Week 3 Spectra, Spectral Energy Distributions & Shockwaves Part 1 Flashcards

1
Q

define spectrum

A

plot of flux/intensity distribution as a function of frequency or wavelength

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2
Q

what is brightness temperature

A

measure intensity at one frequency and match it to the Planck function

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3
Q

how does radiation colour correlate to temperature

A

blue radiation is associated with higher temps and red radiation with lower temps

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4
Q

what is the colour temperature equation

A

T = 7200/[(B-V)+0.64]

where B-V is the colour index

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5
Q

define colour index

A

difference in magnitude between blue light and visible light

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6
Q

what is the Stefan-Boltzmann equation

A

P = σT^4

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7
Q

what is the Wien limit

A

hf&raquo_space; kT

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8
Q

what is the Rayleigh-Jeans limit

A

hf &laquo_space;kT

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9
Q

what are three requirements for a gas to be modelled as a fluid

A

mean free path &laquo_space;length scales of changes in gas
meaningful small volumes are defined
volume element should contain enough particles to describe the gas in a statistical sense

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10
Q

what 3 conservations are important for fluid mechanics

A

conservation of mass
conservation of momentum
conservation of energy

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11
Q

what are the three equations of state in fluid mechanics that derived from the conservations

A
P = nkT
P = Kρ^γ
P = Kρ
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12
Q

when does a shockwave happen

A

generally happens when a supersonic flow of gas meets an obstacle or when an object moves supersonically through a gas

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13
Q

what does a shock result in

A

discontinuities in the thermodynamic properties

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14
Q

define ram pressure

A

momentum gets transferred between object and gas

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15
Q

define supersonic velocity

A

velocity that exceeds the speed of sound

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16
Q

what is the supersonic velocity equation for an ideal gas

A

cs = SQRT[γP/ρ]

17
Q

what is the Mach equation

A

M = v/cs

18
Q

what is a shockwave

A

a large perturbation in a gas