Informazioni sul documento
- Università
- Politecnico di Milano
- Corso di laurea
- Energy Engineering
- Materia
- Heat and Mass Transfer Scambio Termico e di Massa
- Classificazione
- Esercizi · Divisi per argomento
- Formato originale
- Testo
- Testo ricercabile
Divisi per argomento di Heat and Mass Transfer Scambio Termico e di Massa per il corso di Energy Engineering presso Politecnico di Milano. Materiale proveniente dall’archivio storico Studwiz e classificato per la consultazione online.
Divisi per argomento di Heat and Mass Transfer Scambio Termico e di Massa per il corso di Energy Engineering presso Politecnico di Milano. Materiale proveniente dall’archivio storico Studwiz e classificato per la consultazione online.
Qualità dell’importazione: il testo è stato estratto direttamente dal documento originale.
Passaggi rappresentativi riconosciuti nelle diverse parti del materiale. Il testo completo resta presente nella pagina per la ricerca, mentre l’anteprima compatta rende più semplice la lettura.
0.1 Radiative heat transfer: exercise 3 0.1.1 Description The components of an electronic package in an orbiting satellite are mounted in a compartment that is well insulated on all but one of its sides. The uninsulated side is inclined to the sun radiation (surface temperature: Ts 5800K, heat flux at the orbit of the earth: qs 1.35 103W m 2) and consists of an isothermal copper plate (squared, flat, opaque, di↵use, side: l 1.0m, plate temperature: Tp 500K, inclination to sun radiation: ✓ ⇡ 6rad, spectral emissivity: ✏ ,1 0.20 for 0.0; 2.0 µm, ✏ ,2 0.80 for 2.0; µm) whose outer surface is exposed to the vacuum of outer space and whose inner surface is attached to the components. Assuming steady-state operating conditions: 1. compute the power dissipated by the components. 0.1.2 Questions 1. compute the power dissipated by the components. 0.1.3 Data SUN surface temperature: Ts 5800.0 K 5527.0 C heat flux at the orbit of the earth: qs 1.35 103 W m 2 1.35 kW m 2 COPPER PLA TE squared flat opaque di↵use side: l 1.000 m plate temperature: Tp 500.0 K 227.0 C inclination to sun radiation: ✓ 0.5236 rad spectral emissivity: ✏ ✏ ,1 0.20 0.0; 2 .0 µm ✏ ,2 0.80 2.0; µm (1) CONST ANTS Stefan - Boltzmann constant: 5.67 10 8 W m 2 K 4 Wien’s displacement law constant: Cw 2.90 103 µmK 0.1.4 Solution QUESTION 1 The Wien’s law provides the wavelength corresponding to the peak emission of a blackbody at a given surface temperature. That value, which is not strictly required, is useful, selecting the right temperature, to estimate in advance, for a given spectral hemispherical emissivity distribution: • the total hemispherical absorptivity (the sun surface temperature is required), • the total hemispherical emissivity (the copper surface temperature is required), and check the outcome of the…
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