Skip to main content

Basic of Remote Sensing II

Remote Sensing Process



A. Energy Source or Illumination – the first requirement is to have an energy source which illuminates or provides electromagnetic energy to the target of interest.
B. Radiation and the Atmosphere – as the energy travels from its source to the target, it will come in contact with and interact with the atmosphere it passes through. This interaction may take place a second time as the energy travels from the target to the sensor.
C. Interaction with the Target – once the energy makes its way to the target through the atmosphere, it interacts with the target depending on the properties of both the target and the radiation.
D. Recording of Energy by the Sensor – after the energy has been scattered by, or emitted from the target, we require a sensor to collect and record the EMR.
E. Transmission, Reception, Processing – the energy recorded by the sensor has to be transmitted, often in electronic form, to receiving and processing station where the data are processed into an image.
F. Interpretation and Analysis – the processed image is interpreted, visually and/or digitally or electronically, to extract information about the target which was illuminated.
G. Application – the final element of the remote sensing process is achieved when we apply the information we have been able to extract from the imagery about the target in order to better understand it, reveal some new information, or assist in solving a particular problem.

Remote Sensing Principle
Electromagnetic energy reaching the Earth’s surface from the Sun is reflected, transmitted or absorbed.
Specific targets/ objects have individual and characteristic manner of interacting with incident radiation that is described by the spectral response of that target.
Eg. – soils of different types, water with varying degrees of impurities or vegetation of various species.
EMR like radio waves, IR waves make characteristic patterns as they travel through space. Each wave has a certain shape and length. The distance between peaks is called wavelength.
The light which our eyes (our remote sensors) – can detect is part of the VISIBLE SPECTRUM. The visible wavelengths cover a range from approximately 0.4 to 0.7 µm; (1 µm = 1*10-6 of a meter).

Wavelength, Frequency, Amplitude
The EMS ranges from the shorter wavelengths (including gamma & X-rays) to the longer wavelengths (including MWs & RWs).
There are several regions of the EMS which are useful for Remote Sensing.


Electro Magnetic Spectrum

Comments

Popular posts from this blog

Basic of Remote Sensing III

Contents Advantages Limitations Applications Advantages of Remote Sensing : Provides a synoptic view over a large region; Offers Geo-referenced information and digital information; Most of the remote sensors operate in every season, every day, every time and even in tough weather; Limitations : Can be expensive; Can be technically difficult; Not direct; Measure surrogate variables e.g. reflectance (%), brightness temperature, backscatter; Applications of Remote Sensing Urban & Regional Planning Scope: Mapping & updation of city/town maps  Urban sprawl monitoring Town planning Facility management  GIS database development Benefits: Better decision support, planning & management Rapid information updation Infrastructure development monitoring Spatial information analysis Agriculture Scope: Crop acreage estimation Crop modeling for yield & production forecast / estimation Crop & Orchard monitoring Soil sensing ...

Basic of Remote Sensing IV

Sources of Electromagnetic Energy There are three main sources of  electromagnetic radiation that are used in  remote sensing:  Solar radiation (natural radiation from the  sun)  Terrestrial radiation (natural radiation  emitted by Earth's surface)  Artificial radiation (from a remote sensing  system) Solar Radiation The Sun yields a continuous spectrum of EM  energy. This Incident radiation can be reflected  from the Earth's surface. This process produces a large amount of  short wavelength energy (from 0.4 - 0.7 µm;  blue, green, and red light). It can also be emitted by the Earth's  surface. Such emitted radiation is typically  of a longer wavelength, in the middle and  far infra-red wavelengths. Interacts with the atmosphere and surface  materials (reflect, absorb).  Since the Sun has a much higher temperature  (6000 degrees K) than the Earth (303 degrees  K), so t...

Basic of Remote Sensing V

How is Energy Transferred? The energy can be transferred in the three basic ways: conduction, convection, and radiation. The transfer of energy by electromagnetic radiation (EMR) is of primary interest to remote sensing because it is the only form of energy transfer that can take place in a vacuum (the region between the Sun and the Earth). The Sun bathes the Earth’s surface with radiant energy causing the air near the ground to increase in temperature. The less dense air rises, creating convectional currents in the atmosphere. Energy may be conducted directly from one object to another as when a pan is in direct physical contact with a hot burner. Energy Interactions When Electro-Magnetic (EM) energy is incident on any given earth surface feature, three fundamental energy interactions are possible.  Reflection (ER) Absorption (EA) Transmission (ET) Incident Energy (EI) = reflected energy +  transmitted energy + absorbed energy Three forms...