I'm still going to assume that the rain is falling at a constant rate. Furthermore, I'm going to assume that the angle of the rain doesn't change. With those two assumptions stated, let me remind you of the definitions we used last time.

\[\rho - \text{the density of water in the air in liters per cubic meter}\]

\[A_t - \text{top area of a person}\]

\[\Delta t - \text{time elapsed}\]

\[d - \text{distance we have to travel in the rain}\]

\[v_r - \text{raindrop velocity}\]

\[A_f - \text{front area of a person}\]

\[W_{tot} - \text{total amount of water in liters we get hit with}\]

As a reminder, our result from last time was:

\[W_{tot}= \rho d (A_t \frac{v_r}{v} + A_f)\]

Now, let's look at the new analysis. As before, let us consider the stationary state first. Our velocity now has two components, horizontal and vertical. Analogous to the purely vertical situation, we can write down the stationary state, but now we have rain hitting both our top and front (or back). I'm going to define the angle, theta, as the angle the rain makes with the vertical (check out figure 1 below). this gives

\[W = \rho d A_t v_r \cos(\theta) \Delta t+\rho A_f v_r \sin(\theta) \Delta t\]

Let's check our limits. As theta goes to zero (vertical rain), we only get rain on top of us, and as theta goes to 90 (horizontal rain), we only get rain on the front of us. Makes sense! Alright, so let's add in the effect of motion now. This is going to be more challenging than in the vertical rain situation. We're going to examine two separate cases

Fig. 1 - The rain, and our angle. |

__Case 1: Running Against The Rain__This is the easier of the two cases. After thinking about it for a while, I believe that it is the same as when the rain is vertical. Let me explain why. If you are moving with some velocity v, in a time t you will cover a distance x=v*t. Now, suppose we paused the rain, so it is no longer moving, then moved you a distance x, turned the rain back on, and had you wait for a time t. And repeated this over and over until you got to where you were going. This would result in an

*average*velocity equal to v, even though it is not a smooth motion. However, my claim is that in the limit that t and x go to zero, this is a productive way of considering our situation. We note that v=x/t, and in the limit that both x and t go to zero, that is the

*definition*of instantaneous velocity. The recap is, that my 'pausing the rain' scheme of thinking about things is fine, as long as we consider moving ourselves only very small distances over very short times. Using this construction, we have an additional amount of rain absorbed by moving the distance delta x of:

\[ \Delta W = \rho A_f \Delta x \]

\[ \Delta W = \rho A_f v \Delta t \]

This gives a net expression of

\[\Delta W = \rho A_t v_r \cos(\theta) \Delta t+\rho A_f v_r \sin(\theta) \Delta t+\rho A_f v \Delta t \]

\[\Delta W = \rho A_f v \Delta t \left( \left( \frac{A_t}{A_f}\right) \left(\frac{v_r}{v}\right)\cos(\theta)+\left(\frac{v_r}{v}\right)\sin(\theta) + 1 \right)\]

As before, turning the deltas into differentials and integrating yields

\[W = \rho A_f v t \left( \left( \frac{A_t}{A_f} \right) \left(\frac{v_r}{v}\right)\cos(\theta)+\left(\frac{v_r}{v}\right)\sin(\theta) + 1\right)\]

\[W=\rho A_f d \left( \left( \frac{A_t}{A_f}\right) \left(\frac{v_r}{v}\right)\cos(\theta)+ \left(\frac{v_r}{v}\right)\sin(\theta) + 1 \right)\]

Note that when theta is zero, our vertical rain result gives the same thing as we found in the last post (the first term lives, the second term goes to zero, the third term lives). I'm going to use the reasonable numbers I came up with in the last post. However, since we have wind, we'll have to modify our rain velocity. More specifically, we'll assume the rain has the same vertical component of velocity in all cases. Then the wind speed, v_w, will be what controls the angle. More exactly, the magnitude of the raindrop velocity will be

\[v_r=\sqrt{(6 m/s)^2+v_w^2}\]

While the angle will be

\[\theta=\tan^{-1}(v_w/ (6 m/s))\]

