Resonant curve of geo-synchronous satellite including effect of earth’s equatorial ellipticity and resistive force using perturbations technique

New Astronomy ◽  
2021 ◽  
Vol 86 ◽  
pp. 101573
Author(s):  
Sushil Yadav ◽  
Mukesh Kumar ◽  
Virendra Kumar
Actuators ◽  
2020 ◽  
Vol 10 (1) ◽  
pp. 5
Author(s):  
Yong Hae Heo ◽  
Sangkyu Byeon ◽  
Tae-Hoon Kim ◽  
In-Ho Yun ◽  
Jin Ryong Kim ◽  
...  

This paper presents a magneto-rheological (MR) actuator that can be easily inserted into haptic shoes and can haptically simulate the material properties of the ground. To increase the resistive force of the proposed actuator, we designed a movable piston having multiple operation modes of MR fluids. Further, the design of a solenoid coil was optimized to maximize the resistive force in a limited-sized MR actuator. Simulations were conducted to predict the actuation performance and to show that the magnetic flux flows well by forming a closed loop in the proposed actuator. The quantitative evaluation of the proposed actuator was investigated by measuring the resistive force as a function of the input current and its pressed depth. From the result, we found that the proposed actuator can create over 600 N by adjusting the input current.


2018 ◽  
Vol Volume 13 ◽  
pp. 211-220 ◽  
Author(s):  
Junji Katsuhira ◽  
Sumiko Yamamoto ◽  
Nodoka Machida ◽  
Yuji Ohmura ◽  
Masako Fuchi ◽  
...  

2019 ◽  
Vol 879 ◽  
pp. 808-833 ◽  
Author(s):  
B. J. Walker ◽  
K. Ishimoto ◽  
H. Gadêlha ◽  
E. A. Gaffney

We present a generalisation of efficient numerical frameworks for modelling fluid–filament interactions via the discretisation of a recently developed, non-local integral equation formulation to incorporate regularised Stokeslets with half-space boundary conditions, as motivated by the importance of confining geometries in many applications. We proceed to utilise this framework to examine the drag on slender inextensible filaments moving near a boundary, firstly with a relatively simple example, evaluating the accuracy of resistive force theories near boundaries using regularised Stokeslet segments. This highlights that resistive force theories do not accurately quantify filament dynamics in a range of circumstances, even with analytical corrections for the boundary. However, there is the notable and important exception of movement in a plane parallel to the boundary, where accuracy is maintained. In particular, this justifies the judicious use of resistive force theories in examining the mechanics of filaments and monoflagellate microswimmers with planar flagellar patterns moving parallel to boundaries. We proceed to apply the numerical framework developed here to consider how filament elastohydrodynamics can impact drag near a boundary, analysing in detail the complex responses of a passive cantilevered filament to an oscillatory flow. In particular, we document the emergence of an asymmetric periodic beating in passive filaments in particular parameter regimes, which are remarkably similar to the power and reverse strokes exhibited by motile$9+2$cilia. Furthermore, these changes in the morphology of the filament beating, arising from the fluid–structure interactions, also induce a significant increase in the hydrodynamic drag of the filament.


1986 ◽  
Vol 114 ◽  
pp. 293-295
Author(s):  
K. B. Bhatnagar

The motion of a geosynchronous satellite has been studied under the combined gravitational effects of the oblate Earth (including its equatorial ellipticity), the Sun, the Moon and the solar-radiation pressure. It is observed that the orbital plane rotates with an angular velocity the maximum value of which is 0.058°/yr. and regresses with a period which increases both as the orbital inclination and the altitude increase. The effect of earth's equatorial ellipticity on the regression period is oscillatory whereas that of Solar-radiation pressure is to decrease it.The synchronism is achieved when the angular velocity of the satellite is equal to the difference between the spin-rate of the Earth and the regression rate of the orbital plane. With this angular velocity of the satellite, the ground trace is in the shape of figure eight, though its size and position relative to the Earth change as the time elapses. The major effect of earth's equatorial ellipticity is to produce a change in the relative angular position of the satellite as seen from the Earth. If the satellite is allowed to execute large angle oscillations the mid-point of oscillation would be at the position of the minor axis of the earth's equatorial section. The oscillatory period T has been determined in terms of the amplitude Γ and the tesseral harmonic J2(2). From this result we can determine the value of J2(2) as T and Γ can be observed accurately.


2014 ◽  
Vol 10 (3) ◽  
pp. 285-293 ◽  
Author(s):  
Xiao-wei Chen ◽  
Ji-cheng Li

2010 ◽  
Vol 213 (8) ◽  
pp. 1226-1234 ◽  
Author(s):  
B. M. Friedrich ◽  
I. H. Riedel-Kruse ◽  
J. Howard ◽  
F. Julicher

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