Unit C.5: Doppler Effect单元 C.5:多普勒效应
The closing super-topic of Theme C "Wave behaviour". The pitch of a passing siren rises on approach and drops on recession because relative motion between source and observer compresses or stretches the wavefronts. This unit develops that idea from a qualitative picture into quantitative shift equations: the HL-only moving-source and moving-observer sound formulas, and the single low-speed light formula that underpins redshift, blueshift, the evidence for an expanding universe, radar speed guns, Doppler ultrasound, and sonar.主题 C"波的行为"的收官超主题。驶过的警笛在接近时音调升高、远离时音调降低,原因是波源与观察者之间的相对运动压缩或拉伸了波前。本单元把这一定性图像发展为定量的频移方程:HL 专属的波源运动与观察者运动声波公式,以及支撑红移、蓝移、宇宙膨胀证据、雷达测速、多普勒超声与声呐的单一低速光频移公式。
How to use this guide本指南使用说明
C.5 splits cleanly into three layers. The qualitative picture (wavefront bunching, pitch up on approach) is examinable for everyone. The explicit moving-source and moving-observer sound equations are HL only. The light shift $\frac{\Delta f}{f} \approx \frac{v}{c}$ is for everyone and drives the astrophysics applications. Marks are lost by mixing up which speed goes where and by getting the sign of the $\pm$ wrong, so the whole unit rewards drawing a clear "who is moving toward whom" diagram before reaching for a formula.C.5 清晰地分为三层。定性图像(波前堆积、接近时音调升高)人人都要考。显式的波源运动与观察者运动声波公式仅为 HL。光的频移 $\frac{\Delta f}{f} \approx \frac{v}{c}$ 人人都考,并支撑天体物理应用。失分往往来自把哪个速度放错位置,以及搞错 $\pm$ 的符号;因此本单元最看重在动笔前先画一张"谁朝谁运动"的示意图。
Approach $\Rightarrow$ higher frequency (pitch up, blueshift); recession $\Rightarrow$ lower frequency (pitch down, redshift). For sound (HL), moving source: $f' = f\frac{v}{v \pm v_s}$ (minus on approach). Moving observer: $f' = f\frac{v \pm v_o}{v}$ (plus on approach). For light at $v \ll c$: $\frac{\Delta f}{f} \approx \frac{\Delta\lambda}{\lambda} \approx \frac{v}{c}$.
接近 $\Rightarrow$ 频率升高(音调升高、蓝移);远离 $\Rightarrow$ 频率降低(音调降低、红移)。声波(HL)波源运动:$f' = f\frac{v}{v \pm v_s}$(接近取减号)。观察者运动:$f' = f\frac{v \pm v_o}{v}$(接近取加号)。光在 $v \ll c$ 时:$\frac{\Delta f}{f} \approx \frac{\Delta\lambda}{\lambda} \approx \frac{v}{c}$。
Be able to derive the moving-source result from compressed wavelength $\lambda' = (v \pm v_s)/f$ and explain why moving source and moving observer give different formulas even for the same relative speed (the medium picks a rest frame for sound). Know that the light formula is symmetric in source/observer motion (no medium), and that the sign of $v$ is set by whether the separation is increasing (redshift) or decreasing (blueshift). State a sign convention every time.
能从压缩波长 $\lambda' = (v \pm v_s)/f$ 推导波源运动结果,并解释为何即使相对速度相同,波源运动与观察者运动给出不同公式(声波的介质选定了一个静止参考系)。要知道光的公式对波源/观察者运动是对称的(无介质),且 $v$ 的符号由间距是增大(红移)还是减小(蓝移)决定。每次都写明sign convention(符号约定)。
Wavefront Bunching and Why Pitch Shifts波前堆积与音调变化的原因 C.5 SL+HL
- The Doppler effect is the change in observed frequency (and wavelength) of a wave when the source and observer move relative to one another.
- Approach (separation decreasing): wavefronts bunch up $\Rightarrow$ shorter $\lambda$ $\Rightarrow$ higher $f$ $\Rightarrow$ higher pitch / blueshift.
