\chapter{Analytical Prediction of Slapdown Magnitude} \section{Introduction} In this chapter, simple equations are developed that can economically be used to estimate the ratio of the initial vertical velocity to the secondary impact velocity during a slapdown impact orientation. The equations can also be used to determine the critical impact angle $\theta_0$ producing the largest secondary impact velocity. The only variables required are geometric and mass quantities; the force-displacement behavior of the impact is not required. \section{Derivation of Slapdown Equation} The body is approximated by the three degree-of-freedom system shown in Figure~\ref{f:gi} on page~\pageref{f:gi}. The force-displacement behavior is approximated by springs located at the initial and secondary impact points. The slapdown equation is developed assuming that (1)~the springs are linear elastic, (2)~there are no horizontal forces due to friction between the rigid surface and the body, and (3)~at most one spring is in contact with the rigid surface at any time. Assumption~(2) reduces the body to a two degree-of-freedom system, and assumption~(3) further reduces it to a sequence of one degree-of-freedom systems. It will be shown that the linear elastic behavior is a conservative assumption that maximizes the secondary impact velocity. In the text that follows, the nose and tail of the body refer to the initial and secondary impact points, respectively. The sign convention used is that displacements, velocities and accelerations are positive downward; and angular positions, velocities and accelerations are positive clockwise. \subsection{Nomenclature} The nomenclature used in the derivation of the Slapdown equation is defined below. \begin{description} \item[$y$,$\dot y$,$\ddot y$] Vertical displacement, velocity, and acceleration. Positive toward rigid surface, \item[$\theta$,$\omega$,$\alpha$] Angular inclination, velocity, and acceleration of the axis of the body with respect to the rigid surface, positive counterclockwise if the nose is to the left of the tail, \item[$m$,$I_{CG}$] Body mass and moment of inertia about the center of gravity, \item[$l$] Length from the center of gravity to the impact point measured along the axis of the body, \item[$k$] Spring constant (force/length), \item[$v_0$,$\theta_0$] Initial vertical velocity and angular position of the body, \item[$\omega_n$] Natural frequency of the differential equation, and \item[$t$] Time. \end{description} For the geometric variables and the linear displacement quantities, the subscripts $(\cdot)_n$ and $(\cdot)_t$ designate the nose and tail of the body, respectively; a superposed dot indicates the time derivative of the dotted quantity. \subsection{Rigid Body Motion Equations} Using D'Alembert's principle, the vertical acceleration $\ddot y_n$ at the nose and the angular acceleration $\alpha$ about the nose during the time interval that only the nose is in contact with the rigid surface can be determined by the summation of moments and forces. \begin{eqnarray} \sum M_n\rightarrow 0 & = & 2 \ddot y_n l_n +\alpha(l_n-r)^2 +\alpha(l_n+r)^2\label{e1} \\ \sum F_n\rightarrow -ky_n & = & \frac{m}{2}\left\{\left[(l_n-r)\alpha +\ddot y_n \right] +\left[(l_n+r)\alpha+\ddot y_n\right]\right\}\label{e2} \end{eqnarray} \begin{tabbing} where: \=ZZ\= \kill where: \>$r $\> is the radius of gyration ${}=\sqrt{\frac{I_{CG}}{m}}$,\\ \>$l_n$\> is the distance from the center of mass to the nose,\\ \>$y_n$\> is the vertical displacement of the nose,\\ \>$k $\> is the elastic spring constant, and\\ \> \> it is assumed that $\cos\theta\approx 1$. \end{tabbing} Equation~\eref{e1} can be used to give $\alpha$ in terms of $\ddot y_n$: \begin{equation} \alpha = \frac{-\ddot y_n l_n}{l_n^2 + r^2}\label{eq:alpha} \end{equation} Using this result, Equation~\eref{e2} can be written as the single degree-of-freedom equation: \begin{equation} \ddot y_n\left[\frac{m}{\beta_n^2+1}\right] + ky_n = 0\label{eq:diff} \end{equation} where $\beta_n$ is defined to be $l_n/r$. Equation~\eref{eq:diff} has the solution \begin{eqnarray} y_n & = & A\cos\omega_n t + B\sin\omega_n t\label{eq:acbs}\\ \omega_n & = & \sqrt{\frac{k}{m}\left(\beta_n^2+1\right)} \end{eqnarray} At time $t=0$, $\dot y_n = v_0$ and $y_n = 0$. Substituting these conditions into Equation~\eref{eq:acbs} results in the following equations for the vertical displacement, velocity, and acceleration of the nose: \begin{eqnarray} y_n & = & \frac{v_0}{\omega_n}\sin\omega_n t\\ \dot y_n & = & v_0\cos\omega_n t\label{eq:vl}\\ \ddot y_n & = & -v_0\omega_n\sin\omega_n t\label{eq:ayl} \end{eqnarray} The angular quantities are determined by substituting Equation~\eref{eq:ayl} into Equation~\eref{eq:alpha} and integrating. \begin{eqnarray} \alpha & = & \frac{\beta_n v_0\omega_n}{r(\beta_n^2+1)}\sin\omega_n t\\ \omega & = & \frac{-\beta_n v_0}{r(\beta_n^2+1)}[\cos\omega_n t - 1] \label{eq:omega}\\ \theta & = & \frac{-\beta_n v_0}{r(\beta_n^2+1)} \left[\frac{\sin\omega_n t}{\omega_n} - t\right] + \theta_0 \label{etheta} \end{eqnarray} These results are only valid during the time interval ($0\leq t\leq \pi / \omega_n$) when the spring is in contact with the rigid surface. For times $t>\pi/\omega_n$ and before the tail contacts the rigid surface, \begin{eqnarray} \alpha & = & 0, \\ \omega & = & \frac{2\beta_n