Next we note that

\[v_r\cos\theta = 6 m/s\]

which is just the vertical component of our rain. Similarly, the other term is just the horizontal component of our rain. So we can write our as a function of our velocity and the wind speed (the angle and wind speed is interchangeable):

\[W = \rho A_f d\left( \left( \frac{A_t}{A_f}\right) \left(\frac{6 m/s}{v}\right) +\left(\frac{v_w}{v}\right) + 1\right)\]

Using the reasonable numbers I came up with in my last post yields (with a distance of 100m)

\[W = .2 liters \left( \left(\frac{.72 m/s}{v}\right)&+\left(\frac{v_w}{v}\right) + 1\right)\]

Once again, we have a least wet asymptote, which is the same as before. I've plotted this function for various values of theta, and, more intuitively, for various wind speeds (measured in mph, as we're used to here in the US), and the plots are shown below (click to enlarge). Unsurprisingly, you get the most wet when the rain is near horizontal, but interestingly enough you can get the most percentage change from a walk to a run when the rain is near horizontal. All angles are in degrees.

Fig. 3 - How wet you get vs. how fast you run for various wind speeds in mph. |

__Case 2: Running With The Rain__This is the potentially harder case. We've got two obvious limiting cases. If you run with the exact velocity of the rain and the rain is horizontal, you shouldn't get wet. If the rain is vertical, it should reduce to the result from my first post. We'll start with the stationary case. This should be identical to case 1, if you're stationary it doesn't matter if the rain is blowing on your front or back. That means that for v=0, we should have

\[\Delta W = \rho A_t v_r \cos(\theta) \Delta t + \rho A_f v_r \sin(\theta) \Delta t\]

Now, let's use the same method as before, pausing the rain, advancing in x, then letting time run. First we'll deal with our front side. Consider figure 4.

Note that in front of us there is a rainless area, which we'll be advancing into. Consider a delta x less than the length of the base of that triangle. If we advance that delta x, we'll carve out a triangle of rain as indicated, which, by some simple geometry, contains an amount of rain

\[\rho w \frac{(\Delta x)^2}{2 \tan(\theta)} = \rho w \frac{v^2 (\Delta t)^2}{2 \tan(\theta)}\]

where w is the width of our front. Now, consider if delta x is longer than the base of the rainless triangle, as shown in figure 5.

We'll carve out an amount of rain equal to the indicated triangle plus the rectangle. From the diagram we see this gives an amount of water

\[A_f \rho (\Delta x - h \tan(\theta)) + A_f \rho h \tan(\theta)/2 = A_f \rho (\Delta x - \frac{h \tan(\theta)}{2})\]

We could write two separate equations for these two cases, but that's rather inefficient notation. I'm going to use the Heaviside step function, H(x). This is a function that is zero whenever the argument is negative, and 1 whenever the argument is positive. That means that for our front side,

\[\Delta W_f=\rho w \frac{v^2 (\Delta t)^2}{2 \tan(\theta)} H( h\tan(\theta) - \Delta x) \]

\[+A_f \rho \left(\Delta x - \frac{h \tan(\theta)}{2}\right)H(\Delta x - h \tan(\theta))\]

Note that I've written my step function in terms of the relative length of delta x and the base of the rainless triangle. We get the first term when delta x is less than the base length, and the second term when delta x is more than the base length.

Now, let us consider the rain hitting our back. There are two cases here as well. First consider the case where we're running with a velocity less than that of the rain. See figure 6..

We get two terms. There's the triangle of rain that moves down and hits our back, shown above. Hopefully it is apparent that this is the same as the triangle of rain we carved out with our front, and so will contribute a volume of water

\[\rho w \frac{v^2 (\Delta t)^2}{2 \tan(\theta)}\]

There's also the rain that manages to catch up with us,

\[A_f \rho (v_r \sin(\theta) \Delta t - \Delta x) =A_f \rho \Delta t (v_r \sin(\theta) - v)\]

