Sunday, 15 July 2018

A bigger keg stays colder for longer

I spotted this keg of beer at an event at the weekend. What is the advantage of having one large keg versus the same amount in individual bottles? The large amount will have a smaller surface area and since thermal energy crosses the boundary through the surface, it will take longer to get energy in. Also, since energy required is proportional to mass, the larger mass will mean more energy is needed to produce the same temperature rise.

Thursday, 12 July 2018

Heatwave 2: car thermometers

The temperature shown above is quite low but we've been noticing some interesting readings whilst out and about. The main car park in Wigton recorded particularly high temperatures. Concrete has a high specific heat capacity so once it has absorbed thermal energy, it remains hot for a long time, warming the air above it. This was coupled with a metre high wall behind the car park which stopped the breeze shifting the warm air. I have read that the thermometers are placed in different places in different cars. Some are low down in front of the radiator. They can even be in with the wing mirrors. From what I've seen, I would suspect the former for our car.

Wednesday, 11 July 2018

Flow rate: estimating the numbers at the Oxford Race for Life

We were supporting at the Race for Life and were debating the number of participants. I timed a minute and counted the number of rows of runners who went past. Each row was roughly 5 runners wide. About 60 rows went past - so about one per second. That's 300 runners a minute. It went on for 10 minutes which means 3000 runners. The next day the Oxford Mail was saying "more than 2500" so it turned out to be a reasonable method.

Thursday, 5 July 2018

Echo chamber: Carlisle Castle dungeon



It was a lot cooler down in the dungeon. Sound took up to 2 seconds to die away. The reverberation was incredible. Sound must repeatedly bounce from wall to wall with little attenuation each time due to the hard surface. We thought that perhaps the arched roof helped to focus sound waves. I estimated height and width of about 6 m. At 330 m/s the sound would take about 0.02 seconds to go from one side the other so there could be up to 100 reflections before it dies away. I tried humming at different frequencies. There was definitely a resonance at a low frequency. The lowest a human can hear is about 20 Hz. The fundamental mode (1st harmonic) for a 6m chamber would have a wavelength of 12 m. So frequency = wave speed/wavelength = 330/12 = 27.5 Hz. Sounds feasible.

Wednesday, 4 July 2018

Heatwave part 1: railway speed restrictions

We've been enjoying the most amazing spell of weather for the far north of England but trains in the Carlisle area have been experiencing speed restrictions because the line have been warped by the heat. I have always understood that they leave expansion gaps between rails to cope with the expansion of metal in warm weather. This is why trains traditionally go clickety-clack. But it appears that there has been some warping between the joints, hence the speed restrictions. But they have also been painting the rails white in places to reduce the absorption of infra-red from the Sun. I found https://www.networkrail.co.uk/running-the-railway/looking-after-the-railway/delays-explained/buckled-rail/ This suggests that modern rails are made from different bits welded together. I'm wondering if that means the expansions work against each other. Needs some research.

Monday, 2 July 2018

Thinking about the green flash




It has been a brilliant week for sunsets. As light from the Sun passes into and through the atmosphere, it slows down slightly and is bent. This bending depends on the optical density of the air (its refractive index) and varies with the density of the air layers. We could draw a diagram in which light from the Sun was unbent and traveled straight. Then we could work out when it was below the horizon and we could no longer see it. However, because of refraction and the bending, straight line rules don't work and the top of the Sun would still just be visible. This hair-splitting depends on how you choose to define "over the horizon". So in my last picture, I can argue that the Sun is actually over the horizon. At this last point, the refraction splits the light into colours as does a prism. The last colour to be seen should be blue but that is selectively scattered leaving the last colour as a green flash in perfect conditions. I thought I caught a glimpse. I am finding the explanations hard going so expect more when I've done more thinking.

Sunday, 1 July 2018

Melting point of bitumen - road in Wasdale


The asphalt has melted on the roads in Cumbria! It's wonderful that the weather is so hot. They have sent the salt gritters out to spread road stone on the bitumen. Bitumen has a high melting point because it is made of long, heavy molecules. I think that this means that there can be more intermolecular forces to hold the molecules together in a solid formation. More joins to separate means more themral energy needed so higher temperature. The explanations usually focus on higher boiling points. I haven't seen one that explains melting points.