SAE AIR 1213-1971 Radioisotope Power Systems《放射性同位素动力系统》.pdf
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1、- I AIR 1213 REP0 RT Revised the last subsystem is necessary only when the missiQn duration is a substantial fraction of the half-life of the radioisotope fuel selected for the heat source. Operation of the system is as follows: The thermal energy generated in the heat source by the decay of the rad
2、ioisotope is introduced into the energy conversion subsystem from the heat source. in the energy conversion subsystem, a portion of the input heat is converted to electrical energy by either a direct conversion process (i. e. , thermoelectric and thermionic systems) or dynamic conversion process (i.
3、 e. , Rankine and Brayton cycle systems). The unconverted heat is transported from the energy conversion subsystem to the space radiator and then rejected to the environment. if a short half-life radioisotope is utilized in the heat source, excess fuel must be provided at the beginning of the missio
4、n to assure that sufficient thermal energy is available at the end of the mission. For example, when polonium-210 (138-day half-life) is employed as the radioisotope, radioactive decay reduces the initial thermal output by one-half after 138 days of the mission. Some means of controlling the thermal
5、 in- put to the energy conversion system must be provided to prevent an overtemperature of the energy conver- sion system and heat source at the beginning of the mission. To date, this has been accomplished most are controlled by a sensor at a critical temp,erature location. efiectively by allowing
6、the heat source to radiate this heat directly to space through movable shutters Currently, only thermoelectric systems have been extensively developed for use with radioisotope heat sources and practically applied to space missions. These efforts have culminated in numerous terrestrial and space-ori
7、ented systems. Development of radioisotope-powered thermionic systems has been embodied primarily in the SNAP 13 program which is currently inactive. Development of Brayton and Rankine cycle systems for use with radioisotope heat sources is currently in progress. Generally, the efficiency of radiois
8、otope power systems range from 4 to 8 per cent for a thermoelectric system to potentially 20 to 25 per cent for Brayton and Rankine cycle systems with thermionic systems in the intermediate range of potentially 10 to 15 per cent. (The term “potentially“ is used since no extensive system data are ava
9、ilable for these latter systems. ) Typical current 9light-qualifiedtt radioisotope thermo electric space power systems have specific powers of approximately 1-watt per pound and system efficien- cies near 5 per cent. Radioisotope Heat Source: The primary requirements for the radioisotope heat source
10、 are that: (1) It provide a surface for heat input to the power conversion subsystem (2) The half-life of the radioisotope be compatible with the intended mission length (3) Mating components be chemically compatible at the anti- cipated operational temperatures (4) The launch and aerospace nuclear
11、saety requirements are satisfied. The radioisotope heat source contains a naturally decaying radioisotope fuel. This heat source is complete- ly static and requires no control mechanism Bince the thermal output of the fuel is self-regulating, decreas- ing exponentially with time, Thus, he output at
12、any time can be precisely determined f the output at a former time ti is known using the relation COPYRIGHT SAE International (Society of Automotive Engineers, Inc)Licensed by Information Handling ServicesSAE AIR*1213 71 8357340 0003777 O W -3- - Xt = P(ti)e where: p (t) = power at time t P(ti) x =
13、disintegration constant = O. 693 T 1/2 = power at some former time T 1/2 = half-life of radioisotope = time since P(t.) was determined. 1 t From this equation it is evident that the power available (and quantity of radioisotope present) with time de- pends on the half-life of the radioisotope chosen
14、 as the fuel. Ideally, it is desirable to select a radioisotope with a half-life of such length that during the mission the reduction in fuel thermal power is negligible, thus eliminating the complexity of a thermal control device. However, radioisotope availability, nuclear safety requirements and
15、cost must be considered in fuel selection. Presently, plutonium-238 (T 1/2 = 87 years) has been considered primarily for space-oriented systems with missions of 1 year and greater, while curium-242 (T 1/2 = 163 days) and polonium-210 (T 1/2 = 138 days) have shown feasibility for missions up to appro
16、ximately four months. 1.2.1 Nuclear Radiations: Present emphasis in radioisotope power generation is on utilizing the decay energy in a heat engine. beta particle, or as the energy of gamma photons. The slowing down and/or absorption of these radia- tions causes an increase in the temperature of the
17、 surrounding material and, in some cases, secondary radiations are produced. Any radiation which is not absorbed to produce heat will become unavailable for use in the heat engine. The energy from a radioisotope initially appears as motion of the emitted alpha or Alpha (u ) particles (helium nuclei)
18、 have a comparatively large mass and a high positive electrical chargi This means that a high energy alpha particle (all important alpha emitters produce about 5 Mev per dis- integration) will have a relatively low velocity, and because of its charge, interacts strongly with other matter; it will be
19、 thermalized in a few hundredths of a millimeter of solid material. Thus, for all prac- tical purposes the thermal energy of an alpha emitter is produced within the decaying material. In some cases gamma radiation is also emitted and carries a small portion of the decay energy. The absorption of an
20、alpha particle in a light-element nucleus can produce secondary neutrons, but this usually repre- sents a radiation hazard rather than a large energy loss. Some alpha emitting materials also undergo a small amount of spontaneous fission, but for practical purposes this has no effect on the heat prod
21、uc- tion rate with the radioisotopes usually considered for power production. It can, however, lead to high neutron fluxes that present a biological hazard. Alpha particles are helium nuclei, consequently when they have lost the kinetic energy associated with decay, they will capture free electrons
22、and form helium atoms. This helium appears as a free gas in the fuel container and may either be contained in the fuel encapsulation or vented to prevent pressure buildup. Beta () particles (electrons) of the energy associated with fuels used in radioisotope power systems will penetrate one to three
23、 millimeters of solid material and, hence, for practical purposes will not es- cape the fuel container. However, in the process of slowing down these particles, high energy electro- magnetic radiation lmown as bremsstrahlung is produced. This radiation, identical to gamma radiation, can contribute a
24、bout 1% heat loss since the photons produced can have energies ranging up to that of the beta particle. of more seriousness is the biological shielding problem associated with the bremsstrah- lung. Bremsstrahlung production is approximately proportional to the square of the atomic number of the beta
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