In the case where we outrun the rain, we don't want this term, and our triangle gains a maximal length of the horizontal and vertical components of the rain velocity times delta t. We can write this backside term using a step function as

\[\Delta W_b =A_f \rho \Delta t \left(v_r \sin(\theta) - v +w \frac{v^2 (\Delta t)^2}{2 \tan(\theta)}\right)H( v_r \sin(\theta) - v)\]

\[+\rho w v_r^2 \Delta t^2 \frac{\sin(\theta)\cos(\theta)}{2} H(v-v_r\sin(\theta))\]

We can combine these terms, with our usual top term, to get

\[\Delta W =A_f \rho \Delta t \left[ \left(v_r \sin(\theta) - v +\frac{w}{A_f} \frac{v^2 (\Delta t)}{2 \tan(\theta)}\right)H(v_r \sin(\theta) - v)\]

\[+ \frac{w}{A_f} v_r^2 \Delta t \frac{\sin(\theta)\cos(\theta)}{2} H(v-v_r\sin(\theta) \]

\[+ \frac{w}{A_f} \frac{v^2 (\Delta t)}{2 \tan(\theta)} H( h\tan(\theta) - \Delta x)\]

\[+\left(\frac{\Delta x}{\Delta t} - \frac{h \tan(\theta)}{2 \Delta t}\right)H(\Delta x - h \tan(\theta))+\frac{A_t}{A_f} v_r \cos(\theta) ] \]

I'm sure this four line equation looks intimidating (I'm also sure that it is the longest equation we've written here on the virtuosi!). But it'll simplify when we take our limit as delta t goes to zero. Let's do this a little more carefully than usual.

\[\lim_{\Delta t \to 0}\frac{\Delta W}{\Delta t} =\lim_{\Delta t \to 0}A_f \rho \left[ \left(v_r \sin(\theta) - v +\frac{w}{A_f} \frac{v^2 (\Delta t)}{2 \tan(\theta)}\right)\]

\[*H(v_r \sin(\theta) - v)+ \frac{w}{A_f} v_r^2 \Delta t \frac{\sin(\theta)\cos(\theta)}{2} H(v-v_r\sin(\theta) \]

\[+ \frac{w}{A_f} \frac{v^2 (\Delta t)}{2 \tan(\theta)} H( h\tan(\theta) - v \Delta t)\]

\[+\left(v - \frac{h \tan(\theta)}{2 \Delta t}\right)H(v \Delta t - h \tan(\theta))+\frac{A_t}{A_f} v_r \cos(\theta) ] \]

We'll take this term by term. On the left side of our equality, we recognize the definition of a differential of W with respect to t. Any term on the right without a delta t we can ignore. The first term with a delta t is

\[\frac{w}{A_f} \frac{v^2 (\Delta t)}{2 \tan(\theta)}H(v_r \sin(\theta) - v)\]

In all cases except when theta = 0, this term goes to zero. Now, when theta = 0, tan(theta) = 0, so our limit gives zero over zero, which is a number (note, I'm not being extremely careful. If you'd like, tangent goes as the argument to leading order, so we have two things going to zero linearly, hence getting a number back out). However, looking at the step function, when theta goes to zero, we likewise require v to be zero to get a value. However, our term goes as v^2, so we conclude that in our limit, this term goes to zero. Next we have

\[\frac{w}{A_f} v_r^2 \Delta t \frac{\sin(\theta)\cos(\theta)}{2} H(v-v_r\sin(\theta)\]

This obviously goes to zero, no mitigating circumstances like a division by zero. The next term is

\[\frac{w}{A_f} \frac{v^2 (\Delta t)}{2 \tan(\theta)} H( h\tan(\theta) - v \Delta t)\]

This term presents the same theta = 0 issues as the first term. The resolution is slightly more subtle and less mathematical than before. Remember that this term physically represents the rain that hits us when we move forward through the section that our body hasn't shielded from the rain (see the drawing above). I argue from a physical standpoint that when the rain is vertical, this term would double count the rain we absorb with the next term (which doesn't go to zero). I'm going to send this term to zero on physical principles, even though the mathematics are not explicit about what should happen. Next we have

\[vH(v \Delta t - h \tan(\theta))\]

