Industry-relevant training in Business, Technology, and Design to help professionals and graduates upskill for real-world careers.
Fun, engaging games to boost memory, math fluency, typing speed, and English skills—perfect for learners of all ages.
Enroll to start learning
You’ve not yet enrolled in this course. Please enroll for free to listen to audio lessons, classroom podcasts and take practice test.
Listen to a student-teacher conversation explaining the topic in a relatable way.
Good morning, class! Today we're going to explore how electromagnetic radiation interacts with our atmosphere and earth's surfaces. Can anyone tell me what they think happens when light hits a surface?
It probably bounces off, right?
That's right! That's called reflection. EMR can also scatter, get absorbed, or be transmitted. Let's dive deeper into these interactions. Remember the acronym STAR which stands for Scattering, Transmission, Absorption, and Reflection.
Could you explain scattering a bit more?
Of course! Scattering can diffuse incident radiation in all directions. This occurs especially when the surface is rough compared to EMR's wavelength. Can anyone think of an example of scattering in nature?
The blue sky is an example, right?
Exactly! That’s because of Rayleigh scattering, which scatters shorter wavelengths of light more than longer ones. Let's summarize what we discussed today: EMR can interact with surfaces in four ways—reflection, scattering, absorption, and transmission.
Last time, we talked about various interactions of EMR. Now, let's focus on reflection. What do you think matters most for reflection to occur?
I think it's about how smooth the surface is?
Exactly right! Smooth surfaces will reflect EMR more predictably. On the flip side, absorption occurs when EMR is taken up by materials. Why is this important in remote sensing?
Because it can change how much light we can capture in images?
Great insight! It's important for understanding features in satellite images. Let's remember—light can be reflected, absorbed, or transmitted by different materials.
Today we will delve deeper into scattering. Can anyone name the three types of scattering we discussed?
Rayleigh scattering, Mie scattering, and Non-selective scattering!
Awesome! Each type has specific conditions under which it occurs. For instance, Rayleigh scattering occurs with gas molecules in the atmosphere. How does it affect our perception of color?
It makes the sky look blue because it scatters blue light more!
That's correct! That’s why when we see the sunset, we often see reds and oranges instead. The sunlight takes a longer path through the atmosphere, scattering more of the shorter wavelengths. So remember, the scattering effects are pivotal in understanding satellite image clarity.
As we wrap up our exploration of EMR interactions, why do you think these interactions are crucial for remote sensing data interpretation?
Because they influence how we see and analyze data from satellites!
Exactly! Understanding how EMR interacts with the atmosphere helps us improve our image processing techniques. And why would knowing about scattering help in enhancing image quality?
It helps in correcting the blurring that occurs due to scattering!
You all are fantastic! So in summary, the interactions of EMR—reflection, absorption, transmission, and scattering are all critical for reliable remote sensing applications.
Read a summary of the section's main ideas. Choose from Basic, Medium, or Detailed.
The section elaborates on the four main types of interactions (scattering, absorption, transmission, and reflection) of EMR with the atmosphere and earth's surface. Each interaction depends on factors such as the angle of incident radiation and atmospheric conditions, affecting satellite images' quality.
When electromagnetic radiation (EMR) strikes materials or objects on the ground, it undergoes several interactions before being captured by sensors. This section identifies and explains four primary types of interactions that occur with both the atmosphere and the earth's surface: reflection, absorption, transmission, and scattering.
These interactions depend on various factors, including the angle of incident radiation, wavelength of the radiation, and atmospheric conditions. As EMR travels, it first interacts with the atmosphere, then with the objects on the ground, and finally returns to the atmosphere again before reaching satellite sensors. Each interaction plays a significant role in determining the quality and accuracy of satellite images.
Dive deep into the subject with an immersive audiobook experience.
Signup and Enroll to the course for listening the Audio Book
When EMR strikes a material/object on the ground, it is called incident radiation. This incident radiation will first interact with atmosphere and then on the surface of Earth, and then again with atmosphere before it reaches the sensor. Four types of interactions will take place with the atmosphere and surface/objects; scattering, absorption, transmission and reflection.
This chunk introduces the concept of incident radiation, which refers to electromagnetic radiation (EMR) that reaches the Earth. When this radiation interacts with both the atmosphere and the surface of the Earth, it can do so in four distinct ways: scattering, absorption, transmission, and reflection. Each of these interactions can significantly affect the quality and usability of remotely sensed images. For example, scattering tends to blur objects and reduce image clarity.
Think of tossing a ball at a wall. The way the ball behaves when it hits the wall (bouncing back, getting absorbed, or passing through cracks) is similar to how EMR interacts with materials in nature.
Signup and Enroll to the course for listening the Audio Book
It is the process whereby incident radiation bounces-off the surface in a single predictable direction. Reflection is caused by the surfaces that are smooth relative to the wavelengths of incident radiation. As per Snell’s law, the angle of reflection is always equal and opposite to the angle of incidence.
