Re: 2 more questions
Getting my MS in Nuclear Engineering this spring, thought I'd chime in.
You can use pretty much any material you want to for shielding. For gamma rays (from the nucleus) and x-rays (from the electrons of the atom) you want a "High Z" material - basically Tungsten or some other dense material. For neutrons and charged particles you want to use hydrogen for shielding - which one reason most power reactors use either light or heavy water. Thick shielding is better than thin shielding because of "build-up" flux, basically cascade reactions that happen at the surface being irradiated (thick shields attenuate out the build-up flux).
For shielding bases on other planets 2-3 meters of regolith over the habitat should suffice for all but the most intense solar flares (assuming you are basing on the moon or mars).
For D-3He reactions, keep in mind that you are making some tritium and neutrons in the D-D side reactions at about 1%-0.1% of the total fusion reaction rate, so there is radiation present.
A sufficiently advanced society would probably use 3He-3He fusion exclusively. It produces 2 protons and an atom of regular Helium-4. Proton cycle fusion wouldn't be feasible because it requires a carbon catalyst and produces a lot of gamma radiation, and requires a lot more energy to get going.
Another advantage is that 3He from the solar wind is relatively abundant in the first 3 meters of rocky bodies that have no atmosphere. It is also present in Jupiter and Saturn because their gravitational fields are strong enough to retain helium in the atmosphere.