- Recession (separation increasing): wavefronts stretch out $\Rightarrow$ longer $\lambda$ $\Rightarrow$ lower $f$ $\Rightarrow$ lower pitch / redshift.
- 多普勒效应(Doppler effect)是当波源(source)与观察者(observer)相对运动时,观察到的波的频率(与波长)发生变化的现象。
- 接近(间距减小):波前堆积 $\Rightarrow$ $\lambda$ 变短 $\Rightarrow$ $f$ 升高 $\Rightarrow$ 音调升高 / 蓝移。
- 远离(间距增大):波前拉伸 $\Rightarrow$ $\lambda$ 变长 $\Rightarrow$ $f$ 降低 $\Rightarrow$ 音调降低 / 红移。
An ambulance siren emits a steady tone. As it drives past a stationary listener at constant speed, describe what the listener hears, and state the frequency relative to the emitted frequency $f$ both before and after the ambulance passes.救护车警笛发出稳定音调。当它以恒定速度驶过一名静止的听者时,描述听者所听到的声音,并说明在救护车经过前后所听频率相对于发射频率 $f$ 的关系。
Identify. The relevant quantity is the line-of-sight relative motion between source and observer.
识别。关键量是波源与观察者之间沿视线方向的相对运动。
Set up. Before passing, the ambulance is approaching: separation decreases, wavefronts bunch, $\lambda$ shortens. After passing, it is receding: separation increases, wavefronts stretch, $\lambda$ lengthens.
列式。经过前,救护车正在接近:间距减小,波前堆积,$\lambda$ 变短。经过后正在远离:间距增大,波前拉伸,$\lambda$ 变长。
Execute. Before passing, $f' > f$ (higher pitch, roughly constant). After passing, $f' < f$ (lower pitch). At the exact moment of passing, the motion is momentarily perpendicular to the line of sight, so $f' \approx f$.
求解。经过前,$f' > f$(音调偏高、大致恒定)。经过后,$f' < f$(音调偏低)。在恰好经过的瞬间,运动暂时垂直于视线,故 $f' \approx f$。
Evaluate. The listener hears a sudden drop in pitch as the ambulance passes — not a continuous rise. The pitch is high-then-low, with the change concentrated near passing.
评估。听者在救护车经过时听到音调骤降——不是连续升高。音调是先高后低,变化集中在经过附近。
Going deeper: it is the line-of-sight component that matters深入:起作用的是视线方向分量
The Doppler shift depends only on the component of relative velocity along the line joining source and observer (the radial component). A source moving in a circle around the observer at constant radius produces no shift, because its radial velocity is always zero even though its speed is large.
多普勒频移只取决于相对速度沿波源与观察者连线方向(径向)的分量。绕观察者做等半径圆周运动的波源不产生频移,因为其径向速度始终为零,尽管速率很大。
This is why an aircraft flying tangentially overhead shows the strongest pitch drop just as it crosses directly above you: that is when the radial velocity swings fastest from $+v$ (approaching) through $0$ to $-v$ (receding).
这就是为何切向飞过头顶的飞机在它恰好越过你正上方时音调降得最明显:此刻径向速度从 $+v$(接近)经 $0$ 最快地摆到 $-v$(远离)。
Moving Source, Stationary Observer波源运动、观察者静止 HL C.5 HL
f' = f v / (v ± v_s):
$$ f' = f\,\frac{v}{v \pm v_s}. $$
Sign rule. Use the minus sign when the source moves toward the observer (denominator smaller $\Rightarrow$ $f' > f$, blueshift). Use plus when the source moves away ($f' < f$, redshift).