Reflection occurs when incoming electromagnetic radiation hits a smooth surface and bounces back in a predictable direction. For instance, if light hits a calm pond or a mirror, it reflects back. This reflection is governed by Snell’s law, which states that the angle at which the light hits the surface (angle of incidence) is equal to the angle at which it reflects away (angle of reflection). The amount of energy that reflects back depends on factors like surface material and atmospheric conditions.
Imagine looking into a mirror. The way you see your reflection back at you is much like how EMR reflects off smooth surfaces on the Earth, such as water or glass, allowing sensors to capture clear images.
Signup and Enroll to the course for listening the Audio Book
It is the process by which small particles diffuse a portion of the incident radiation in all directions. Scattering occurs when incident radiation is dispersed or spread out unpredictably in different directions. Scattering of radiation by the constituent gases and aerosols in the atmosphere causes degradation of remotely sensed images.
Scattering happens when small particles in the atmosphere, such as dust or water droplets, cause the incident radiation to spread in multiple directions rather than reflecting back in a straight line. This can lead to loss of detail in remotely sensed images as blurring can obscure the features that the sensor is trying to detect. In practice, this results in images that can be less sharp and harder to interpret.
Consider a foggy day. Just as the fog scatters light, making it difficult to see clearly, scattering in the atmosphere creates similar challenges for satellites trying to capture clear images of the Earth.
Signup and Enroll to the course for listening the Audio Book
Three types of scattering commonly take place in the atmosphere: Rayleigh scattering, Mie scattering and Non-selective scattering. These will depend on the wavelength of incident radiant energy, and the size of gas molecule, dust particle, and/or water vapor droplet interacting with the EMR.
There are three main types of scattering: Rayleigh scattering, Mie scattering, and non-selective scattering. Rayleigh scattering occurs when particles are much smaller than the wavelength of radiation (like gases in the atmosphere), and it causes shorter wavelengths (like blue light) to scatter more. Mie scattering occurs with particles similar in size to the wavelength and affects both longer and shorter wavelengths. Non-selective scattering involves larger particles that scatter all wavelengths equally. Each type of scattering impacts how energy is perceived by sensors.
Imagine throwing different-sized balls (particles) at a net (wavelength). Small balls slip through easily (Rayleigh), medium balls get stuck in the net more evenly (Mie), while large balls won't fit and just bounce around (non-selective). Each size interacts differently with light, affecting how we perceive colors in the sky.
Signup and Enroll to the course for listening the Audio Book
Rayleigh scattering mainly consists of scattering from the gases present in the atmosphere. It is primarily caused by air particles i.e., O and N molecules. Rayleigh scattering takes place when the dimension of the particles present in the atmosphere is much smaller than the size of wavelength λ, and can be represented as: Rayleigh scattering ꭀ 1 / λ4.
Rayleigh scattering happens when gas molecules in the atmosphere scatter shorter wavelengths of light (like blue) more than longer wavelengths (like red). This is why the sky appears blue during the day—blue light is scattered in all directions while red light continues straight through. The intensity of this scattering is inversely related to the fourth power of the wavelength, meaning the shorter the wavelength, the stronger the scattering effect. This principle affects both how we see the sky and how satellite sensors gather data.
Think of a prism dispersing light into a rainbow. Just as the prism separates colors based on their wavelengths, Rayleigh scattering causes different colors of light to scatter differently in the atmosphere, making the sky appear blue instead of red during the day.
Learn essential terms and foundational ideas that form the basis of the topic.
Key Concepts
Scattering: The diffusion of EMR in many directions due to particles.
Reflection: The predictable bouncing of EMR off surfaces.
Absorption: The uptake of EMR by materials, leading to energy conversion.
Transmission: Passing of certain EMR wavelengths through materials.
See how the concepts apply in real-world scenarios to understand their practical implications.
Example of reflection is how sunlight reflects off a calm body of water, showing the sky's colors.
An example of scattering is the blue color of the sky caused by Rayleigh scattering of sunlight.
Use mnemonics, acronyms, or visual cues to help remember key information more easily.
When sunlight hits a surface that's smooth, it reflects light in a way that's smooth.
Imagine throwing a ball against a wall. If it hits smoothly, it bounces straight back like light reflecting, but if it hits unevenly, it scatters everywhere!
S.A.R.T. helps you remember: Scattering, Absorption, Reflection, Transmission.
Review key concepts with flashcards.
Review the Definitions for terms.
Term: Electromagnetic Radiation (EMR)
Definition:
A form of energy that is propagated as waves through space and can interact with matter.
Term: Reflection
Definition:
The bouncing back of incident radiation from a surface at a predictable angle.
Term: Scattering
Definition:
The diffusion of incident radiation in multiple directions, often caused by particles in the atmosphere.
Term: Absorption
Definition:
The process by which materials take in EMR and convert it into other forms of energy.
Term: Transmission
Definition:
The process by which certain wavelengths of radiation pass through the atmosphere or surface materials.