We discuss determination of kinematic velocities out of kinematic positions that enter the gravity field determination in the form of kinetic orbital energy. After testing several numerical differentiation techniques, we selected conceptually two alternative methods, the Newton-Gregory interpolation and the ...
Transiting planet light curves have historically been used predominantly for measuring the depth and hence ratio of the planetstar radii, p . Equations ha... DM Kipping - 《Monthly Notices of the Royal Astronomical Society》 被引量: 108发表: 2010年 Three-body orbital stability criteria for circu...
derivation of phase rule terminal velocity derivation maxwell boltzmann distribution derivation derivation of prism formula young’s double slits experiment derivation bulk modulus formula derivation coriolis force derivation orbital velocity derivation darcy weisbach equation derivation one dimensional wave equation...
For the Labrador Sea, sediment core logs contain important information about deepwater current velocities and also reflect the variable input of ice-rafted debris from different sources as inferred from grain-size analysis, the relation of density and P wave velocity, and magnetic susceptibility. For...
When a velocity-dependent Lorentz-like gravitomagnetic force is present, the Hamilton vector, as well as the canonical orbital momentum are no longer conserved and begin to precess. It is easy to calculate their precession rates, which are related to the Lense-Thirring precession of the orbit....
The existence of sensor pairs (one at the surface and one in depth) and the availability of P- and S-wave velocity profiles allow deriving two "virtual" datasets associated to outcropping hard rock sites with V~(S)in the range [1000, 3000]?m/s with two independent corrections: 1/down-...
For the Labrador Sea, sediment core logs contain important information about deepwater current velocities and also reflect the variable input of ice-rafted debris from different sources as inferred from grain-size analysis, the relation of density and P wave velocity, and magnetic susceptibility. For...
When a velocity-dependent Lorentzlike gravitomagnetic force is present, the Hamilton vector, as well as the canonical orbital momentum are no longer conserved and begin to precess. It is easy to calculate their precession rates, which are related to the Lense-Thirring precession of the orbit....
velocity nondegenerate equilibrium carrier density/ A7125J Effective mass and g-factors (condensed matter electronic structure) A7320A Surface states, band structure, electron density of states A7115F Atomic- and molecular-orbital methods (condensed matter electronic structure) B0587 Fullerenes, carbon ...
We simulate single particle impacts in various relative velocity directions in space with current ejecta model, in order to figure out features in ejecta orbital evolution such as orbital lifetime. In view of the nearly continuous generation of this secondary source, information of the on-orbit ...