Why. The source chases its own wavefronts, so the emitted wavelength ahead is compressed to $\lambda' = (v \pm v_s)/f$.
f' = f v / (v ± v_s):
$$ f' = f\,\frac{v}{v \pm v_s}. $$
符号规则。当波源朝观察者运动时取减号(分母变小 $\Rightarrow$ $f' > f$,蓝移)。当波源远离时取加号($f' < f$,红移)。
原因。波源追赶自己的波前,故前方发出的波长被压缩为 $\lambda' = (v \pm v_s)/f$。
A train sounds a $400\ \mathrm{Hz}$ whistle and moves toward a stationary observer at $30\ \mathrm{m\,s^{-1}}$. The speed of sound is $340\ \mathrm{m\,s^{-1}}$. Find the frequency the observer hears, then the frequency after the train has passed and is receding at the same speed.火车鸣 $400\ \mathrm{Hz}$ 汽笛,以 $30\ \mathrm{m\,s^{-1}}$ 朝静止观察者运动。声速为 $340\ \mathrm{m\,s^{-1}}$。求观察者听到的频率,以及火车经过后以同速远离时的频率。
Identify. Source moving, observer stationary $\Rightarrow$ use the HL moving-source equation f' = f v / (v ± v_s).
识别。波源运动、观察者静止 $\Rightarrow$ 用 HL 波源运动公式 f' = f v / (v ± v_s)。
Approaching (minus sign).
接近(取减号)。
$$ f' = 400 \times \frac{340}{340 - 30} = 400 \times \frac{340}{310} \approx 439\ \mathrm{Hz}. $$Receding (plus sign).
远离(取加号)。
$$ f' = 400 \times \frac{340}{340 + 30} = 400 \times \frac{340}{370} \approx 368\ \mathrm{Hz}. $$Evaluate. The observer hears the pitch jump from about $439\ \mathrm{Hz}$ to about $368\ \mathrm{Hz}$ as the train passes — a drop of roughly $71\ \mathrm{Hz}$. Note the shifts are not symmetric: the rise on approach ($+39$) exceeds the fall on recession ($-32$), a hallmark of the moving-source case.
评估。火车经过时观察者听到音调由约 $439\ \mathrm{Hz}$ 跳到约 $368\ \mathrm{Hz}$——下降约 $71\ \mathrm{Hz}$。注意频移并不对称:接近时升高($+39$)大于远离时降低($-32$),这是波源运动情形的特征。
Going deeper: deriving $f' = f v/(v - v_s)$ from compressed wavefronts深入:由压缩波前推导 $f' = f v/(v - v_s)$
In one period $T = 1/f$ the source emits one wavefront and itself advances a distance $v_s T$ toward the observer. The next wavefront is emitted from that advanced position. So ahead of the source, successive wavefronts are separated not by $\lambda = vT$ but by
在一个周期 $T = 1/f$ 内,波源发出一个波前,自身朝观察者前进 $v_s T$。下一个波前从前进后的位置发出。因此在波源前方,相继波前的间距不再是 $\lambda = vT$,而是
$$ \lambda' = vT - v_s T = (v - v_s)\,T = \frac{v - v_s}{f}. $$The observer still measures the wave travelling at speed $v$, so the frequency received is
观察者测得的波速仍为 $v$,故接收频率为
$$ f' = \frac{v}{\lambda'} = \frac{v}{(v - v_s)/f} = f\,\frac{v}{v - v_s}. $$Replacing $v_s \to -v_s$ for a receding source gives the $+$ version. This derivation shows clearly that what changes is the wavelength, not the wave speed in the medium.
对远离的波源用 $v_s \to -v_s$ 即得 $+$ 形式。该推导清楚表明:改变的是波长,而非介质中的波速。
Moving Observer, Stationary Source观察者运动、波源静止 HL C.5 HL
f' = f (v ± v_o) / v:
$$ f' = f\,\frac{v \pm v_o}{v}. $$
Sign rule. Use plus when the observer moves toward the source ($f' > f$); use minus when moving away ($f' < f$).
