IOAA 2021, Теория — Задача 5. Under pressure (10 points).

Theory — Q5-1 — English (Official) — Under pressure (10 points). · 10 т.

Условие

Magnetic fields in the Sun are constantly shaping the structure of various different features in the Solar atmosphere. Inside any feature, the magnetic field ($B$) adds to the total pressure exerted by the gas. This so-called magnetic pressure is a function of the height z and can be expressed as:

On the other hand, the gas can be considered to be in hydrostatic equilibrium and hence the gas pressure decays exponentially from an initial pressure value $P_0$ with increasing z. It can be expressed as,

where H is the scale height, i.e. the height at which the pressure falls to $\frac{P_0}{e}$.
Consider one type of feature, a magnetic flux tube rising from the Solar surface up into an unmagnetized environment (see Figure below). Assuming that the total pressure of the material inside the tube and of the material outside it is in equilibrium,

5.1 Find an expression for the magnetic field strength as a function of height $z$. [7 т.]

5.2 If the magnetic field at the base of a flux tube is $0.3T$, and scale height $H$ in a given solar model is $150\ km$, at what height will the magnetic field be reduced to $0.03T$? [3 т.]

Отговори

Решение

Official solution source discrepancy

The first line of official solution 5.2 states “At z = H” and uses an exponent −z/150, whereas its following substitution uses −z/(2×150). These source statements are retained.

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Оригинал в Архива: TQ-5-Q.pdf · официални решения: TQ5 (3).pdf · допълнителни данни: TQ-5-A.pdf · допълнителни данни: Standard-Table-of-constants.docx.pdf · допълнителни данни: TQ-G.pdf · допълнителни данни: data.pdf