She thinks the intense solar radiation is going to destroy film in a camera! That extra 20% sure does make a difference. If only there was a way to block the intense solar radiation so it doesn't destroy film in a camera we could have had over a hundred years of people being able to use cameras that used film right here on earth!
*Turns f-stop ring one click to the right*
We already discussed ulltraviolet.
@Vixen gave us the irrelevant results of a frantic web search and then declared the subject closed without addressing the rebuttal.
Solar x-rays might possibly be a problem if there had been many. When the sun has certain kinds of events, the result is a massive increase in x-ray radiation. However, there are x-rays and then there are x-rays. Back in the day, we were all warned to take our film out of the carry-on luggage at the airport, lest the x-ray machine fog it. Toward that end, David Percy and a friend who claimed to be a physicist showed that if you put ISO 160 film in an x-ray machine and blasted it with 8 MeV x-rays, it would indeed fog the film. But that begs the question that this is what intensity and energy of x-rays come from the sun. A physicist would have known that, or at least known to go look it up since the study of physics includes understanding that photons come in vastly different energies.
The most energetic solar x-rays during solar events are in the 100 keV range. Most solar x-ray radiation is in the 100 eV to 10 keV range. Energy determines how far into material a particle penetrates and how much damage that particle does when it's absorbed. The
most powerful x-rays from the sun are orders of magnitude less energetic than a diagnostic x-ray and don't bother ISO 160 film.
A physicist would know flux density too. That is, the energy of a single photon is one thing. That's the electron-volt measurement. How many photons of that energy per unit area per unit time you're dealing with is the other prong of the exposure question. Airport x-ray scanners go up to 100 W/m
2. The peak density during an X-class solar flare at Earth-Moon distance is about 10
-3 W/m
2, or around four orders of magnitude less intense than a diagnostic x-ray. So no, I don't trust Percy's "physicist." Even at their worst, solar x-rays aren't enough to penetrate the magazine or fog the film. And the worst didn't happen during the missions.
Gamma energies are naturally much higher. That's what makes them gamma rays. However, the flux density even during an X-class event is again on the order of negative exponents per square meter. And the rub is that the gamma rays we would have to worry about are produced in the atmosphere by the collision of solar protons with air molecules. Paradoxically you're much safer from gamma rays on the lunar surface than you would be in low Earth orbit due to the lack of atmosphere in which to generate gamma rays. Yes, we do use photographic film in dosimeters to detect gamma rays. But they have to be behind several layers of absorptive and attenuative materials in order to catch them.
That's it for the EM spectrum. As for particles—solar electrons and solar protons—we have evidence consistent with heavy particle absorption in the Apollo photography. Modern space imaging gives us many more examples of what that looks like in much more sensitive sensors. We probably don't have any evidence specifically of low-mass particle interaction, such as from electrons, because those would be absorbed in the magazine and lens. The reseau plate was partially silvered and would likely absorb all electrons passing into the lens. There is no reason to suppose they would ever reach the film. This is also true for protons, but to a lesser extent since protons are more massive. But since conspiracy theorists don't understand what a particle interaction with film would look like, they don't know that they're looking right at stuff they say should be there but isn't. You should be looking for dots or short, sharp track lines that preferentially affect the blue-absorbing layers.