diff options
Diffstat (limited to '3769/CH19')
-rw-r--r-- | 3769/CH19/EX19.1/Ex19_1.sce | 12 | ||||
-rw-r--r-- | 3769/CH19/EX19.10/Ex19_10.sce | 13 | ||||
-rw-r--r-- | 3769/CH19/EX19.11/Ex19_11.sce | 13 | ||||
-rw-r--r-- | 3769/CH19/EX19.14/Ex19_14.sce | 19 | ||||
-rw-r--r-- | 3769/CH19/EX19.16/Ex19_16.sce | 10 | ||||
-rw-r--r-- | 3769/CH19/EX19.17/Ex19_17.sce | 12 | ||||
-rw-r--r-- | 3769/CH19/EX19.18/Ex19_18.sce | 16 | ||||
-rw-r--r-- | 3769/CH19/EX19.19/Ex19_19.sce | 11 | ||||
-rw-r--r-- | 3769/CH19/EX19.2/Ex19_2.sce | 12 | ||||
-rw-r--r-- | 3769/CH19/EX19.21/Ex19_21.sce | 17 | ||||
-rw-r--r-- | 3769/CH19/EX19.3/Ex19_3.sce | 10 | ||||
-rw-r--r-- | 3769/CH19/EX19.4/Ex19_4.sce | 12 | ||||
-rw-r--r-- | 3769/CH19/EX19.5/Ex19_5.sce | 13 | ||||
-rw-r--r-- | 3769/CH19/EX19.6/Ex19_6.sce | 13 | ||||
-rw-r--r-- | 3769/CH19/EX19.7/Ex19_7.sce | 11 | ||||
-rw-r--r-- | 3769/CH19/EX19.8/Ex19_8.sce | 13 |
16 files changed, 207 insertions, 0 deletions
diff --git a/3769/CH19/EX19.1/Ex19_1.sce b/3769/CH19/EX19.1/Ex19_1.sce new file mode 100644 index 000000000..5d2f30967 --- /dev/null +++ b/3769/CH19/EX19.1/Ex19_1.sce @@ -0,0 +1,12 @@ +clear +//Given +v=-75.0 +u=0 + +//Calculation +f=v +P=100/f + +//Result +printf("\n Focal length is %0.3f cm", f) +printf("\n Power of the lens is %0.2f D",P) diff --git a/3769/CH19/EX19.10/Ex19_10.sce b/3769/CH19/EX19.10/Ex19_10.sce new file mode 100644 index 000000000..afaeeb0cb --- /dev/null +++ b/3769/CH19/EX19.10/Ex19_10.sce @@ -0,0 +1,13 @@ +clear +//Given +f=4.80 //cm +a=1.20 +v=-24.0 //cm + +//Calculation +D=f/(a-1) +u=1/((1/v)-1/f) + +//Result +printf("\n (i) The least distance of distinct vision is %0.3f cm",D) +printf("\n (ii) Distance from the lens is %0.3f cm",-u) diff --git a/3769/CH19/EX19.11/Ex19_11.sce b/3769/CH19/EX19.11/Ex19_11.sce new file mode 100644 index 000000000..3a5887b9e --- /dev/null +++ b/3769/CH19/EX19.11/Ex19_11.sce @@ -0,0 +1,13 @@ +clear +//Given +v0=15.0 //cm +f0=3.0 //cm +D=25 +fe=9 + +//Calculation +u0=1/((1/v0)-1/f0) +M=-(v0*D)/(u0*fe) + +//Result +printf("\n Magnifying power is %0.1f ",M) diff --git a/3769/CH19/EX19.14/Ex19_14.sce b/3769/CH19/EX19.14/Ex19_14.sce new file mode 100644 index 000000000..003b84bb6 --- /dev/null +++ b/3769/CH19/EX19.14/Ex19_14.sce @@ -0,0 +1,19 @@ +clear +//Given +f0=1.0 +u0=-1.1 //cm +D=25 +fe=5.0 +ve=25.0 + +//Calculation +v0=1/((1/f0)+1/u0) +d=v0+fe +M=-(v0*D)/(u0*fe) +ue=-1/((1/ve)+1/fe) +D1=v0-ue +M1=-(v0/u0)*(1+(D/fe)) + +//Result +printf("\n (i) Distance between the lenses when image is at