Skip to content
  • Home
  • Categories
    • Geology
    • Geography
    • Space and Astronomy
  • About
    • Privacy Policy
  • About
  • Privacy Policy
Our Planet TodayAnswers for geologist, scientists, spacecraft operators
  • Home
  • Categories
    • Geology
    • Geography
    • Space and Astronomy
  • About
    • Privacy Policy
on September 21, 2023

Which part of solar radiation (VIS, NIR) keeps Earth warm?

Solar Terrestrial Physics

Contents:

  • Understanding Solar Radiation and its Effect on the Earth’s Temperature
  • Absorption and Transmission of Solar Radiation
  • The Greenhouse Effect and the Regulation of the Earth’s Temperature
  • The Importance of Visible and Near-Infrared Radiation to the Earth’s Climate
  • FAQs

Understanding Solar Radiation and its Effect on the Earth’s Temperature

Solar radiation plays a critical role in determining Earth’s temperature and sustaining life on our planet. The Sun emits a wide range of electromagnetic radiation, including visible (VIS) and near-infrared (NIR) wavelengths. However, not all parts of solar radiation contribute equally to the Earth’s heating. In this article, we will explore which part of solar radiation, between VIS and NIR, primarily keeps the Earth warm, shedding light on the fascinating field of solar terrestrial physics and Earth science.

Absorption and Transmission of Solar Radiation

Solar radiation is composed of different wavelengths that interact differently with the Earth’s atmosphere, surface, and various components. When solar radiation reaches the Earth, it encounters the atmosphere, which acts as a filter and modifies the incoming radiation. The atmosphere consists of gases such as nitrogen, oxygen, carbon dioxide, and water vapor, and particles such as aerosols and clouds.
Visible (VIS) radiation refers to the portion of solar radiation that can be perceived by the human eye. It includes wavelengths from about 400 to 700 nanometers. VIS radiation is critical to life on Earth, fueling photosynthesis in plants and providing the illumination we rely on. When VIS radiation interacts with the atmosphere, some is absorbed by gases and particles, while the rest reaches the Earth’s surface.

Near-infrared (NIR) radiation, on the other hand, consists of wavelengths from about 700 to 2,500 nanometers. NIR radiation is not visible to the human eye, but it has important implications for the Earth’s energy balance. Unlike VIS radiation, NIR radiation is less affected by atmospheric gases and particles. As a result, a significant portion of NIR radiation reaches the Earth’s surface, where it interacts with land, oceans, and vegetation.

The Greenhouse Effect and the Regulation of the Earth’s Temperature

To understand what part of the sun’s radiation primarily keeps the Earth warm, we need to look at the greenhouse effect. The greenhouse effect is a natural process that regulates the Earth’s temperature by trapping some of the radiation that is emitted. When solar radiation reaches the Earth’s surface, it is absorbed and re-emitted as heat radiation in the form of infrared (IR) radiation.

The atmosphere contains greenhouse gases, including water vapor, carbon dioxide (CO2), methane (CH4), and others. These gases have a remarkable ability to absorb and re-emit IR radiation. In particular, CO2 and water vapor are the most important greenhouse gases. They create a “blanket” in the atmosphere that traps some of the outgoing IR radiation, preventing it from escaping back into space. This trapped energy is then re-radiated in all directions, including back to the Earth’s surface.
In this context, NIR radiation plays an important role in keeping the Earth warm. While a significant portion of VIS radiation is absorbed by the atmosphere and surface, NIR radiation is less affected by these interactions. It can more easily penetrate the atmosphere and reach the Earth’s surface, where it is absorbed by land, oceans, and vegetation. This absorption causes these components to heat up, contributing to the overall warming of the planet.

The Importance of Visible and Near-Infrared Radiation to the Earth’s Climate

Both VIS and NIR radiation are important to the Earth’s climate system, but in different ways. VIS radiation is critical for photosynthesis, which allows plants to grow and sustain ecosystems. It also plays a role in the Earth’s energy balance by directly heating the surface. However, a significant amount of VIS radiation is reflected back into space by clouds, aerosols, and the Earth’s surface itself. This reflected radiation reduces the amount of energy absorbed by the Earth, thereby regulating its temperature.
NIR radiation, on the other hand, contributes to the warming of the Earth’s surface. As mentioned earlier, NIR radiation can penetrate the atmosphere more effectively than VIS radiation. It is less susceptible to scattering and absorption by atmospheric gases and particles. As a result, more of the NIR radiation reaches the surface where it is absorbed and converted to heat. This energy transfer helps maintain the Earth’s temperature, making NIR radiation a critical component of the planet’s overall energy budget.

In summary, while both visible (VIS) and near-infrared (NIR) radiation from the Sun are important to Earth’s climate and energy balance, NIR radiation is primarily responsible for keeping Earth warm. Its ability to penetrate the atmosphere, interact less with atmospheric gases and particles, and be absorbed by the Earth’s surface contributes significantly to the overall temperature of the planet. By understanding the complex interactions between solar radiation and the Earth’s atmosphere, scientists can gain valuable insights into climate dynamics and improve our understanding of the delicate balance that sustains life on our planet.

FAQs

Which part of solar radiation (VIS, NIR) keeps Earth warm?

The part of solar radiation that keeps Earth warm is primarily in the form of infrared (NIR) radiation.

What is visible (VIS) radiation?

