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638 nm Red Light: Understanding Visible Electromagnetic Waves | 638纳米红光:认识可见电磁波

2026-08-05 06:38 · 本文部分内容由AI辅助创作

📚 638 nm Red Light: Understanding Visible Electromagnetic Waves | 638纳米红光:认识可见电磁波

Light with a wavelength of 638 nanometres sits right at the red end of the visible spectrum. This particular wavelength is commonly produced by red laser diodes and high-brightness LEDs, making it a familiar sight in barcode scanners, optical fibre communications and laser pointers. Understanding 638 nm red light helps IGCSE students master core ideas about waves, the electromagnetic spectrum, energy calculations and real-world applications.

波长为638纳米的光位于可见光谱的红色末端。这一特定波长通常由红色激光二极管和高亮度发光二极管产生,因此在条形码扫描器、光纤通信和激光指示器中随处可见。理解638纳米红光有助于IGCSE学生掌握关于波、电磁波谱、能量计算和实际应用的核心概念。


1. What is 638 nm Red Light? | 什么是638纳米红光?

avelength is the distance between two consecutive crests of a wave. Because it falls between roughly 620 nm and 750 nm, our eyes perceive it as a deep red colour. In the physics laboratory, a helium-neon laser often emits light at 632.8 nm, which is very close to 638 nm, so many textbook examples essentially use similar values.

数字638纳米告诉我们这种光的波长:638 × 10⁻⁹ 米。波长是波的两个相邻波峰之间的距离。由于它大约落在620纳米到750纳米之间,我们的眼睛将其感知为深红色。在物理实验室中,氦氖激光器常常发出632.8纳米的光,非常接近638纳米,因此许多教材示例实际上使用了类似的数值。

The shorter the wavelength within the visible band, the more the light shifts towards violet; the longer the wavelength, the more it shifts towards red. 638 nm therefore represents one of the longest wavelengths we can still see as a pure colour before entering the invisible infrared region.

在可见光波段内,波长越短,光越偏向紫色;波长越长,光越偏向红色。因此,638纳米代表我们在进入不可见的红外区域之前,仍然能作为一种纯粹颜色看到的最长波长之一。


2. The Electromagnetic Spectrum and Visible Light | 电磁波谱与可见光

rum arranges these waves by wavelength or frequency, from radio waves with kilometres-long wavelengths to gamma rays with wavelengths smaller than an atomic nucleus. Visible light occupies only a tiny slice from about 380 nm to 750 nm.

所有电磁波在真空中都以光速 c = 3.00 × 10⁸ m/s 传播。电磁波谱按照波长或频率将这些波排列起来,从波长几千米的无线电波到波长比原子核还小的伽马射线。可见光只占据从大约380纳米到750纳米的很小一段。

is is lower than the frequency of green or blue light, which is why red light carries less energy per photon.

在这一段中,638纳米红光位于可见光范围的长波长、低频率一端。它的频率可以用波动方程计算:f = c ÷ λ。代入 λ = 638 × 10⁻⁹ m 得到 f ≈ 4.70 × 10¹⁴ Hz。这个频率低于绿光或蓝光的频率,因此红光每个光子携带的能量较少。


3. The Wave Equation: Speed, Frequency and Wavelength | 波动方程:速度、频率与波长的关系

central to IGCSE physics and is used routinely to switch between frequency and wavelength.

对于任何波,速度 v、频率 f 和波长 λ 之间的关系由波动方程给出。对于真空中的电磁波,这就变成了 c = f λ。这个方程是IGCSE物理的核心,经常用于在频率和波长之间进行转换。

c = f × λ

his calculation in reverse when given the frequency of red light to find its wavelength, reinforcing their algebraic manipulation skills.