Combined case. Source and observer both moving:
$$ f' = f\,\frac{v \pm v_o}{v \pm v_s}. $$
Pick each sign so that approach raises $f'$.
f' = f (v ± v_o) / v:
$$ f' = f\,\frac{v \pm v_o}{v}. $$
符号规则。观察者朝波源运动取加号($f' > f$);远离取减号($f' < f$)。
组合情形。波源与观察者都运动:
$$ f' = f\,\frac{v \pm v_o}{v \pm v_s}. $$
取号原则:接近使 $f'$ 升高。
A stationary loudspeaker emits a $500\ \mathrm{Hz}$ tone. A cyclist rides toward it at $10\ \mathrm{m\,s^{-1}}$ ($v_{\text{sound}} = 340\ \mathrm{m\,s^{-1}}$). (a) Find the frequency the cyclist hears. (b) Now suppose the speaker is itself carried toward the cyclist at $10\ \mathrm{m\,s^{-1}}$ while the cyclist still rides toward it at $10\ \mathrm{m\,s^{-1}}$; find the new frequency.静止扬声器发出 $500\ \mathrm{Hz}$ 音调。骑车者以 $10\ \mathrm{m\,s^{-1}}$ 朝它骑行($v_{\text{声}} = 340\ \mathrm{m\,s^{-1}}$)。(a) 求骑车者听到的频率。(b) 若扬声器本身也以 $10\ \mathrm{m\,s^{-1}}$ 朝骑车者运动,而骑车者仍以 $10\ \mathrm{m\,s^{-1}}$ 朝它骑行,求新频率。
Identify (a). Observer moving toward stationary source $\Rightarrow$ f' = f (v + v_o)/v with the plus sign.
识别 (a)。观察者朝静止波源运动 $\Rightarrow$ f' = f (v + v_o)/v,取加号。
Identify (b). Both moving toward each other $\Rightarrow$ combined formula, plus on top (observer approaches), minus on bottom (source approaches).
识别 (b)。两者相向运动 $\Rightarrow$ 组合公式,分子取加号(观察者接近),分母取减号(波源接近)。
$$ f' = 500 \times \frac{340 + 10}{340 - 10} = 500 \times \frac{350}{330} \approx 530\ \mathrm{Hz}. $$Evaluate. Even though both speeds are $10\ \mathrm{m\,s^{-1}}$, the moving-observer shift ($+15\ \mathrm{Hz}$) and the moving-source contribution differ slightly because the formulas are different. Sound, unlike light, is not symmetric in which body moves: the medium defines a rest frame.
评估。尽管两速率都是 $10\ \mathrm{m\,s^{-1}}$,观察者运动的频移($+15\ \mathrm{Hz}$)与波源运动的贡献略有不同,因为公式不同。声波(不同于光)对"谁运动"不对称:介质定义了一个静止参考系。
Going deeper: why moving observer adds, moving source divides深入:为何观察者运动是相加、波源运动是相除
A moving observer does not change the wavelength in the medium — the wavefronts are still spaced by $\lambda = v/f$. What changes is the rate at which the observer sweeps through them. Moving toward the source at $v_o$, the observer meets wavefronts at the relative speed $v + v_o$, so
运动的观察者不改变介质中的波长——波前间距仍为 $\lambda = v/f$。改变的是观察者掠过波前的速率。以 $v_o$ 朝波源运动时,观察者以相对速度 $v + v_o$ 遇到波前,故
$$ f' = \frac{v + v_o}{\lambda} = \frac{v + v_o}{v/f} = f\,\frac{v + v_o}{v}. $$A moving source instead changes $\lambda$ itself (Section C5.2), which is why $v_s$ enters in the denominator. Same relative speed, different physics — and the two formulas only coincide to first order in $v/v_{\text{sound}}$.
而运动的波源改变的是 $\lambda$ 本身(见 C5.2),这就是 $v_s$ 进入分母的原因。相同相对速度、不同物理——两个公式仅在 $v/v_{\text{声}}$ 的一阶近似下一致。
Doppler Shift for Electromagnetic Waves电磁波的多普勒频移 C.5 SL+HL
Δf / f ≈ Δλ / λ ≈ v / c:
$$ \frac{\Delta f}{f} \approx \frac{\Delta\lambda}{\lambda} \approx \frac{v}{c}. $$
What is symmetric. Light needs no medium, so only the relative velocity matters — moving source and moving observer give the same shift. There is one formula, not two.
