high-speed shadowgraphy, various rising behaviours such as periodic bouncing, sliding, migrating away, and non-periodic oscillation without collisions are measured and analysed. Unlike low-Reynolds- and Weber-number bubbles, the contribution of the surface deformation to the transport between the energy components becomes significant during the bubble’s rise. In particular, across the bubble–wall collision, the excess surface energy compensates the deficit of kinetic energy. This enables a large deformable bubble to maintain a relatively constant bouncing kinematics, despite the obvious wall-induced energy dissipation. The wall effect, predominantly appearing as energy loss, is found to decrease as the initial distance from the bubble centre to the wall increases. Compared to the regular (no-slip) wall, a hydrophobic surface enhances or reduces the wall effect depending on the wall distance, whereas a porous surface reduces the energy loss due to the wall, regardless of the initial distance from the wall. Furthermore, the bubble–wall collision behaviour is assessed in terms of a restitution coefficient and modified impact Stokes number (ratio of the inertia to viscous forces), which shows a good correlation, the trends of which agree well with the variations in the energy components. The dependence of near-wall bubble motion on the wall distance and boundary condition may suggest a way of predicting or controlling the near-wall gas void-fraction distribution in gas–liquid flow systems.


2013 ◽  
Vol 29 (6) ◽  
pp. 1366-1379 ◽  
Author(s):  
Deniz Ozsoyeller ◽  
Andrew Beveridge ◽  
Volkan Isler
Keyword(s):  

Author(s):  
Roy J. Crawford

This Paper Proposes A Method For Reconstructing A Certain Type Of Collinear, Front-To-Rear Vehicle Crash, Eastern Kentucky Single-Unit Coal Truck Underrides. The Crashes Discussed Are Those In Which A Following Vehicle Gains Rapidly From A Long Initial Distance On A Leading Slowly Moving Vehicle That Is Not Sufficiently Conspicuous For Crash Avoidance. The Results Of These Analyses Provide Insight Into The Details Of What Occurs In These Types Of Crashes, Show That Inattention And/Or Speeding By The Victims Are Not Necessarily Causes Of The Crashes, And Can Support Or Refute Independent Human Factors Evidence.


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