Visible (VIS) radiation refers to the portion of the electromagnetic spectrum that is visible to the human eye. It consists of different wavelengths of light that range from violet to red.

What is near-infrared (NIR) radiation?

Near-infrared (NIR) radiation is a part of the electromagnetic spectrum that has wavelengths slightly longer than visible light. It is not visible to the human eye but can be detected by certain instruments. NIR radiation carries heat energy and is responsible for warming the Earth’s surface.

How does solar radiation warm the Earth?

Solar radiation warms the Earth through a process called the greenhouse effect. When sunlight reaches the Earth’s atmosphere, a portion of it is absorbed by the surface of the Earth, including land, oceans, and vegetation. The absorbed sunlight is then re-emitted in the form of longer-wavelength infrared radiation (NIR). Greenhouse gases in the atmosphere, such as carbon dioxide and water vapor, trap some of this outgoing radiation, preventing it from escaping into space. This trapped energy heats up the Earth’s surface and the lower atmosphere, contributing to the overall warming of the planet.

Why is infrared (NIR) radiation important for Earth’s climate?

Infrared (NIR) radiation is crucial for Earth’s climate because it plays a vital role in maintaining the planet’s temperature. Without NIR radiation, the Earth would be much colder, making it inhospitable for life as we know it. The greenhouse effect, driven by the absorption and re-emission of NIR radiation, helps regulate the Earth’s temperature and creates a habitable environment.



Is visible (VIS) radiation responsible for Earth’s warming?

Visible (VIS) radiation contributes to the overall energy input from the Sun, but it is not primarily responsible for Earth’s warming. While visible light is absorbed by various objects on Earth’s surface, it is the subsequent re-emission of this energy as infrared (NIR) radiation that retains heat and warms the planet. The majority of the Sun’s energy that reaches the Earth is in the form of NIR radiation.

Recent

  • Exploring the Geological Features of Caves: A Comprehensive Guide
  • What Factors Contribute to Stronger Winds?
  • The Scarcity of Minerals: Unraveling the Mysteries of the Earth’s Crust
  • How Faster-Moving Hurricanes May Intensify More Rapidly
  • Adiabatic lapse rate
  • Exploring the Feasibility of Controlled Fractional Crystallization on the Lunar Surface
  • The Greenhouse Effect: How Rising Atmospheric CO2 Drives Global Warming
  • Examining the Feasibility of a Water-Covered Terrestrial Surface
  • What is an aurora called when viewed from space?
  • Measuring the Greenhouse Effect: A Systematic Approach to Quantifying Back Radiation from Atmospheric Carbon Dioxide
  • Asymmetric Solar Activity Patterns Across Hemispheres
  • Unraveling the Distinction: GFS Analysis vs. GFS Forecast Data
  • The Role of Longwave Radiation in Ocean Warming under Climate Change
  • Esker vs. Kame vs. Drumlin – what’s the difference?

Categories

  • English
  • Deutsch
  • Français
  • Home
  • About
  • Privacy Policy

Copyright Our Planet Today 2025

We use cookies on our website to give you the most relevant experience by remembering your preferences and repeat visits. By clicking “Accept”, you consent to the use of ALL the cookies.
Do not sell my personal information.
Cookie SettingsAccept
Manage consent

Privacy Overview

This website uses cookies to improve your experience while you navigate through the website. Out of these, the cookies that are categorized as necessary are stored on your browser as they are essential for the working of basic functionalities of the website. We also use third-party cookies that help us analyze and understand how you use this website. These cookies will be stored in your browser only with your consent. You also have the option to opt-out of these cookies. But opting out of some of these cookies may affect your browsing experience.
Necessary
Always Enabled
Necessary cookies are absolutely essential for the website to function properly. These cookies ensure basic functionalities and security features of the website, anonymously.
CookieDurationDescription
cookielawinfo-checkbox-analytics11 monthsThis cookie is set by GDPR Cookie Consent plugin. The cookie is used to store the user consent for the cookies in the category "Analytics".
cookielawinfo-checkbox-functional11 monthsThe cookie is set by GDPR cookie consent to record the user consent for the cookies in the category "Functional".
cookielawinfo-checkbox-necessary11 monthsThis cookie is set by GDPR Cookie Consent plugin. The cookies is used to store the user consent for the cookies in the category "Necessary".
cookielawinfo-checkbox-others11 monthsThis cookie is set by GDPR Cookie Consent plugin. The cookie is used to store the user consent for the cookies in the category "Other.
cookielawinfo-checkbox-performance11 monthsThis cookie is set by GDPR Cookie Consent plugin. The cookie is used to store the user consent for the cookies in the category "Performance".
viewed_cookie_policy11 monthsThe cookie is set by the GDPR Cookie Consent plugin and is used to store whether or not user has consented to the use of cookies. It does not store any personal data.
Functional
Functional cookies help to perform certain functionalities like sharing the content of the website on social media platforms, collect feedbacks, and other third-party features.
Performance
Performance cookies are used to understand and analyze the key performance indexes of the website which helps in delivering a better user experience for the visitors.
Analytics
Analytical cookies are used to understand how visitors interact with the website. These cookies help provide information on metrics the number of visitors, bounce rate, traffic source, etc.
Advertisement
Advertisement cookies are used to provide visitors with relevant ads and marketing campaigns. These cookies track visitors across websites and collect information to provide customized ads.
Others
Other uncategorized cookies are those that are being analyzed and have not been classified into a category as yet.
SAVE & ACCEPT