如果我们知道 λ = 638 nm = 6.38 × 10⁻⁷ m,那么 f = c / λ = (3.00 × 10⁸) / (6.38 × 10⁻⁷) ≈ 4.70 × 10¹⁴ Hz。学生经常在给出红光频率时反过来进行这个计算以求出波长,这加强了他们的代数处理能力。

Knowing that red light has a longer wavelength than blue light helps explain why radio telescopes are huge — they observe even longer wavelengths — and why blu-ray technology can store more data by using the shorter wavelength of a blue laser.

了解红光比蓝光波长更长,有助于解释为什么射电望远镜如此巨大——它们观测的是更长的波长——以及为什么蓝光技术可以利用蓝色激光较短的波长存储更多数据。


4. Photon Energy of Red Light | 红光的光子能量

a stream of photons. The energy E of a single photon is linked to its frequency by Planck's equation: E = h f, where h is Planck's constant, 6.63 × 10⁻³⁴ J·s.

E = h × f

about 1.95 eV. This relatively low photon energy explains why red light is less likely to cause photochemical damage than ultraviolet light, which has a much higher frequency and photon energy.

对于我们的638纳米红光,f 约等于 4.70 × 10¹⁴ Hz。乘以 h 得到 E = 6.63 × 10⁻³⁴ × 4.70 × 10¹⁴ ≈ 3.12 × 10⁻¹⁹ J。用电子伏特表示约为 1.95 eV。这种相对较低的光子能量解释了为什么红光比紫外线更不容易引起光化学损伤,紫外线具有高得多的频率和光子能量。

IGCSE Science students may not always need to calculate photon energy, but the concept is useful when comparing different parts of the spectrum. It also underpins the operation of photoelectric devices: a red photon may not have enough energy to eject electrons from certain metals, whereas a blue or ultraviolet photon often does.

IGCSE科学的学生也许不总是需要计算光子能量,但这一概念在比较光谱不同部分时很有用。它也是光电器件工作的基础:一个红色光子可能没有足够的能量从某些金属中打出电子,而蓝色或紫外光子则常常可以。


5. Sources of Red Light | 红光的来源

There are several common sources that produce light around 638 nm. Red laser diodes, such as those found in DVD players and laser pointers, emit a very narrow band of wavelengths centred near 638–650 nm. High-brightness red LEDs made from aluminium gallium arsenide (AlGaAs) also peak in this region. Incandescent bulbs emit a broad spectrum that includes red, but they are inefficient compared to LEDs.

有几种常见的光源可以产生大约638纳米的光。红光激光二极管,例如DVD播放机和激光指示器中的那些,发射出以638–650纳米为中心的极窄波段。由铝镓砷化物(AlGaAs)制成的高亮度红色发光二极管也在该区域达到峰值。白炽灯泡发出包含红光在内的宽广光谱,但与LED相比效率较低。

In the laboratory, students can isolate red light by passing white light through a red filter or by using a prism to disperse light and selecting the red portion. The ability to produce and manipulate specific wavelengths is fundamental to optical experiments at IGCSE level.

在实验室里,学生可以通过让白光通过红色滤光片,或者使用棱镜将光色散并选择红色部分来分离出红光。产生并操控特定波长的能力是IGCSE阶段光学实验的基础。


6. Everyday Applications of Red Light | 红光在日常生活中的应用

Red light at 638 nm and nearby wavelengths has numerous practical uses. Barcode scanners in supermarkets often use a red laser because the light is highly visible, can be focused into a fine spot, and is safe for consumer use. Optical fibre communication systems sometimes use red lasers due to low absorption in certain types of plastic fibre, allowing data to travel short distances reliably.

638纳米及其附近波长的红光有许多实际用途。超市里的条形码扫描器常常使用红色激光,因为这种光非常显眼、可以聚焦成极小的光点,并且对消费者使用是安全的。光纤通信系统有时使用红色激光,因为在某些类型的塑料光纤中吸收较低,使数据能够在短距离内可靠传输。

Red light-emitting diodes are used in television remote controls, indicator lights, and bicycle rear lamps. In art galleries and museums, red lighting is often employed to protect sensitive pigments because red photons carry less energy and are less likely to break chemical bonds than blue or ultraviolet light.