The argument of the step function makes it clear that to have any chance at a non-zero value we need theta = 0. The mathematics isn't completely clear here, as the value of a step function at zero is usually a matter of convention (typically .5). Let's think physically about what this term represents. This is the rain we absorb beyond the shielded region (see above figure). This is the term I said the previous term would double count with when the rain is vertical, so we're required to keep it. However, only when theta = 0. I'm going to use another special function to write that mathematically, the Kronecker delta, which is 1 when the subscript is zero, and zero otherwise. This is a bit of an odd use of the Kronecker delta, because it's typically only used for integers, but for those purists out there, there is an integral definition which has the same properties for any (non-integer) value. Thus

\[vH(v \Delta t - h \tan(\theta))=v\delta_{\theta}\]

The last term we have to concern ourselves with is

\[- \frac{h \tan(\theta)}{2 \Delta t}H(v \Delta t - h \tan(\theta))\]

Again, there is some mathematical confusion when theta = 0, so we think physically again. This term represents the rain in the unblocked triangle (see above). Obviously, there is no rain in the triangle when theta is zero, because there is no triangle! We set this term to zero as well. This gives us a much simler expression than before,

\[\Delta W = \rho A_t v_r \cos(\theta) \Delta t + \rho A_f v_r \sin(\theta) \Delta t\]

Now, let's use the same method as before, pausing the rain, advancing in x, then letting time run. First we'll deal with our front side. Consider figure 4.

Fig. 4 - Geometry for small delta x. |

Note that in front of us there is a rainless area, which we'll be advancing into. Consider a delta x less than the length of the base of that triangle. If we advance that delta x, we'll carve out a triangle of rain as indicated, which, by some simple geometry, contains an amount of rain

\[\rho w \frac{(\Delta x)^2}{2 \tan(\theta)} = \rho w \frac{v^2 (\Delta t)^2}{2 \tan(\theta)}\]

where w is the width of our front. Now, consider if delta x is longer than the base of the rainless triangle, as shown in figure 5.

Fig. 5 - Geometry for large delta x. |

We'll carve out an amount of rain equal to the indicated triangle plus the rectangle. From the diagram we see this gives an amount of water

\[A_f \rho (\Delta x - h \tan(\theta)) + A_f \rho h \tan(\theta)/2 = A_f \rho (\Delta x - \frac{h \tan(\theta)}{2})\]

We could write two separate equations for these two cases, but that's rather inefficient notation. I'm going to use the Heaviside step function, H(x). This is a function that is zero whenever the argument is negative, and 1 whenever the argument is positive. That means that for our front side,

\[\Delta W_f=\rho w \frac{v^2 (\Delta t)^2}{2 \tan(\theta)} H( h\tan(\theta) - \Delta x) \]

\[+A_f \rho \left(\Delta x - \frac{h \tan(\theta)}{2}\right)H(\Delta x - h \tan(\theta))\]

Note that I've written my step function in terms of the relative length of delta x and the base of the rainless triangle. We get the first term when delta x is less than the base length, and the second term when delta x is more than the base length.

Now, let us consider the rain hitting our back. There are two cases here as well. First consider the case where we're running with a velocity less than that of the rain. See figure 6..

Fig. 6 - The back. |

We get two terms. There's the triangle of rain that moves down and hits our back, shown above. Hopefully it is apparent that this is the same as the triangle of rain we carved out with our front, and so will contribute a volume of water

\[\rho w \frac{v^2 (\Delta t)^2}{2 \tan(\theta)}\]

There's also the rain that manages to catch up with us,

\[A_f \rho (v_r \sin(\theta) \Delta t - \Delta x) =A_f \rho \Delta t (v_r \sin(\theta) - v)\]

In the case where we outrun the rain, we don't want this term, and our triangle gains a maximal length of the horizontal and vertical components of the rain velocity times delta t. We can write this backside term using a step function as

\[\Delta W_b =A_f \rho \Delta t \left(v_r \sin(\theta) - v +w \frac{v^2 (\Delta t)^2}{2 \tan(\theta)}\right)H( v_r \sin(\theta) - v)\]

\[+\rho w v_r^2 \Delta t^2 \frac{\sin(\theta)\cos(\theta)}{2} H(v-v_r\sin(\theta))\]

