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Question: Because of pressure and temperature difference the refractive index of air varies with height $h$ as...

Because of pressure and temperature difference the refractive index of air varies with height hh as μ=μ01+(106)h\mu = \mu_0\sqrt{1+(10^{-6})h}. There is a point object placed on surface, the maximum horizontal distance of the observer at height 4m is able to see it is dd km

A

The angle with horizontal the point object will be seen by observer is θ=tan1(102)\theta = \tan^{-1}(10^{-2}) rad.

B

d=4d = 4 km

C

Horizontal distance of point on trajectory is 2 km for height of 1 m

D

Equation is trajectory is hyperbolic in nature

Answer

B, C

Explanation

Solution

The problem describes the variation of the refractive index of air with height hh as μ=μ01+(106)h\mu = \mu_0\sqrt{1+(10^{-6})h}. We need to analyze the path of light rays and determine the maximum horizontal distance an observer at a certain height can see an object on the surface.

1. Principle of Light Ray Propagation in a Stratified Medium:

For a light ray propagating in a medium where the refractive index μ\mu varies only with height hh, Snell's law in differential form implies that the quantity μcosθ\mu \cos \theta remains constant, where θ\theta is the angle the ray makes with the horizontal. Let the light ray start from the object placed on the surface (h=0h=0) with an initial angle θ0\theta_0 with the horizontal. So, μ(h)cosθ=μ0cosθ0\mu(h) \cos \theta = \mu_0 \cos \theta_0.

2. Condition for Maximum Horizontal Distance:

To achieve the maximum horizontal distance for an observer at height HH to see an object on the surface, the light ray must be launched from the object at the smallest possible angle with the horizontal, effectively tangent to the surface. This means θ00\theta_0 \to 0, so cosθ01\cos \theta_0 \to 1. Under this condition, the constant becomes μ0\mu_0. Thus, the relation for the ray that defines the maximum horizontal distance is: μ01+(106)hcosθ=μ0\mu_0\sqrt{1+(10^{-6})h} \cos \theta = \mu_0 cosθ=11+(106)h\cos \theta = \frac{1}{\sqrt{1+(10^{-6})h}}

3. Trajectory of the Light Ray:

The horizontal distance xx traversed by the ray for a vertical change dhdh is given by dx=dhtanθdx = \frac{dh}{\tan \theta}. First, let's find tanθ\tan \theta: sin2θ=1cos2θ=111+(106)h=1+(106)h11+(106)h=(106)h1+(106)h\sin^2 \theta = 1 - \cos^2 \theta = 1 - \frac{1}{1+(10^{-6})h} = \frac{1+(10^{-6})h - 1}{1+(10^{-6})h} = \frac{(10^{-6})h}{1+(10^{-6})h} tanθ=sinθcosθ=(106)h1+(106)h11+(106)h=(106)h\tan \theta = \frac{\sin \theta}{\cos \theta} = \frac{\sqrt{\frac{(10^{-6})h}{1+(10^{-6})h}}}{\frac{1}{\sqrt{1+(10^{-6})h}}} = \sqrt{(10^{-6})h}

Now, substitute tanθ\tan \theta into the dxdx equation: dx=dh(106)h=1106dhh=103h1/2dhdx = \frac{dh}{\sqrt{(10^{-6})h}} = \frac{1}{\sqrt{10^{-6}}} \frac{dh}{\sqrt{h}} = 10^3 h^{-1/2} dh

To find the horizontal distance xx for a given height hh, we integrate from 00 to hh: x=0h103h1/2dh=103[h1/21/2]0h=103[2h]0h=2×103hx = \int_0^h 10^3 h'^{-1/2} dh' = 10^3 \left[ \frac{h'^{1/2}}{1/2} \right]_0^h = 10^3 [2\sqrt{h'}]_0^h = 2 \times 10^3 \sqrt{h} So, the equation of the trajectory is x=2×103hx = 2 \times 10^3 \sqrt{h}.

4. Evaluating the Options:

A. The angle with horizontal the point object will be seen by observer is θ=tan1(102)\theta = \tan^{-1}(10^{-2}) rad. The observer is at height H=4H=4m. The angle θ\theta is the angle the ray makes with the horizontal at the observer's position. Using tanθ=(106)h\tan \theta = \sqrt{(10^{-6})h} and h=4h=4m: tanθ=(106)×4=4×106=2×103\tan \theta = \sqrt{(10^{-6}) \times 4} = \sqrt{4 \times 10^{-6}} = 2 \times 10^{-3} So, θ=tan1(2×103)\theta = \tan^{-1}(2 \times 10^{-3}) rad. Since 2×103=0.0022 \times 10^{-3} = 0.002 and 102=0.0110^{-2} = 0.01, option A is incorrect.

