Wednesday, 24 April 2013

Sky Wave or Ionospheric propagation

Sky Wave or Ionospheric propagation

The ionosphere is the upper portion of the atmosphere, which absorbs large quantities of radiant energy like ultra violet rays, cosmic rays etc., from the sun, becoming heated and ionised. This ionised region contains free electrons, positive and negative ions.

Radio waves in the short wave band, radiated from an antenna at large angles with ground, travel through the atmosphere and encounters the ionised region in the upper atmosphere, Under favourable circumstances, the radiowaves get bent downwards due to refraction from the different parts of the ionised region and again reach the earth at a fer distant point. Such a radio wave is called the sky wave and such a propagation of radio wave is known as sky wave propagation or ionospheric propagation. Long distance radio communication is thus possible through the sky wave propagation.

Monday, 22 April 2013

Nuclear fusion

Nuclear fusion

Nuclear fusion is a process in which two or more lighter nuclei combine to form a heavier nucleus. the mass of the product is always less than the sum of masses of the individual lighter nuclei. The difference in mass is converted into energy. The fusion process can be carried out only at a extremely high temperature of the ode of 107 K because, only at these very high temperatures the nuclei are able to overcome their mutual repulsion. Therefore before fusion, the lighter nuclei must have their temperature raised by several million degrees. The nuclear fusion reactions are known as thermo-nuclear reactions.

Saturday, 6 April 2013

Colours of thin films

Colours of thin films

Everyone is familiar with the brilliant colours exhibited by a thin oil film spread on the surface of water and also by a soap bubble. These colours are due to interference between light waves reflected from the top and bottom surfaces of thin filims. When white light is incident on a thin film, the film appers coloured and the colour depends upon the thickness of the film and also the angle of incidence of the light.

Saturday, 16 March 2013

Uses of Polaroid

Uses of Polaroid

  1. Polaroids are used in the laboratory to produce and analyse plane polarised light.
  2. Polaroids are widely used as polarising sun glasses.
  3. They are used to eliminate the head light glare in motor cars.
  4. They are used to improve colour contrasts in old oil paintings.
  5. polaroid films are used to produce three-dimensonal moving pictures.
  6. They are used as glass windows in trains and aeroplanes to control the intensity of light. In aeroplane one polaroid is fixed outside the window while the other is fitted inside which can be rotated. The intensity of light can be adjusted by rotating the inner polaroid.
  7. Aerial pictures may be taken from slightly different angles and when viewed through polaroids give a better perception of depth.
  8. In calculators and watches, letters and numbers are formed by liquid crystal display(LCD) through polarisation of light.
  9. Polarisation is also used to study size and shape of molecules.  

Friday, 8 March 2013

Types of Crystals

Types of Crystals

Crystals like calcite, quartz, ice and tourmaline having only one optic axis are called uniaxial crystals.

Crystals like mica, topaz, selenite and aragonite having two optic axes are called biaxial crystals

Monday, 4 March 2013

Polarisation

Polarisation

The phenomena of reflection, refraction, interference, diffraction are common to both transverse waves and longitudinal waves. But the transverse nature of light waves is demonstrated only by the phenomenon of polarisation.

Sunday, 24 February 2013

Fluoresence


Fluoresence

When an atomic or molecular system is excited into higher energy state by absorption of energy, it returns back to lower energy state in a time less than 10-5 second and the system is found to glow brightly by 
emitting radiation of longer wavelength.

When ultra violet is incident on certain substance, they emit visible light.

It may be noted that fluorescence exists as long as the fluorescing substance remain exposed to incident ultraviolet light and re-emission of light stops as soon as incident light is cut off.