Stars/Surface fusion/Quiz

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The image shows the cooling post-flare arcade (rotated by -90 degrees so that north is to the right) 6h after the flare (at 00:11 UT on September 8. Credit: TRACE/NASA.

Stellar surface fusion is a lecture. Although a research project on its own, it is also part of the radiation astronomy department course on the principles of radiation astronomy.

You are free to take this quiz based on stellar surface fusion at any time.

To improve your scores, read and study the lecture, the links contained within, listed under See also, External links, and in the {{principles of radiation astronomy}} template. This should give you adequate background to get 100 %.

As a "learning by doing" resource, this quiz helps you to assess your knowledge and understanding of the information, and it is a quiz you may take over and over as a learning resource to improve your knowledge, understanding, test-taking skills, and your score.

Suggestion: Have the lecture available in a separate window.

To master the information and use only your memory while taking the quiz, try rewriting the information from more familiar points of view, or be creative with association.

Enjoy learning by doing!


Hypotheses

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  1. Surface fusion occurs because the interstellar electron influx has high enough energy to cause fusion of lighter nuclei.

See also

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{{Radiation astronomy resources}}{{Principles of radiation astronomy}}