Signs. Recession (separation increasing) $\Rightarrow$ $\lambda$ increases (redshift). Approach $\Rightarrow$ $\lambda$ decreases (blueshift). $\Delta\lambda = \lambda_{\text{obs}} - \lambda_{\text{rest}}$.
Δf / f ≈ Δλ / λ ≈ v / c:
$$ \frac{\Delta f}{f} \approx \frac{\Delta\lambda}{\lambda} \approx \frac{v}{c}. $$
对称之处。光不需要介质,故只有相对速度起作用——波源运动与观察者运动给出相同频移。只有一个公式,而非两个。
符号。远离(间距增大)$\Rightarrow$ $\lambda$ 增大(红移)。接近 $\Rightarrow$ $\lambda$ 减小(蓝移)。$\Delta\lambda = \lambda_{\text{obs}} - \lambda_{\text{rest}}$。
A hydrogen line with rest wavelength $656.3\ \mathrm{nm}$ is observed from a distant galaxy at $658.5\ \mathrm{nm}$. Taking $c = 3.00\times10^{8}\ \mathrm{m\,s^{-1}}$, find the radial speed of the galaxy and state whether it is approaching or receding.某谱线静止波长 $656.3\ \mathrm{nm}$ 的氢线,从遥远星系观测为 $658.5\ \mathrm{nm}$。取 $c = 3.00\times10^{8}\ \mathrm{m\,s^{-1}}$,求该星系的径向速度,并说明是接近还是远离。
Identify. Light source, small shift $\Rightarrow$ use Δλ/λ ≈ v/c.
识别。光源、小频移 $\Rightarrow$ 用 Δλ/λ ≈ v/c。
Compute the shift. $\Delta\lambda = 658.5 - 656.3 = 2.2\ \mathrm{nm}$. The wavelength has increased, so this is a redshift (recession).
计算频移。$\Delta\lambda = 658.5 - 656.3 = 2.2\ \mathrm{nm}$。波长增大,故为红移(远离)。
$$ v \approx c\,\frac{\Delta\lambda}{\lambda} = (3.00\times10^{8}) \times \frac{2.2}{656.3} \approx 1.0\times10^{6}\ \mathrm{m\,s^{-1}}. $$Evaluate. The galaxy recedes at about $1.0\times10^{6}\ \mathrm{m\,s^{-1}}$, roughly $0.3\%$ of $c$. Since $v \ll c$, the low-speed approximation is well justified.
评估。星系以约 $1.0\times10^{6}\ \mathrm{m\,s^{-1}}$ 远离,约为 $c$ 的 $0.3\%$。由于 $v \ll c$,低速近似完全成立。
Going deeper: why $\Delta f/f$ and $\Delta\lambda/\lambda$ have opposite signs but equal magnitude深入:为何 $\Delta f/f$ 与 $\Delta\lambda/\lambda$ 符号相反但大小相等
For light in vacuum $c = f\lambda$ is fixed, so $f\lambda = \text{const}$. Differentiating, $\lambda\,\Delta f + f\,\Delta\lambda \approx 0$, hence
真空中光满足 $c = f\lambda$ 恒定,即 $f\lambda = \text{常数}$。微分得 $\lambda\,\Delta f + f\,\Delta\lambda \approx 0$,于是
$$ \frac{\Delta f}{f} \approx -\frac{\Delta\lambda}{\lambda}. $$The magnitudes match (both $\approx v/c$), but a redshift means $\Delta\lambda > 0$ and $\Delta f < 0$. The data-booklet line $\frac{\Delta f}{f} \approx \frac{\Delta\lambda}{\lambda} \approx \frac{v}{c}$ is a magnitude statement; in problems you decide red vs blue from the physical direction of motion. This formula is the non-relativistic limit — for $v$ comparable to $c$ the full relativistic Doppler formula is needed, but the IB course stays at $v \ll c$.