infinity %0.3f cm", d) +printf("\n (ii) Distance between the lenses when image is at distinct vision %0.2f cm",D1) diff --git a/3769/CH19/EX19.16/Ex19_16.sce b/3769/CH19/EX19.16/Ex19_16.sce new file mode 100644 index 000000000..0fc93b8bf --- /dev/null +++ b/3769/CH19/EX19.16/Ex19_16.sce @@ -0,0 +1,10 @@ +clear +//Given +fe=3 +M=4 + +//Calculation +f0=fe*M + +//Result +printf("\n Focal length of the lenses is %0.3f cm and %0.3f cm",f0,fe) diff --git a/3769/CH19/EX19.17/Ex19_17.sce b/3769/CH19/EX19.17/Ex19_17.sce new file mode 100644 index 000000000..d4c1cb5f5 --- /dev/null +++ b/3769/CH19/EX19.17/Ex19_17.sce @@ -0,0 +1,12 @@ +clear +//Given +u0=-200.0 //cm +f0=30.0 //cm +fe=3 + +//Calculation +v0=1/((1/f0)+1/u0) +a=v0+fe + +//Result +printf("\n Separation between the objective and eyepiece is %0.1f cm",a) diff --git a/3769/CH19/EX19.18/Ex19_18.sce b/3769/CH19/EX19.18/Ex19_18.sce new file mode 100644 index 000000000..ac6d5335b --- /dev/null +++ b/3769/CH19/EX19.18/Ex19_18.sce @@ -0,0 +1,16 @@ +clear +//Given +ve=24.0 +fe=8.0 +f0=250.0 +a=10 + +//Calculation +ue=1/((1/ve)-(1/fe)) +D=f0-ue +d=a/2.0 +A=d/f0 + +//Result +printf("\n (i) Distance between objective and eyepiece is %0.3f cm", D) +printf("\n (ii) Angle subtended by the sun at the objective is %0.3f rad",A) diff --git a/3769/CH19/EX19.19/Ex19_19.sce b/3769/CH19/EX19.19/Ex19_19.sce new file mode 100644 index 000000000..33b016880 --- /dev/null +++ b/3769/CH19/EX19.19/Ex19_19.sce @@ -0,0 +1,11 @@ +clear +//Given +M=-20 +R=-120 + +//Calculation +f0=R/2.0 +fe=f0/M + +//Result +printf("\n Focal length of eyepiece is %0.3f cm", fe) diff --git a/3769/CH19/EX19.2/Ex19_2.sce b/3769/CH19/EX19.2/Ex19_2.sce new file mode 100644 index 000000000..9088b85ea --- /dev/null +++ b/3769/CH19/EX19.2/Ex19_2.sce @@ -0,0 +1,12 @@ +clear +//Given +u=-25.0 //cm +v=-150.0 //cm + +//Calculation +f=1/((1/v)-1/u) +P=100/f + +//Result +printf("\n Focal length of the lens is %0.3f cm", f) +printf("\n Power of the lens is %0.2f D",P) diff --git a/3769/CH19/EX19.21/Ex19_21.sce b/3769/CH19/EX19.21/Ex19_21.sce new file mode 100644 index 000000000..8b5ae5fcd --- /dev/null +++ b/3769/CH19/EX19.21/Ex19_21.sce @@ -0,0 +1,17 @@ +clear +//Given +u0=-200.0 //cm +fa=50.0 //cm +ve=-25.0 //cm +fe=5.0 //cm + +//Calculation +v0=1/((1/fa)+1/u0) +M0=v0/u0 +ue=1/((1/ve)-1/fe) +Me=ve/ue +D=v0-ue +M=M0*Me + +//Result +printf("\n (i) Saparation between the objective and eyepiece is %0.2f cm",D) diff --git a/3769/CH19/EX19.3/Ex19_3.sce b/3769/CH19/EX19.3/Ex19_3.sce new file mode 