At the altitude that the balloon will reach it will be bobbing around in the stratosphere – a layer of the atmosphere between 20km and 50km above the Earth’s surface which comes with some unusual features. It has been found that certain species of bacteria call the stratosphere home, as does the odd massively ambitious bird. The stratosphere also has a funky temperature profile – it actually gets warmer the higher up through the stratosphere you go.
This counter-intuitive temperature situation is down to the way the gases in the stratosphere interact with radiation. Ozone (O3) in the high stratosphere absorbs most of the sun’s high energy ultraviolet (UV) radiation with wavelengths between 100 and 315nm – UVB and UVC for the SPF-savvy among us. This has the effect of protecting life on Earth from some nasty mutagenesis caused by the UVB and UVC interacting with DNA, leading to all sorts of cancery havoc. In the process, the UV breaks down the O3 into a pair of oxygens, i.e. bog-standard molecular oxygen (O2), and a singular oxygen atom (O1).
Further down the stratosphere, once the UVB and UVC have been absorbed, the O2 and O1 can recombine to form O3 again and this process generates heat. Below this level the stratosphere receives very little UVB and UVC so the O3 remains intact and since there’s no O2 and O1 combining then no additional heat is generated. Overall this means the stratosphere starts off at the bottom a seriously chilly -60oC and by the time you get to the top the temperature has reached almost 0oC. Toasty.
So travelling up through the stratosphere means that our payload will experience increasing amounts of UV radiation. In addition it will experience more of other sorts of radiation as the amount of shielding provided by the atmosphere decreases. Cosmic rays are a type of radiation made of particles, their origin unknown. These particles play in the atmosphere and interact with the particles there, creating all sorts of secondary particles. Some of these eventually reach the ground and give us all a dose of radiation.
People who work in environments where their exposure to radiation could be higher than normal (such as in hospitals, nuclear power stations and aircraft) can wear badges, called film badge dosimeters, that record exposure to this kind of radiation by examining the changes to photographic film in the badge. The photographic film changes when hit by radiation, so when the film is developed it is possible to see how much radiation the badge (and therefore the wearer of the badge) has been exposed to.
We will use a similar process to record the balloon and payload’s exposure to radiation. We’ll send up some photographic film in a bag that will stop light getting to the film but that won’t stop the cosmic rays or it’s secondary particles. We’ll cover part of the film with a message written in lead. The lead will prevent the film underneath it from being exposed by the cosmic rays, and this will create a pattern on the film which will be revealed when it is developed into a photograph. Cosmic!




