两者大小相等(都约 $v/c$),但红移意味着 $\Delta\lambda > 0$ 而 $\Delta f < 0$。数据手册的 $\frac{\Delta f}{f} \approx \frac{\Delta\lambda}{\lambda} \approx \frac{v}{c}$ 是大小关系式;解题时由运动的物理方向判断红/蓝。该公式是非相对论极限——当 $v$ 接近 $c$ 时需用完整的相对论多普勒公式,但 IB 课程停留在 $v \ll c$。
Astronomical Evidence for an Expanding Universe宇宙膨胀的天文证据 C.5 SL+HL
- Redshift: observed $\lambda$ longer than rest $\lambda$ ($\Delta\lambda > 0$) $\Rightarrow$ source receding.
- Blueshift: observed $\lambda$ shorter than rest $\lambda$ ($\Delta\lambda < 0$) $\Rightarrow$ source approaching.
- 红移(redshift):观测 $\lambda$ 长于静止 $\lambda$($\Delta\lambda > 0$)$\Rightarrow$ 波源远离。
- 蓝移(blueshift):观测 $\lambda$ 短于静止 $\lambda$($\Delta\lambda < 0$)$\Rightarrow$ 波源接近。
A calcium line of rest wavelength $393.4\ \mathrm{nm}$ appears redshifted to $401.2\ \mathrm{nm}$ in a galaxy's spectrum. (a) Find the recession speed. (b) State what this, together with similar measurements at many distances, is evidence for.某星系光谱中静止波长 $393.4\ \mathrm{nm}$ 的钙线红移至 $401.2\ \mathrm{nm}$。(a) 求退行速度。(b) 说明这一结果连同许多不同距离上的类似测量能作为什么证据。
Identify. Redshift of a light source $\Rightarrow$ v ≈ c Δλ/λ.
识别。光源红移 $\Rightarrow$ v ≈ c Δλ/λ。
Shift. $\Delta\lambda = 401.2 - 393.4 = 7.8\ \mathrm{nm}$, positive $\Rightarrow$ recession.
频移。$\Delta\lambda = 401.2 - 393.4 = 7.8\ \mathrm{nm}$,为正 $\Rightarrow$ 远离。
$$ v \approx c\,\frac{\Delta\lambda}{\lambda} = (3.00\times10^{8}) \times \frac{7.8}{393.4} \approx 5.9\times10^{6}\ \mathrm{m\,s^{-1}}. $$Interpret (b). The galaxy recedes at about $5.9\times10^{6}\ \mathrm{m\,s^{-1}}$ ($\sim 2\%$ of $c$). The systematic redshift of distant galaxies, growing with distance, is direct evidence that the universe is expanding (the Big Bang picture).
解读 (b)。星系以约 $5.9\times10^{6}\ \mathrm{m\,s^{-1}}$ 退行(约 $c$ 的 $2\%$)。遥远星系普遍红移且随距离增大,是宇宙正在膨胀(大爆炸图景)的直接证据。
Going deeper: why we still see blueshift sometimes深入:为何有时仍能看到蓝移
Not everything is redshifted. The Andromeda galaxy, our nearest large neighbour, is blueshifted: its local gravitational pull toward the Milky Way exceeds the cosmological recession at such close range, so it is actually approaching us. Cosmological redshift only dominates for galaxies far enough that the expansion of space outruns local "peculiar" velocities.
并非一切都红移。仙女座星系是离我们最近的大邻居,呈蓝移:在如此近的距离上,它朝银河系的局部引力吸引超过宇宙学退行,故它实际上正在接近我们。宇宙学红移只在足够远、空间膨胀超过局部"本动"速度的星系上占主导。
In a binary star system, the two stars alternately approach and recede as they orbit, so their spectral lines shift back and forth periodically — a Doppler signature used to detect unseen companions, including exoplanets.
