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JEE Main 2019
LEVELJEE Advanced

Animated Solution for Physics - Electromagnetic Waves: The electric field of a plane polarised electromagnetic wave in free space at time is given by an expression. The magnetic field is given by (where, is the velocity of light)

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Visualized Solution

The Sigma Insight: Characteristics of Electromagnetic Waves

Solution Diagram

Analyzing the Setup

Imagine you are standing in free space, observing an electromagnetic wave passing by. The problem gives us the electric field of this wave: .
This single equation is packed with information. First, the amplitude of the electric field, , is .
Second, the tells us that the electric field is oscillating strictly along the y-axis.
But the real treasure lies inside the cosine function. The term is the spatial phase of the wave, which dictates how the wave is oriented in space.

Extracting the Wave Vector

From the spatial phase , we can immediately write down the wave vector, .
The coefficients of and give us the components of this vector. So, .
This vector points exactly in the direction the wave is traveling. Let's find its magnitude, .
Using the Pythagorean theorem, .
Now, we know that for any electromagnetic wave in free space, the angular frequency is related to the wave number by the speed of light .
The master relation is .
Substituting our value of , we get .
With this, we can construct the complete time-dependent phase of the wave. Since it's a forward-traveling wave, the phase is , which becomes .

The Magnetic Field Direction

Now comes the most thrilling part: finding the magnetic field!
In an electromagnetic wave, the electric field , the magnetic field , and the direction of propagation are locked in a perfectly perpendicular dance.
The direction of the magnetic field is always given by the cross product: .
Let's set up this cross product carefully. The unit vector of propagation is . The direction of the electric field is .
So, .
Distributing the cross product, we use the standard right-hand rule for unit vectors: and .
This gives us .

Final Calculation

We have the direction, and we have the phase. All we need now is the amplitude of the magnetic field, .
In free space, the amplitudes are related by .
Since , we find that .
Finally, let's assemble the complete magnetic field vector. We multiply the amplitude, the direction unit vector, and the cosine phase together.
The in the numerator and denominator beautifully cancel out, leaving us with our final, elegant expression:
And there we have it! A perfect match with option (b).

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