Physics Times 07.2019

(Kiana) #1
tan
H

B
B

 tan^0
H 2

ni
B
r


 


0


(^2) tan tan

 
  
 
i r BH K
n
 i Ktan
Where K is called as T.G. constant (or) reduction
factor of T.G., r-radius of the coil in meter;
BH Horizontal component of earth’s magnetic
field in tesla;
icurrent in amperes



  1. Deflection Magnetometer
    (I)Tan A position : In this position the
    magnetometer is set perpendicular to magnetic
    meridian so that, magnetic field due to magnet,
    is in axial position and perpendicular to earth’s
    field.
    18. Magnetic Susceptibility


0
2 2 2

2
tan.
H 4 ( )

M r
B
r l




 

0
3
tan.^2
H 4
B M
r

 
 (r>>l)
(II)Tan B position : The arms of magnetometer
are set in magnetic meridian, so that the
magnetic field due to magnet is at its equatorial
position,


  1. Relative permeability


0
Htan 4 .( 2 2 3/2)
B M
r l

 




0
Htan 4. 3
B M
r

 




(r>>l)

(III) Comparison of magnetic moments :

According to deflection method

1 1
2 2

tan
tan

M
M




According to null deflection method

3
1 1
2 2

M d
M d

 
 
 



  1. Magnetic Field Intensity (^) (H)
    
     The force experienced by unit north pole of one
    weber is called magnetic field strength or intensity
    of magnetic field strength. i.e., H = F / m
     SI unit : Am^1 or weber




  2. Intensity of Magnetisation(I)




 
 

2
2

M m l m
I
V A l A

  

Where m = pole strength; M= Magnetic moment
a = area of cross-section of the magnet;
V=Volume of the magnet
SI unit : Am^1

 

I
H



It has no units


  1. Magnetic permeability  


i.e.,

B
H



 It is a scalar having unit Hm^1
 r

0

r
 

 It has no units and dimensions


  1. Relation between r and 


As



  1. Deflection Magnetometer
    16. Magnetic Field Intensity




  1. Intensity of Magnetisation(I)

  2. Magnetic Susceptibility

  3. Magnetic permeability




  1. Relative permeability




  1. Relation between and

  2. Curie’s Law:


0

r
 
^   r  ^1 


  1. Curie’s Law:
    It states that intensity of magnetisation (I) and
    hence  are inversely proportional to the absolute
    temperature (T)


i.e.,

C
T

 where C- Curie constant
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