We can combine these terms, with our usual top term, to get

\[\Delta W =A_f \rho \Delta t \left[ \left(v_r \sin(\theta) - v +\frac{w}{A_f} \frac{v^2 (\Delta t)}{2 \tan(\theta)}\right)H(v_r \sin(\theta) - v)\]

\[+ \frac{w}{A_f} v_r^2 \Delta t \frac{\sin(\theta)\cos(\theta)}{2} H(v-v_r\sin(\theta) \]

\[+ \frac{w}{A_f} \frac{v^2 (\Delta t)}{2 \tan(\theta)} H( h\tan(\theta) - \Delta x)\]

\[+\left(\frac{\Delta x}{\Delta t} - \frac{h \tan(\theta)}{2 \Delta t}\right)H(\Delta x - h \tan(\theta))+\frac{A_t}{A_f} v_r \cos(\theta) ] \]

I'm sure this four line equation looks intimidating (I'm also sure that it is the longest equation we've written here on the virtuosi!). But it'll simplify when we take our limit as delta t goes to zero. Let's do this a little more carefully than usual.

\[\lim_{\Delta t \to 0}\frac{\Delta W}{\Delta t} =\lim_{\Delta t \to 0}A_f \rho \left[ \left(v_r \sin(\theta) - v +\frac{w}{A_f} \frac{v^2 (\Delta t)}{2 \tan(\theta)}\right)\]

\[*H(v_r \sin(\theta) - v)+ \frac{w}{A_f} v_r^2 \Delta t \frac{\sin(\theta)\cos(\theta)}{2} H(v-v_r\sin(\theta) \]

\[+ \frac{w}{A_f} \frac{v^2 (\Delta t)}{2 \tan(\theta)} H( h\tan(\theta) - v \Delta t)\]

\[+\left(v - \frac{h \tan(\theta)}{2 \Delta t}\right)H(v \Delta t - h \tan(\theta))+\frac{A_t}{A_f} v_r \cos(\theta) ] \]

We'll take this term by term. On the left side of our equality, we recognize the definition of a differential of W with respect to t. Any term on the right without a delta t we can ignore. The first term with a delta t is

\[\frac{w}{A_f} \frac{v^2 (\Delta t)}{2 \tan(\theta)}H(v_r \sin(\theta) - v)\]

In all cases except when theta = 0, this term goes to zero. Now, when theta = 0, tan(theta) = 0, so our limit gives zero over zero, which is a number (note, I'm not being extremely careful. If you'd like, tangent goes as the argument to leading order, so we have two things going to zero linearly, hence getting a number back out). However, looking at the step function, when theta goes to zero, we likewise require v to be zero to get a value. However, our term goes as v^2, so we conclude that in our limit, this term goes to zero. Next we have

\[\frac{w}{A_f} v_r^2 \Delta t \frac{\sin(\theta)\cos(\theta)}{2} H(v-v_r\sin(\theta)\]

This obviously goes to zero, no mitigating circumstances like a division by zero. The next term is

\[\frac{w}{A_f} \frac{v^2 (\Delta t)}{2 \tan(\theta)} H( h\tan(\theta) - v \Delta t)\]

This term presents the same theta = 0 issues as the first term. The resolution is slightly more subtle and less mathematical than before. Remember that this term physically represents the rain that hits us when we move forward through the section that our body hasn't shielded from the rain (see the drawing above). I argue from a physical standpoint that when the rain is vertical, this term would double count the rain we absorb with the next term (which doesn't go to zero). I'm going to send this term to zero on physical principles, even though the mathematics are not explicit about what should happen. Next we have

\[vH(v \Delta t - h \tan(\theta))\]

