IOAA 2021 — Задача 1. ALMA - Calculating photons (10 points).

Автор: Olympiads XYZ · транскрипция на официалните материали

Проверена срещу оригинала на 13.9.2026 от същия модел, който я е транскрибирал (без независима проверка)

Съдържание

УсловиеРешение

Theory — Q4-1, English (Official) — ALMA - Calculating photons · 10 т.

Условие

ALMA is a radio observatory with a revolutionary design. It consists of 66 high-precision antennas, operating in the wavelength range from 0.32 mm0.32\ \mathrm{mm} to 8.60 mm8.60\ \mathrm{mm}. The principal array has fifty antennas of 12 m12\ \mathrm{m} diameter each that can work together as a single telescope in the so-called interferometric mode. There is also another array of four 12 m12\ \mathrm{m} antennas, and twelve smaller antennas of 7 m7\ \mathrm{m} diameter each.

Imagine that a single 12 m12\ \mathrm{m} antenna is being calibrated, pointing to a source with a known incident flux of 1×1020 W/m21 \times 10^{-20}\ \mathrm{W/m^2}

4.1 Assuming that all the flux arrives at the shortest wavelength of ALMA sensitivity, determine the average number of photons that would reach the detector every second. [2 т.]

4.2 Compare it to the average number of photons that would have reached the detector, if all the flux arrived at the longest wavelength of operation. [2 т.]

4.3 What is the angular resolution (in arcsec) of a single 12 m12\ \mathrm{m} antenna, operating at 74.9 GHz74.9\ \mathrm{GHz}? [2 т.]

4.4 Imagine the principal array operating at 74.9 GHz74.9\ \mathrm{GHz} in the interferometric mode. Assuming for simplicity that the spatial resolution is solely given by the longest baseline (largest distance between any pair of antennas), which turns to be Dmax=16 kmD_{\max} = 16\ \mathrm{km}, what would be the angular resolution (in arcsec) in this case? Treat this case as a single slit aperture instead of a circular one. [2 т.]

4.5 For a radio antenna, the term SEFD refers to 'System Equivalent Flux Density', which is a characteristic energy flux density of the antenna, depending on its temperature and size. We also note that for energy estimation of radio photons, Rayleigh-Jeans approximation is valid. Assuming a system temperature of 691 K691\ K, what would be the SEFD of the full ALMA observatory in Jansky if all the 66 antennas could work together? [2 т.]

Решение

Внимание: Непълно решение

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Оригинал в Архива: TQ-4-Q.pdf