在双星系统中,两颗恒星随轨道运动交替接近与远离,其谱线周期性来回移动——这一多普勒特征被用来探测看不见的伴星,包括系外行星。
Radar Speed Guns, Doppler Ultrasound and Sonar雷达测速枪、多普勒超声与声呐 C.5 SL+HL
A police radar gun emits microwaves of frequency $24.0\ \mathrm{GHz}$ at a car driving directly toward it. The reflected beam returns shifted up by $4.0\ \mathrm{kHz}$. Taking $c = 3.0\times10^{8}\ \mathrm{m\,s^{-1}}$, find the car's speed.警用雷达枪向迎面驶来的汽车发射 $24.0\ \mathrm{GHz}$ 微波。反射波返回时频率升高 $4.0\ \mathrm{kHz}$。取 $c = 3.0\times10^{8}\ \mathrm{m\,s^{-1}}$,求车速。
Identify. Reflection off a moving target $\Rightarrow$ double shift: $\Delta f / f \approx 2v/c$.
识别。波从运动目标反射 $\Rightarrow$ 双重频移:$\Delta f / f \approx 2v/c$。
Rearrange for $v$.
解出 $v$。
$$ v \approx \frac{c\,\Delta f}{2 f} = \frac{(3.0\times10^{8})(4.0\times10^{3})}{2 \times (24.0\times10^{9})}. $$ $$ v \approx \frac{1.2\times10^{12}}{4.8\times10^{10}} = 25\ \mathrm{m\,s^{-1}} \approx 90\ \mathrm{km\,h^{-1}}. $$Evaluate. The car travels at about $25\ \mathrm{m\,s^{-1}}$. Forgetting the factor of $2$ (treating it as a one-way shift) would double the reported speed — a classic exam trap.
评估。车速约 $25\ \mathrm{m\,s^{-1}}$。漏掉因子 $2$(当作单程频移)会使报出的速度翻倍——典型考试陷阱。
Going deeper: Doppler ultrasound and the cosine factor深入:多普勒超声与余弦因子
In medical Doppler ultrasound, a probe sends sound (typically a few $\mathrm{MHz}$) into tissue; it reflects off red blood cells moving at speed $v$ and returns shifted by $\Delta f \approx \frac{2 f v \cos\theta}{v_{\text{sound}}}$, where $\theta$ is the angle between the beam and the flow direction. The $\cos\theta$ appears because only the component of blood velocity along the beam Doppler-shifts the echo.
在医学多普勒超声中,探头向组织发出声波(通常几 $\mathrm{MHz}$);它从以速率 $v$ 运动的红细胞反射,返回时频移 $\Delta f \approx \frac{2 f v \cos\theta}{v_{\text{声}}}$,其中 $\theta$ 是声束与血流方向的夹角。出现 $\cos\theta$ 是因为只有沿声束方向的血流速度分量才产生多普勒频移。
Clinicians measure $\Delta f$, know $f$, $v_{\text{sound}}$ in tissue, and $\theta$, and solve for blood-flow speed $v$ — for example to detect a narrowed artery, where flow speeds up. This is the same physics as the radar gun, just with sound in tissue instead of microwaves in air.
临床上测出 $\Delta f$,已知 $f$、组织中 $v_{\text{声}}$ 与 $\theta$,即可解出血流速度 $v$——例如检测变窄的动脉(此处血流加速)。这与雷达枪是同样的物理,只是把空气中的微波换成组织中的声波。
Exam Strategy and Common Pitfalls考试策略与常见陷阱
- Decide "approach or recede" first, then force the sign to match. Approach must give $f' > f$; recede must give $f' < f$. Check your $\pm$ against this before computing.
- 先判断"接近还是远离",再让符号匹配。接近必须给出 $f' > f$;远离必须给出 $f' < f$。计算前先用此核对你的 $\pm$。
- For sound, $v_s$ lives in the denominator and $v_o$ in the numerator. Putting them in the wrong place is the single most common C.5 error.
- 声波中 $v_s$ 在分母、$v_o$ 在分子。放错位置是 C.5 最常见的单一错误。
- The explicit $f' = f v/(v \pm v_s)$ and $f' = f(v \pm v_o)/v$ are HL and apply to sound only. SL questions stay qualitative for sound.
