Posts in physics
Turbulent flow in hoses
Yet another pump operations/water flow post, sorry folks! If only it weren't so darn interesting...
This is another "Zeph convinces themself that the book is right" post, this time on a statement about laminar versus turbulent flow in hoses:
The pressures in hose are typically high enough to cause turbulent flow.
If you're interested in a demonstration of this, buckle in and come along! If not, might I suggest different reading material?
Hydrant capacity calculations
Yet another post on pump operations, sorry y'all. This one, like a previous post, is me coming to terms with a statement about water flow in a textbook. This time around, I'm looking at how to estimate additional hydrant capacity if you're already flowing some amount of water from your hydrant.
Big picture, I'll do some calculations based on Bernoulli's equation to show how much additional water flow a hydrant can provide, then I'll briefly compare that to two of the three methods discussed in Sykes and Sturtevant's 1999 Fire Apparatus Operator: Pumper textbook.
Ways of viewing pressure
Well, guess who's still making sense of water flow through hose and pumps these days? (Yep, you got it. It's me.)
Today I finally figured out a point of confusion I'd had for weeks around the relationship between pressure and volume of flow out of a nozzle. Turns out the answer has to do with a new-to-me way of viewing pressure that offers some additional tools for reasoning about how water flow works.
Head pressure
Head pressure is the pressure created by a difference in height between where water is coming from and a discharge. It's important for things like how much pressure you'll get from a hydrant or how much pressure you lose if you're pumping up a steep driveway. If you read a textbook, it'll say something like
To convert head in feet to head pressure in psi, divide the number of feet by 2.304.
This is me proving to myself that that works. (Spoiler alert: it does.)
Pumps and suction
I've been slowly learning how to operate the pumps on Mt. Erie's apparatus. A lot of that is hands-on stuff – flip this switch and then pull this lever to accomplish goal xyz. Those details are really important, but for my specific brain, I benefit from understanding the underlying theory too, so I've been reading up a bit and trying to build intuition around some of the fundamentals.
In doing so, I learned something that blew my mind: there is a physical limit to how high up you can possibly suck water, no matter how good your pump is. This is my attempt to explain that in a way that actually builds intuition rather than just memorizing "oh, we can only suction 10 vertical meters in the best case".
Neutrino Astrophysics: PeV-energy neutrinos!
Well, I thought I was done with neutrino astrophysics yesterday, but then I read about the recent discovery of two extremely high-energy neutrinos by the IceCube collaboration.
Neutrino Astrophysics: Outstanding mysteries
As you've probably guessed by now, there's a lot we don't know about neutrinos and how they function in astrophysics. They have a lot of mysteries in store for us. Here are a few:
Neutrino Astrophysics: Cosmic neutrino background
Neutrino Astrophysics: Supernova 1987A
Apart from the neutrinos from the Sun, we can also observe neutrinos from high-energy cosmic events. The best example of this is supernova 1987A, a stellar explosion in the Large Magellanic Cloud, a nearby galaxy, whose light reached us in February of 1987.
Neutrino Astrophysics: Neutrino oscillations
When last we left our heroes, the Sudbury Solar Neutrino Observatory (SNO) had concluded that while predictions for the total flux of neutrinos at the Earth were accurate, only about a third of those that reach us are electron neutrinos. This naturally begs the question: what are the rest of them?
Neutrino Astrophysics: The solar neutrino problem
The neutrino detectors discussed in the last post are all well and good, but there's a bit of a problem, and it's substantial enough to have earned itself a catchy name: the solar neutrino problem.
Neutrino Astrophysics: Detectors
Neutrino detection is a tricky enterprise in the best of cases. Since neutrinos interact only via the weak interaction, their interactions have fantastically low cross-sections, which means that detectors end up seeing only a couple of neutrinos per day in some of the better cases.
Neutrino Astrophysics: Rationale and production
Chaotic Pendulum
This post was originally a paper written with Vivian Steyert for a class, Theoretical Mechanics. In summer 2015 I adapted it for this blog. If you're interested in the original paper (pdf), you can read it here.