B. d=4d = 4 km dd is the maximum horizontal distance when the observer is at height H=4H=4m. Using the trajectory equation x=2×103hx = 2 \times 10^3 \sqrt{h}, set h=4h=4m: d=2×1034=2×103×2=4×103d = 2 \times 10^3 \sqrt{4} = 2 \times 10^3 \times 2 = 4 \times 10^3 meters =4= 4 km. So, option B is correct.

C. Horizontal distance of point on trajectory is 2 km for height of 1 m Using the trajectory equation x=2×103hx = 2 \times 10^3 \sqrt{h}, set h=1h=1m: x=2×1031=2×103x = 2 \times 10^3 \sqrt{1} = 2 \times 10^3 meters =2= 2 km. So, option C is correct.

D. Equation is trajectory is hyperbolic in nature The equation of the trajectory is x=2×103hx = 2 \times 10^3 \sqrt{h}. Squaring both sides, we get x2=(2×103)2h=4×106hx^2 = (2 \times 10^3)^2 h = 4 \times 10^6 h. Rearranging, h=14×106x2h = \frac{1}{4 \times 10^6} x^2. This is of the form y=ax2y = ax^2, which represents a parabola, not a hyperbola. So, option D is incorrect.

The final answer is B,C\boxed{B, C}

Explanation of the solution:

  1. Snell's Law for Varying Refractive Index: For light traveling in a medium where refractive index μ\mu varies only with height hh, the quantity μcosθ\mu \cos \theta (where θ\theta is the angle with the horizontal) remains constant.

  2. Maximum Horizontal Distance: To achieve the maximum horizontal distance for an observer at height HH to see an object on the ground, the light ray must be launched from the object horizontally (θ00\theta_0 \approx 0^\circ). This makes the constant μ0cos0=μ0\mu_0 \cos 0^\circ = \mu_0.

  3. Ray Path Equation: From μcosθ=μ0\mu \cos \theta = \mu_0, substitute μ=μ01+(106)h\mu = \mu_0\sqrt{1+(10^{-6})h} to get cosθ=11+(106)h\cos \theta = \frac{1}{\sqrt{1+(10^{-6})h}}.

  4. Differential Horizontal Distance: The change in horizontal distance dxdx for a change in height dhdh is dx=dhtanθdx = \frac{dh}{\tan \theta}. Using tanθ=1cos2θ1=1+(106)h1=(106)h\tan \theta = \sqrt{\frac{1}{\cos^2 \theta} - 1} = \sqrt{1+(10^{-6})h - 1} = \sqrt{(10^{-6})h}.

  5. Integration for Trajectory: Integrate dx=dh(106)h=103h1/2dhdx = \frac{dh}{\sqrt{(10^{-6})h}} = 10^3 h^{-1/2} dh from 00 to hh to get the trajectory equation x=2×103hx = 2 \times 10^3 \sqrt{h}.

  6. Verify Options:

    • A (Angle): At h=4h=4m, tanθ=(106)×4=2×103\tan \theta = \sqrt{(10^{-6}) \times 4} = 2 \times 10^{-3}. So θ=tan1(2×103)\theta = \tan^{-1}(2 \times 10^{-3}), not tan1(102)\tan^{-1}(10^{-2}). Incorrect.
    • B (Distance dd): For H=4H=4m, d=2×1034=4×103d = 2 \times 10^3 \sqrt{4} = 4 \times 10^3 m =4= 4 km. Correct.
    • C (Distance at 1m): For h=1h=1m, x=2×1031=2×103x = 2 \times 10^3 \sqrt{1} = 2 \times 10^3 m =2= 2 km. Correct.
    • D (Trajectory Type): Squaring x=2×103hx = 2 \times 10^3 \sqrt{h} gives x2=4×106hx^2 = 4 \times 10^6 h, or h=14×106x2h = \frac{1}{4 \times 10^6} x^2. This is a parabolic equation (y=ax2y=ax^2). Incorrect.

Answer: The correct options are B and C.