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  • Snell's Law: Understanding Refraction in Physics - Definition & Formula
    The tangent law in physics, also known as Snell's law or the law of refraction, describes the relationship between the angles of incidence and refraction when a wave traveling in one medium strikes a boundary with a second medium and is partially reflected and partially transmitted. It can be mathematically expressed as:

    ```

    n1 * sin(θ1) = n2 * sin(θ2)

    ```

    Where:

    - n1 and n2 are the refractive indices of the first and second medium, respectively.

    - θ1 is the angle of incidence.

    - θ2 is the angle of refraction.

    When light travels from a rarer medium (lower refractive index) to a denser medium (higher refractive index), the refracted ray bends towards the normal (straight line perpendicular to the interface). Conversely, when light travels from a denser to a rarer medium, the refracted ray bends away from the normal.

    The tangent law demonstrates the change in the direction of the wave as it passes from one medium to another. As a result, light rays traveling from air into water appear to bend downwards, while rays traveling from water into air appear to bend upwards. This concept underpins the working principles of optical devices like lenses and prisms.

    The tangent law finds applications in diverse fields, including optics, telecommunications, seismology, and more. It facilitates the understanding and analysis of light refraction, reflection, propagation, and interference phenomena. Engineers, scientists, and researchers employ the tangent law to design devices and systems that involve precise control and manipulation of light and other waves.

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