红色发光二极管用于电视遥控器、指示灯和自行车尾灯。在美术馆和博物馆中,经常采用红色照明来保护敏感的颜料,因为红色光子携带的能量较少,与蓝色或紫外光相比,打断化学键的可能性更小。


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7. Red Light in Biology and Medicine | 红光在生物学与医学中的应用

In biology, red light plays a key role in photosynthesis. Chlorophyll absorbs strongly in the blue and red parts of the spectrum but reflects green, which is why plants appear green. The absorption peak near 660 nm means that 638 nm light can be effectively used by plants to drive the light-dependent reactions of photosynthesis.

在生物学中,红光在光合作用里扮演关键角色。叶绿素在光谱的蓝光和红光部分吸收强烈,但反射绿光,这就是植物呈现绿色的原因。其吸收峰在660纳米附近,这意味着638纳米的光可以被植物有效地用来驱动光合作用的光反应阶段。

Medical therapies also make use of red light. Low-level laser therapy (LLLT) using wavelengths around 630–670 nm is employed to promote wound healing, reduce inflammation and relieve pain. The relatively low photon energy allows deep tissue penetration without causing thermal damage.

医学治疗也利用了红光。使用630–670纳米波长的低强度激光疗法(LLLT)被用于促进伤口愈合、减轻炎症和缓解疼痛。相对较低的光子能量可以深入组织而不会造成热损伤。


8. Comparing Red Light with Blue Light | 红光与蓝光的比较

Comparing 638 nm red light with 450 nm blue light highlights several important wave properties. Red light has a longer wavelength, lower frequency, and lower photon energy. Blue light has a shorter wavelength, higher frequency, and higher photon energy. The table below summarises the contrast.

将638纳米红光与450纳米蓝光进行比较,可以突显几个重要的波的性质。红光波长更长、频率更低、光子能量更小。蓝光波长更短、频率更高、光子能量更大。下表总结了这一对比。

PropertyRed Light (638 nm)Blue Light (450 nm)
Wavelength (m)6.38 × 10⁻⁷4.50 × 10⁻⁷
Frequency (Hz)4.70 × 10¹⁴6.67 × 10¹⁴
Photon energy (J)3.12 × 10⁻¹⁹4.42 × 10⁻¹⁹
Diffraction spreadingGreaterSmaller

Because red light diffracts more around obstacles, it is less suitable for reading extremely fine details in optical discs, which is why Blu-ray uses a shorter-wavelength blue laser to store more data on the same-sized disc.

由于红光在障碍物周围衍射更多,它不太适合读取光盘上极其微小的细节,这就是为什么蓝光光盘使用波长更短的蓝色激光在同样尺寸的光盘上存储更多数据。


9. Diffraction and Interference of Red Light | 红光的衍射与干涉

Diffraction is the spreading of waves when they pass through a gap or around an obstacle. The amount of diffraction increases with wavelength. Red light, having a relatively long wavelength, diffracts more noticeably than blue light. This can be demonstrated by shining a red laser through a narrow slit and observing the broad central maximum on a screen.

衍射是波通过狭缝或绕过障碍物时扩散开来的现象。衍射量随着波长的增加而增加。红光具有相对较长的波长,其衍射比蓝光更明显。这可以用红色激光照射狭缝并在屏幕上观察宽阔的中央亮纹来演示。

where w is fringe spacing, D is the slit-to-screen distance, and s is the slit separation.

当红光通过双缝时,会产生明暗相间的干涉条纹。条纹间距与波长成正比,因此红光产生的条纹间距比蓝光更宽。这一行为由方程 w = λD / s 描述,其中 w 是条纹间距,D 是缝到屏幕的距离,s 是缝间距。

w = λD ÷ s

This relationship allows students to determine an experimental value for the wavelength of red light, connecting practical skills with wave theory.

