1/2 pound of TNT
released in ~ 10 µs
250 food calories
released in ~ 1000 s
NIF fusion ignition capsule
released in ~ 0.1 ns
SLS engines ~100 GW at launch
NIF ignition shot ~500 TW
Ignition target before its cryogenic shroud closes. It takes a day or two to grow the solid hydrogen fuel layer inside the capsule before it can be shot.
A bare cryogenic hohlraum target. The silicon arms conduct heat away so the capsule inside can be cooled below 20 K to freeze a layer of DT fuel inside the capsule.
Hohlraum filled with low pressure helium tamping gas held in by LEH windows.
HDC (aka diamond) ignition capsule. The barely visible hair at the top is the hollow glass tube used to fill the capsule with deuterium-tritium fusion fuel.
Cryogenic hohlraum. Wires are for temperature sensors and the heater coils (black bands above and below center) needed to grow a spherical hydrogen ice layer inside the capsule.
Target before a shot with shroud slightly open. Note copper tube and block holding slicon arms.
After a shot with shroud fully retracted. The copper tube split open and folded back around the base of the target positioner. Note the wires dangling from the block that held the silicon arms.
Using simulations to compare two different hohlraum designs.
The "hohlraum" is the hollow gold case containing the capsule - in simple terms it is a 1 cm tall oven. The laser beams enter the top and bottom of the hohlraum through laser entrance holes (LEH), heating the interior to $3\times 10^6$ K in under 10 ns. This causes the outer layers of the capsule to explode, imploding the fuel inside it.
Higher resolution simulations of the capsule only guide interpretations of what instruments record during an actual experiment. There are too many unknowns for these models to actually describe a real implosion, but without them we would have no idea what we were looking at.
X-ray framing cameras make movies of NIF implosions - like the core of an imploded ignition capsule near "bang time" (BT) below.
Dozens of diagnostic instruments measure light, X-rays, neutrons, and other products from each target shot.
Fusion reactivities versus temperature
D = deuterium (²H), T = tritium (³H), n = neutron
Temperature scale: 1 keV = 11,600,000 K
Temperature at core of Sun is 1.3 keV (surface 0.5 eV)
None of these reactions power the Sun! The fusion reactions in the Sun must be far slower than any of these!
Extracting deuterium from seawater is extremely expensive. Tritium comes from lithium which must be mined to provide the other half of DT fusion fuel.