The argument of the step function makes it clear that to have any chance at a non-zero value we need theta = 0. The mathematics isn't completely clear here, as the value of a step function at zero is usually a matter of convention (typically .5). Let's think physically about what this term represents. This is the rain we absorb beyond the shielded region (see above figure). This is the term I said the previous term would double count with when the rain is vertical, so we're required to keep it. However, only when theta = 0. I'm going to use another special function to write that mathematically, the Kronecker delta, which is 1 when the subscript is zero, and zero otherwise. This is a bit of an odd use of the Kronecker delta, because it's typically only used for integers, but for those purists out there, there is an integral definition which has the same properties for any (non-integer) value. Thus

\[vH(v \Delta t - h \tan(\theta))=v\delta_{\theta}\]

The last term we have to concern ourselves with is

\[- \frac{h \tan(\theta)}{2 \Delta t}H(v \Delta t - h \tan(\theta))\]

Again, there is some mathematical confusion when theta = 0, so we think physically again. This term represents the rain in the unblocked triangle (see above). Obviously, there is no rain in the triangle when theta is zero, because there is no triangle! We set this term to zero as well. This gives us a much simler expression than before,

\[\frac{dW}{dt} =A_f \rho \left[ (v_r \sin(\theta) - v)H(v_r \sin(\theta) - v)+v\delta_{\theta}+\frac{A_t}{A_f} v_r \cos(\theta) \right]\]

We can pull out a v and integrate with respect to t, giving

\[W=A_f \rho v t \left[ (\frac{v_r \sin(\theta)}{v} - 1)H(v_r \sin(\theta) - v)+\delta_{\theta}+\frac{A_t}{A_f} \frac{v_r \cos(\theta)}{v} \right]\]

As before, we can write this in terms of the wind velocity and the vertical rain velocity,

\[W=A_f \rho d \left[ (\frac{v_w}{v} - 1)H(v_w - v)+\delta_{v_w}+\frac{A_t}{A_f} \frac{v_{r,vert}}{v} \right]\]

This is a nice, simple expression that we can easily plot. There is one thing that bothers me, I feel like there should be another step function term that kicks in when your velocity exceeds the horizontal rain velocity, and you start getting more rain on your front. But I'm going to trust my analysis, and assert that such a term would be at least second order in our work. If someone does find it, let me know! Using the reasonable numbers from my last post gives

\[W=.2 liters \left[ (\frac{v_w}{v} - 1)H(v_w - v)+\delta_{v_w}+\frac{.72 m/s}{v} \right]\]

Because this post is long enough already, I've gone ahead and plotted this only vs. wind velocity. I've also plotted the former least wet asymptote. Most interesting (and you'll probably have to click on the graph to enlarge to see this) is that there no longer is a least wet asymptote! In theory if you run fast enough you can stay as dry as you want.

This is a nice, simple expression that we can easily plot. There is one thing that bothers me, I feel like there should be another step function term that kicks in when your velocity exceeds the horizontal rain velocity, and you start getting more rain on your front. But I'm going to trust my analysis, and assert that such a term would be at least second order in our work. If someone does find it, let me know! Using the reasonable numbers from my last post gives

\[W=.2 liters \left[ (\frac{v_w}{v} - 1)H(v_w - v)+\delta_{v_w}+\frac{.72 m/s}{v} \right]\]

Because this post is long enough already, I've gone ahead and plotted this only vs. wind velocity. I've also plotted the former least wet asymptote. Most interesting (and you'll probably have to click on the graph to enlarge to see this) is that there no longer is a least wet asymptote! In theory if you run fast enough you can stay as dry as you want.

Fig. 6 - How wet you get vs. how fast you run for various wind speeds in mph. |

__Comparison__I will conclude with a comparison of the two results, to each other and to the vertical case. First, lets take the appropriate limits.

\[W_{with}=A_f \rho d \left[ (\frac{v_w}{v} - 1)H(v_w - v)+\delta_{v_w}+\frac{A_t}{A_f} \frac{v_{r,vert}}{v} \right]\]

\[W_{against} = \rho A_f d\left( \left( \frac{A_t}{A_f}\right) \left(\frac{v_{r,vert}}{v}\right) +\left(\frac{v_w}{v}\right) + 1\right)\]

\[W_{stationary} = \rho t A_f \left(\frac{A_t}{A_f} v_{r,vert}+v_w\right)\]

\[W_{vert}= \rho d A_f \left(\frac{A_t}{A_f} \frac{v_r}{v} + 1 \right)\]