这一关系使学生可以通过实验测定红光的波长数值,将实践技能与波动理论联系起来。


10. Measuring Wavelength with a Diffraction Grating | 用衍射光栅测量波长

ction grating. The grating equation is n λ = d sin θ, where n is the order number (1, 2, 3… lines on the grating, and θ is the angle of diffraction measured from the central maximum.

n λ = d sin θ

≈ 3.33 × 10⁻⁶ × 0.191 ≈ 6.36 × 10⁻⁷ m = 636 nm, which closely matches the expected 638 nm.

在学校的实验室里,使用衍射光栅是更精确测量红光波长的方法。光栅方程为 n λ = d sin θ,其中 n 是级数(1, 2, 3…),λ 是波长,d 是光栅相邻刻线间的距离,θ 是从中央极大测量的衍射角。典型的光栅每毫米可能有300条刻线,由此得出 d = 1/300 mm = 3.33 × 10⁻⁶ m。用红色激光照射光栅,测量一级亮斑的角度 θ,学生就能计算出 λ。如果测得 n = 1 时 θ = 11.0°,则 λ = d sin θ = 3.33 × 10⁻⁶ × sin 11.0° ≈ 3.33 × 10⁻⁶ × 0.191 ≈ 6.36 × 10⁻⁷ m = 636 nm,非常接近预期的638纳米。

This experiment consolidates understanding of wave optics, trigonometry, and the nature of light. It also provides a memorable numerical link to the label "638".

这个实验巩固了对波动光学、三角学以及光本质的理解,也提供了一个令人难忘的与数字“638”联系起来的数值结果。


11. Safety and Precautions with Red Lasers | 红色激光的安全与注意事项

Although red lasers emitting 638 nm light are generally low-power, safety must be a priority. Direct eye exposure can cause retinal damage because the lens of the eye focuses the laser beam onto a tiny spot on the retina. IGCSE students should always follow laboratory rules: never point a laser at anyone, avoid reflective surfaces, and use a laser warning sign. Even low-power Class 2 lasers, which rely on the blink reflex for protection, should be treated with care.

虽然发射638纳米光的红色激光通常功率较低,但安全必须放在首位。直接照射眼睛会导致视网膜损伤,因为眼睛的晶状体将激光束聚焦到视网膜上的一个微小光点。IGCSE学生应始终遵守实验室规则:切勿将激光对准任何人,避开反射表面,并使用激光警告标志。即便是依赖眨眼反射来保护的2类低功率激光器,也应当小心对待。

Red high-brightness LEDs are generally safer than lasers, but they can still cause discomfort if viewed at close range for extended periods. Good experimental practice includes securing all optical components on optical benches and keeping the beam path below eye level.

高亮度红色LED通常比激光更安全,但如果长时间近距离注视仍会引起不适。良好的实验操作包括将所有光学元件固定于光具座上,并保持光束路径低于眼睛水平。


12. Why 638 nm Matters in Science Education | 为什么638纳米在科学教育中重要

umber. It is a gateway to understanding the entire electromagnetic spectrum, the dual wave– ch as c = f λ and E = h f with hands-on experiments using diffraction gratings and lasers.

638纳米这个波长不仅仅是一个数字。它是理解整个电磁波谱、光的波粒二象性、能量量子化以及光子学实际世界的一扇大门。它将 c = f λ 和 E = h f 这些理论概念与使用衍射光栅和激光器的动手实验联系起来。

By looking closely at red light, students gain a deeper appreciation of why the sky is blue, why sunsets appear red, and how technology harnesses specific wavelengths for communication, medicine and data storage. The journey from a simple three-digit figure to a full wave model exemplifies the spirit of IGCSE Science.

通过仔细研究红光,学生能更深刻地理解为什么天空是蓝色的、为什么日落呈现红色,以及科技如何利用特定波长进行通信、医疗和数据存储。从一个简单的三位数字到完整的波动模型,这一历程体现了IGCSE科学的探索精神。


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