100644 index 000000000..7cf6928a6 --- /dev/null +++ b/3769/CH19/EX19.3/Ex19_3.sce @@ -0,0 +1,10 @@ +clear +//Given +u=-25.0 //cm +v=-50.0 //cm + +//Calculation +f=1/((1/v)-1/u) + +//Result +printf("\n Focal length is %0.3f cm", f) diff --git a/3769/CH19/EX19.4/Ex19_4.sce b/3769/CH19/EX19.4/Ex19_4.sce new file mode 100644 index 000000000..3e0565e7d --- /dev/null +++ b/3769/CH19/EX19.4/Ex19_4.sce @@ -0,0 +1,12 @@ +clear +//Given +v=-80.0 //cm + +//Calculation +f=v +P=100/f + +//Result +printf("\n (a) Power of the lens is %0.3f D", P) +printf("\n (b) No the corrective lens is concave and it reduces the size of the image. Because it bring the object at the far point of the eye") +printf("\n (c) The myopic person may have a normal near point. He must keep the book at a distance greater than 25 cm.") diff --git a/3769/CH19/EX19.5/Ex19_5.sce b/3769/CH19/EX19.5/Ex19_5.sce new file mode 100644 index 000000000..a4d222fb6 --- /dev/null +++ b/3769/CH19/EX19.5/Ex19_5.sce @@ -0,0 +1,13 @@ +clear +//Given +v=-75.0 //cm +u=-25.0 //cm + +//Calculation +f=1/((1/v)-1/u) +P=100/f + +//Result +printf("\n (a) Power of the lens is %0.2f D",P) +printf("\n (b) The corrective lens produce a virtual imageof an object at 25 cm. The angular size of this image is the same as the object") +printf("\n (c) A hypermetropic eye may have normal far point.Hence the person prefers not to use the spectacles for distant object") diff --git a/3769/CH19/EX19.6/Ex19_6.sce b/3769/CH19/EX19.6/Ex19_6.sce new file mode 100644 index 000000000..f43a29f24 --- /dev/null +++ b/3769/CH19/EX19.6/Ex19_6.sce @@ -0,0 +1,13 @@ +clear +//Given +P=-0.8 //d +v1=-15.0 //cm +v2=-100.0 //cm + +//Calculation +f=100/P +u1=1/((1/v1)-1/f) +u2=1/((1/v2)-(1/f)) + +//Result +printf("\n The person can see objects lying between %0.0f cm and %0.3f cm",-u1,-u2) diff --git a/3769/CH19/EX19.7/Ex19_7.sce b/3769/CH19/EX19.7/Ex19_7.sce new file mode 100644 index 000000000..3c431a3d6 --- /dev/null +++ b/3769/CH19/EX19.7/Ex19_7.sce @@ -0,0 +1,11 @@ +clear +//Given +u=-25 //cm +p=3.0 + +//Calculation +f=100/p +v=1/((1/f)+1/u) + +//Result +printf("\n Distance is %0.0f m",v) diff --git a/3769/CH19/EX19.8/Ex19_8.sce b/3769/CH19/EX19.8/Ex19_8.sce new file mode 100644 index 000000000..bd0c37ffd --- /dev/null +++ b/3769/CH19/EX19.8/Ex19_8.sce @@ -0,0 +1,13 @@ +clear +//Given +u=-25.0 //cm +v=-90.0 //cm + +//calculation +f=1/((1/v)-1/u) +f1=(1/2.0)*10**2 +u=1/((1/v)-1/f1) + +//Result +printf("\n (i) focal length is %0.1f cm",f) +printf("\n (ii) Distance is %0.1f cm",u) |