1. Fission and Fukushima part 1 Gordon J
Fission and Fukushima part 1 Gordon J. Aubrecht, II SOS/AAPT presentation, 30 April 2011

2. “Fukushima Dai-ichi” Fukushima means “Blessed island” Dai-ichi means No. 1 Dai-ni means No. 2 Dai-san means No. 3 Dai-yon means No. 4 etc.

3. What happened on 11 March? Friday, March 11, 2011 at 05:46:23 UTC Friday, March 11, 2011 at 02:46:23 PM at epicenter at a depth of 32 km The earthquake of magnitude 9 (energy release ~ 2 EJ = 2 x 1018 J) was followed by a tsunami that rose as high as 14 m!

4. Site of the earthquake

5. How many magnitude 9 or higher earthquakes do we know of
How many magnitude 9 or higher earthquakes do we know of? (the magnitude scale was first devised in 1934)
Date - UTC Time
Latitude
Longitude
Magnitude
Fatalities
Region
5/22/60 19:11
-38.29
-73.05
9.5
1655
Chile
3/28/64 3:36
61.02
9.2
125
Prince William Sound, Alaska
12/26/04 0:58
3.295
95.982
9.1
227898
off the west coast of N. Sumatra
11/4/52 16:58
52.76
160.06 9
Kamchatka, Russia
3/11/11 5:46
38.322
28050
Near the E. Coast of Honshu, Japan

6. “Japan faces power struggle,” Jeff Tollefson, Nature 472, 143-144 (2011), 14 April 2011.

7. The tsunami hit the BWRs at Fukushima, and made the backup generators inoperable. This initiated catastrophic events.

8. To understand what happened, we need to understand something about the operation of reactors. To do that, we need to get some background in how energy can be liberated by combining or breaking up nuclei.

9. Fusion — energy liberated by combining nucleons into larger nuclei
Fusion — energy liberated by combining nucleons into larger nuclei. Fission — energy liberated by breaking up nuclei into pieces.

10. Both happen because of binding energy
Both happen because of binding energy. This is the energy that the nucleons (constituents of the nucleus) give up to become part of the nucleus.

11. It is the difference between the sum of the masses of protons, neutrons, and electrons in an atom and the actual atomic mass of that atom.

12. The first nucleons in the nucleus fall farthest in
The first nucleons in the nucleus fall farthest in. The next don’t fall quite as far, and they continue to fall a lesser distance in as the number of nucleons increases.

13. This occurs because of the Pauli Exclusion Principle, the same reason that not all electrons in an atom are in the same shell. It is the average binding energy per nucleon that counts.

15. On the left side of this curve, the nucleons on average give up more energy as A increases up to about iron-56. After iron-56, the nucleons on average give up less energy as A increases.

16. If we’re forming nuclei on the left side of this curve, fusing nucleons, energy is released—the binding energy. Fusion holds promise on Earth as well, but there are still no energy-producing fusion reactors operating.

17. In normal stars, elements up to iron are made (depending on size; our Sun will make only carbon in its normal operation) by fusion inside the star. This is because temperatures in the Sun’s center are millions of kelvin.

18. To get binding energy to be released on Earth, we need to go to the other end of the curve of the binding energy. Splitting something with A = 235, we can produce, say, nuclei with A = 100 and 135 or other combinations.

19. The nuclei with the smaller A are deeper on average than for A = 235, so energy, binding energy, is released when the bigger nucleus breaks up.

21. The energy released is about 200 MeV per fission.

22. This energy must be captured
This energy must be captured. Typically, in a nuclear reactor, water is used to capture much of the energy released.

23. There are two main types of reactor utilized: BWRs and PWRs.

25. The six reactors at Fukushima are BWRs.

26. The GE BWR schematic. http://www. gereports

27. In general, for any harm caused by something: Dose = Potency
In general, for any harm caused by something: Dose = Potency * Exposure and Health risk = Dose * Exposed population [= Potency * Exposure * Exposed population]

28. For exposure to radiation, Dose = Q
For exposure to radiation, Dose = Q * Exposure, where Q is a quality factor establishing “the value of absorbed dose of any radiation that engenders the same risk as a given absorbed dose of reference radiation.”

29. The gray [Gy] is now the internationally accepted measure of absorbed energy from any type of radiation: it is the exposure from radiation losing 1 J/kg of material (such as tissue). This is actually exposure, but is known as “absorbed dose.”

30. The sievert [Sv] is the internationally accepted measure of dose: it is the dose consequent to an exposure to ionizing radiation undergoing an energy loss of 1 J/kg of body tissue [i.e., 1 gray].

32. This chart is in millisieverts per hour.

33. Converted to mrem (1 Sv = 100 rem)

34. Now that we have some idea of reactor type and health risk, I will turn to the details of the Fukushima disaster in part 2.