In the stationary limit, we have to break up the d in our equations into v t, and that gives

\[\lim_{v \to 0}W_{with}= \lim_{v \to 0} W_{against}=\rho t A_f \left(\frac{A_t}{A_f} v_{r_vert}+v_w\right)\]

While in the vertical rain limit

\[\lim_{v_w \to 0}W_{with}= \lim_{v_w \to 0} W_{against} =\rho d A_f \left(\frac{A_t}{A_f} \frac{v_r}{v} + 1 \right)\]

So our limits work. Finally, it's a little hard to tell the difference between the forward and backwards case, so I've plotted the two lines together for a few values of v_w. You'll notice that for zero wind speed they have the same result (which is good, since our limit was the same), but for the other wind speeds they are remarkably divergent, more so as you run faster! (again, click to enlarge)

Fig. 7 - Solid lines are running with the rain, dashed lines are running against the rain. |

__Conclusions__Hopefully this has been an interesting exercise for you. I know it certainly took me longer to work and write than I initially thought. While you can't see it in the post, there were a lot of scribblings and thinking going on before I came to these conclusions. Most of it went something like: "No, that can't be right, it doesn't have the right (zero velocity/zero angle) limit!". I think this concludes all of the running in the rain that I want to do, but if you have more followup questions, post them below, and I'll do my best to answer. Also, I admit that my analysis may be a bit rough, so if you have other approaches, let me know. Finally, note that everything I've found favors running in the rain, so get yourself some exercise and stay dry!

It seems like if you run extremely fast, it appears as if the rain drops are stationary in the air. So I would guess that you'd still encounter the same volume of water droplets in your path as you spoke about in your first post.

ReplyDeleteI couldn't make out the scales in your graphs, does it show that you would stay virtually dry while running very fast?

"There is one thing that bothers me, I feel like there should be another step function term that kicks in when your velocity exceeds the horizontal rain velocity, and you start getting more rain on your front."

ReplyDeleteBohn's right about running really fast, and it seems if you are missing a term that took into account what you said in the quote above, you would get a result that showed arbitrary dryness. That is, I think your model allows you to run as fast as you like away from the rain, without ever running into the droplets in front of you. See Bohn's other comment for what I believe to be the correct model.

What if you considered running at a certain velocity w, and with the rain at a velocity v angle theta measured from the +y axis.

ReplyDeleteThe rain velocity would look like

v_x = v*sin(theta)

v_y = v*cos(theta)

but if we transform our system by a velocity w (non-relativistically please), we get

v_x = v*sin(theta) - w

v_y = v*cos(theta)

We can split up the head and body terms to find the total volume of rain using flux*area*time.

The time should be t = d / w, where d is the distance traveled.

Let p be the density of water droplets in the air.

So our final wetness expression should look like:

Volume = p*distance*[ A_head * |v * cos(theta) / w| + A_body*|(v * sin(theta) / w) - 1| ]

The absolute values are because we don't care about negative or positive fluxes, just the magnitude.

This gives the correct limits for theta = 0, 90, -90, as well as the limit where horizontal rain velocity is equal to the running velocity.

Bohn,

ReplyDeleteAs for the graphs, just click on them. You'll get the big version. Should be more than possible to see the scale.

As for the velocity transform . . . I like it. I remember thinking about it a while back, but for some reason seem to have rejected it as an approach. Maybe I'm masochistic and like a lot of math. Or maybe I forgot in the intervening month. If I remember why (if) I rejected it, I'll let you know.

Also, I think you can use tex in your comments, which would make it easier to read.

Clara,

As you say, there's something intuitively wrong with the solution I came up with. Good call!

A bit of an echo of the other posts: I like Bohn's analysis, and his result seems correct to me.

ReplyDeleteThe result of the original article doesn't make sense to me: I am surprised by the claim that "for the other wind speeds they are remarkably divergent, more so as you run faster!" In the limit that the running velocity is >> the wind velocity, running with and against the wind should return the same answer.

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