v_0}{r(\beta_n^2+1)},\\ \theta & = & \frac{\beta_n v_0}{r(\beta_n^2+1)}\left[\frac{-\pi}{\omega_n} + 2t\right] + \theta_0\label{e12} \end{eqnarray} \subsection{Velocity of Tail at Impact} The vertical velocity at the tail of the body $v_t$ is related to the vertical velocity and angular velocity at the nose by \begin{equation} v_t = v_n + \omega(l_n + l_t)\cos\theta \end{equation} where $v_n = \dot y_n$. Substituting Equations~\eref{eq:vl} and~\eref{eq:omega} into the above equation and assuming that $\cos\theta\approx 1$, the ratio of the velocity at the tail to the initial vertical velocity is: \begin{equation} \frac{v_t}{v_0} = \cos\omega_nt - \frac{\beta_n(\beta_n+\beta_t)} {(1+\beta_n^2)}\left[\cos\omega_n t-1\right]\label{eq:vrv0t} \end{equation} where $\beta_t$ is defined to be $l_t/r$. This ratio is maximized at time $t = \pi/\omega_n$ and gives a maximum velocity ratio of \begin{equation} \frac{v_t}{v_0} = \frac{2\beta_n(\beta_n+\beta_t)}{1+\beta_n^2} - 1 \label{eq:vrv0} \end{equation} This result indicates that if linear elastic response is assumed, the magnitude of the slapdown velocity of the body can be estimated using only geometric and mass quantities; the force-displacement behavior of the body is not needed. Furthermore, Equation~\eref{eq:vrv0} can be used to show that \begin{equation} {\rm If} \quad\beta_n\beta_t \leq1, \quad{\rm then} \quad\frac{v_t}{v_0} \leq1\label{eq:blbr} \end{equation} \subsection{Effect of Inelastic Force-Displacement Behavior} The results in the previous section were derived assuming a linear elastic force-displacement behavior. In general, the force-displacement behavior is inelastic and energy is dissipated by plastic deformation. In this section it will be shown that when energy is dissipated by plastic deformation, the slapdown velocity ratio is closer to unity than if there is no energy dissipation. In this derivation, the springs are assumed to have an infinite unloading modulus which means that all of the internal energy in the spring is dissipated. Equations \eref{e1} through~\eref{etheta} are still valid, except that the time interval is reduced to ($0\leq t\leq \pi / 2\omega_n$). If the tail impacts the rigid surface at time $t=\pi/2\omega_n$, then Equation~\eref{eq:vrv0t} gives the following expression for the maximum inelastic velocity ratio: \begin{equation} \frac{v_t}{v_0} = \frac{\beta_n(\beta_n+\beta_t)}{1+\beta_n^2} \label{eq:vrv0i} \end{equation} which can be written as: \begin{equation} \left(\frac{v_t}{v_0}\right)_\infty = \left(\frac{v_t}{v_0}\right)_E + \left(\frac{1-\beta_n\beta_t}{1+\beta_n^2}\right)\label{eisum} \end{equation} where the subscripts $(\ )_\infty$ and $(\ )_E$ denote infinite unloading modulus and elastic unloading modulus, respectively. The last term on the right-hand-side is greater than zero if $\beta_n\beta_t\leq1$ and is less than zero if $\beta_n\beta_t\geq1$. Therefore, an infinite unloading modulus results in a tip velocity ratio that is closer to unity than the velocity ratio calculated assuming linear elastic impact behavior. These two cases bound the possible unloading behavior of all bodies, therefore \begin{displaymath} \begin{array}{cccc} {\rm If\;} & \left\{\begin{array}{rcl} \beta_n\beta_t & \leq & 1\\ {} & {} & {}\\ \beta_n\beta_t & \geq & 1 \end{array}\right\}, & {\quad\rm then\quad} & \left\{\begin{array}{rclcl} \left[\frac{v_t}{v_0}\right]_E & \leq & \left[\frac{v_t}{v_0}\right]_I & \leq & 1\\ {} & {} & {} & {} & {}\\ \left[\frac{v_t}{v_0}\right]_E & \geq & \left[\frac{v_t}{v_0}\right]_I & \geq & 1 \end{array}\right\} \end{array} \end{displaymath} where the subscripts $(\ )_E$ and $(\ )_I$ refer to the elastic and inelastic responses, respectively. The above results have been verified using the \SLAP\ program. Note that although the velocity ratio for the inelastic case increases when $\beta_n\beta_t \leq 1$, it does not increase to greater than unity. If the body is symmetric, then $\beta_n = \beta_t$ and this result states that there will be no slapdown if $L/r < 2$. \section{Conclusions} An equation has been derived which gives a conservative estimate of the velocity ratio for slapdown of a body impacting a rigid surface. Only easily obtainable geometric and mass quantities are required. This equation can be used during the design process to help determine a body geometry which will minimize the slapdown potential. Equation~\eref{e12} can be used to determine the minimum initial drop angle $\theta_0$ such that the secondary impact occurs at the same time or after the initial impact point has rebounded from the rigid surface. This angle is important for three-dimensional finite element analyses of the slapdown event. The drop angle is given by \begin{equation} \theta_0 = \frac{\beta_n v_0\pi}{r(\beta_n^2+1)\omega_n} \end{equation} This angle is measured counter-clockwise from the horizontal and assumes that the body has the same radius at the initial and secondary impact points. If the body is not symmetric, the angle $\tan^{-1}\left(\frac{R_n-R_t}{l_n+l_t}\right)$ must be subtracted from the initial angle $\theta_0$ to account for the asymmetric geometry. $R_n$ and $R_t$ are the radii at the nose and tail of the body, respectively, and the radius is defined as the perpendicular distance from the longitudinal axis of the body to the impact point.