- 显式的 $f' = f v/(v \pm v_s)$ 与 $f' = f(v \pm v_o)/v$ 属 HL,仅适用于声波。SL 对声波只考定性。
- For light, never split into "source vs observer"; use the single $\Delta f/f \approx v/c$ with the relative speed.
- 对光绝不区分"波源还是观察者";直接用单一的 $\Delta f/f \approx v/c$ 配相对速度。
- Any "bounce off a moving target" device (radar, ultrasound, sonar) doubles the shift: $\Delta f/f \approx 2v/c$ or $2v/v_{\text{sound}}$.
- 任何"从运动目标反射"的装置(雷达、超声、声呐)都使频移加倍:$\Delta f/f \approx 2v/c$ 或 $2v/v_{\text{声}}$。
- Read the question: a one-way shift (a passing star) has no factor of 2; a reflected echo does.
- 看清题意:单程频移(驶过的恒星)没有因子 2;反射回波有。
- Keep wavelengths in consistent units; $\Delta\lambda/\lambda$ is dimensionless, so $\mathrm{nm}$ cancels $\mathrm{nm}$. Carry $c$ in $\mathrm{m\,s^{-1}}$.
- 波长保持单位一致;$\Delta\lambda/\lambda$ 无量纲,$\mathrm{nm}$ 与 $\mathrm{nm}$ 相消。$c$ 用 $\mathrm{m\,s^{-1}}$。
- The light formula is the $v \ll c$ limit. If a question gives $v$ near $c$, flag that the simple formula is only approximate.
- 光公式是 $v \ll c$ 极限。若题目给出接近 $c$ 的 $v$,要指出简单公式只是近似。
Flashcards闪卡
Unit C.5 Practice Quiz单元 C.5 练习测验
Readiness Checklist备考清单
Tick each item when you can do it cold, without notes, on your first attempt.
每一条都要"裸做"做对(不看笔记、一次过)才打勾。
- Explain qualitatively why pitch rises on approach and falls on recession using wavefront bunching用波前堆积定性解释为何接近时音调升高、远离时降低
- Describe what a stationary listener hears as a siren passes (high, then a sudden drop)描述警笛驶过时静止听者所听(先高后骤降)
- State that only the radial (line-of-sight) component of relative velocity Doppler-shifts the wave说明只有径向(视线方向)相对速度分量产生多普勒频移
- HL Apply $f' = f v/(v \pm v_s)$ for a moving source with the correct sign用 $f' = f v/(v \pm v_s)$ 求波源运动并取对符号
- HL Apply $f' = f(v \pm v_o)/v$ for a moving observer, and the combined formula when both move用 $f' = f(v \pm v_o)/v$ 求观察者运动,并在两者都动时用组合公式
- HL Explain why moving source and moving observer give different sound formulas (the medium sets a rest frame)解释为何波源运动与观察者运动给出不同声波公式(介质设定静止参考系)
- Use $\Delta f/f \approx \Delta\lambda/\lambda \approx v/c$ for light at $v \ll c$对 $v \ll c$ 的光用 $\Delta f/f \approx \Delta\lambda/\lambda \approx v/c$
- Distinguish redshift from blueshift and link each to recession or approach区分红移与蓝移并各自对应远离或接近
- State that the distance-dependent redshift of galaxies is evidence for an expanding universe说明星系随距离增大的红移是宇宙膨胀的证据
- Apply the factor-of-2 reflected-wave shift to a radar speed gun, ultrasound or sonar problem将因子 2 的反射波频移用于雷达测速、超声或声呐问题
- Describe how Doppler ultrasound measures blood-flow speed from the echo off moving red cells描述多普勒超声如何由运动红细胞回波测血流速度
IB Paper-Style PracticeIB 试卷风格练习
C.5 Practice and Solutions are on the roadmap, to ship under Practice Questions/Unit_C5_*.html with the bilingual built-in pattern.
C.5 配套 Practice 与 Solutions 在排期,上线后位于 Practice Questions/Unit_C5_*.html。