There are two classic explanations for the mass loss of stars by stellar winds. For stars of high luminosityradiation pressure is the driving force; for fainter stars like the Sun the stellar wind is driven by mechanical effects such as shock waves or magnetic fields. To what level a stellar wind swells, depends on accidental features of the mechanism. The strength of the wind is not easily related to the basic properties of the star. Andriesse's fluctuation theory is a metatheory for the two mechanisms mentioned. It does not matter much which mechanism occurs in a certain star, as long as that mechanism meets certain requirements: the stellar wind must take the form of puffs that are so pronounced that they affect the equilibrium between gravitational and thermal forces of the star as a whole. Only after the equilibrium is regained, a subsequent puff may take place. The fluctuation theory establishes a clear link between the strength of the stellar wind and the basic properties of the star, which, as mentioned above, the mechanisms by themselves cannot establish. Metatheories are not very common in astrophysics. Also fluctuations are usually ignored rather than taken as a starting point. When the fluctuation theory, which Andriesse still sees as his best work, did not gain much acceptance, Andriesse left astrophysics in disappointment in 1980.
Nuclear Energy
He joined the research institute KEMA of the Dutch electricity companies in Arnhem and started a 'source-term' program, with the aim to determine which and how many radioactive substances would be released by nuclear reactors, when they become overheated. Tiny amounts of uranium oxide, irradiated by neutrons, and thus containing fission products, were heated above 2,000 degrees. When these experiments were under way, the nuclear reactor in Chernobyl exploded. There happened outdoors what Andriesse with his student Richard Tanke were doing inside a safe laboratory His results, presented to the International Atomic Energy Agency, showed that even at very high temperatures most fission products will stay in the reactor core He later cautioned for an explosion of the Petten nuclear reactor caused by a sudden break of the cooling circuit.
After age forty Andriesse started to write fiction for a general audience. In his novels, he steps back from exact science and sketches poetic, often erratic images of a disordered world. His first historical novel "Titan kan niet slapen" got a place on the longlist of the AKO Literatuurprijs in 1994. It is about the life and works of Christiaan Huygens, and it has been translated in French and English. "De opstand" and "Alsnog een portret voor Heinsius" are historical novels about the physician Gadso Coopmans and the politician Anthonie Heinsius. He also wrote books about the history of physics, nuclear energy and science publishing.
Books available in English
Huygens, The Man Behind the Principle, scientific biography of Christiaan Huygens, translated from Dutch by Sally Miedema, Cambridge University Press, Cambridge, 2005, hardcover, 440 pages,. Reviews: