Question map
With reference to the Earth's atmosphere, which one of the following statements is correct?
Explanation
The correct answer is Option 3.
The Earth's atmosphere is transparent to shortwave solar radiation but opaque to longwave terrestrial radiation. Water vapour, concentrated primarily in the troposphere (lower atmosphere), acts as a potent greenhouse gas. It possesses high absorption bands for infrared radiation, trapping heat and maintaining the Earth's thermal balance. This process is crucial for the greenhouse effect.
Other options are incorrect because:
- Option 1: Insolation at the equator is roughly 2.4 times (not 10 times) that at the poles.
- Option 2: Infrared radiation accounts for approximately 45-50% of the total solar spectrum, while visible light accounts for about 40%; thus, it is not two-thirds.
- Option 4: Infrared waves are not part of the visible spectrum; they have longer wavelengths and are located beyond the red end of the visible light range in the electromagnetic spectrum.
PROVENANCE & STUDY PATTERN
Full viewThis is a classic 'NCERT Fundamental' check, specifically targeting the confusion between Incoming Solar Radiation (Insolation) and Outgoing Terrestrial Radiation. It combines concepts from Chapter 7 (Composition) and Chapter 8 (Heat Budget) of Class XI Physical Geography. The trap lies in mixing up the properties of Shortwave (Solar) and Longwave (Terrestrial) radiation.
This question can be broken into the following sub-statements. Tap a statement sentence to jump into its detailed analysis.
- Statement 1: In the context of Earth's atmosphere, is the total solar insolation received at the equator roughly ten times the insolation received at the poles?
- Statement 2: In the context of Earth's atmosphere, do infrared rays constitute roughly two-thirds of the incoming solar radiation (insolation)?
- Statement 3: In Earth's atmosphere, are infrared waves largely absorbed by atmospheric water vapour?
- Statement 4: In Earth's atmosphere, is atmospheric water vapour concentrated in the lower atmosphere (the troposphere)?
- Statement 5: In the context of Earth's atmosphere and solar radiation, are infrared waves part of the visible spectrum of electromagnetic radiation?
- Explicitly states that total insolation by latitude "does not vary a great deal", which argues against a large (β10Γ) difference.
- Notes curvature is important but implies latitudinal differences are moderate rather than an order-of-magnitude.
- States equator gets more intense sunlight but gives a concrete example at 60Β°N where the sun "heats a given parcel of ground with only a half", implying roughly ~2Γ differences in intensity at mid-latitudes rather than ~10Γ.
- Supports the view that differences are substantial but not order-of-magnitude.
- Notes simply that "The amount of insolation decreases from the equator towards the poles," confirming a gradient but giving no support for a 10Γ factor.
- Provides general confirmation of latitudinal decrease but no large-magnitude claim.
Gives actual measured surface insolation ranges: ~320 W/mΒ² in the tropics and ~70 W/mΒ² in the poles, showing a multiβfold difference between low and high latitudes.
A student can compare these numbers (320 vs 70 W/mΒ² β ~4.6Γ) with the claimed 10Γ ratio to judge that the claim seems larger than the values cited.
States the general geometric rule that energy per unit area decreases from equator to poles because rays are direct at the equator and increasingly oblique toward poles.
Combine this geometric rule with the cosine (angle) effect from basic geometry or a world map to estimate relative insolation at different latitudes and check plausibility of a 10Γ factor.
Explains that at the equator solar rays are concentrated while near the poles they are spread over a larger area and pass through more atmosphere, both reducing polar insolation.
Use the two effects (area spreading + longer atmospheric path) together with simple trigonometry or known latitude differences to estimate how much weaker polar insolation should be.
Gives the average incoming solar radiation at the top of the atmosphere (1.94 cal/cmΒ²/min β solar constant at TOA), providing a baseline before atmospheric attenuation.
A student can compare TOA values with surface values (from other snippets) to see how atmospheric losses alter latitudinal contrasts and whether a 10Γ surface ratio is feasible.
Describes latitudinal patterns of net radiation (surplus in tropics, deficit near poles), confirming systematic decrease poleward though not giving exact multipliers.
Use this qualitative pattern plus quantitative surface numbers (snippet 1) to infer that while poles receive markedly less, the difference is on the order of a few times rather than an order of magnitude.
States that the Earth's surface receives most of its energy in short wavelengths and defines insolation as incoming solar radiation.
A student could combine this with a standard solar spectrum (or TOA spectral fractions) to judge whether infrared could be as large as two-thirds if most energy is shortwave.
Says the atmosphere is largely transparent to short-wave solar radiation and that tropospheric gases absorb much of the near-infrared.
Use the note that shortwave predominates at TOA but near-IR is partially absorbed in the atmosphere to estimate the split between visible/UV and IR in incoming solar energy.
Explicitly lists the Sun's radiation components as visible, ultraviolet and infrared and notes a substantial fraction (~35%) is reflected back from atmosphere/particles.
Combine the qualitative component list and the reflected fraction with external spectral data (e.g., solar spectral irradiance) to infer the fraction of incoming energy in infrared.
States Earth receives solar radiation in the form of short waves (visible and ultraviolet), implying incoming solar energy is dominated by shortwave rather than longwave/IR.
A student could take this rule and compare it to known percent distributions of solar spectrum to test whether IR can plausibly be two-thirds.
Notes water vapour absorbs not only outgoing long-wave terrestrial radiation but also part of incoming short-wave (visible and UV), implying some incoming energy in near-IR/shortwave is absorbed in atmosphere.
Use this to refine an estimate of how much incoming IR is removed before reaching surface versus how much of total insolation is IR at TOA.
- Explicitly says water vapour in the troposphere absorbs much of the near-infrared radiation.
- Places the absorption process within the atmospheric layer where most water vapour resides (troposphere).
- States water vapour absorbs long-wave terrestrial radiation (infrared/heat emitted by the Earth).
- Links water vapour with the insulating/greenhouse action that retains emitted infrared energy.
- Affirms that water vapour absorbs both incoming and outgoing radiation, implicating infrared in Earth's heat budget.
- Identifies water vapour as crucial to atmospheric radiative processes that govern heat retention.
- Explicitly quantifies that the vast majority of atmospheric moisture is close to the surface (90% within ~6 km).
- Directly supports the idea that water vapour is concentrated in the lower atmosphere.
- States that the troposphere contains the bulk of all water vapour, clouds and weather.
- Identifies the troposphere as the primary layer for atmospheric moisture, linking moisture concentration to this lower layer.
- Asserts that water vapour decreases with altitude, implying higher concentrations near the surface.
- Provides regional percentage context while confirming the vertical decline of moisture.
- Separates visible 'white' light from less visible ultraviolet and infra-red, implying infra-red is not part of the visible band.
- Presents infra-red as a distinct, less visible component of solar radiation.
- Defines insolation as short waves (UV and visible) and contrasts these with terrestrial longwave (infrared).
- Explicitly treats infrared as longwave radiation distinct from the visible shortwave band.
- States the Earth emits energy as infrared at wavelengths longer than the incoming solar energy.
- Identifies infrared with longer wavelengths, distinguishing it from shorter-wavelength visible solar radiation.
- Bullet 1. [THE VERDICT]: Sitter. Directly solvable from NCERT Class XI Fundamentals of Physical Geography (Chapter 8: Solar Radiation & Chapter 7: Composition).
- Bullet 2. [THE CONCEPTUAL TRIGGER]: The 'Heat Budget' and 'Atmospheric Circulation'. Specifically, the mechanism of the Greenhouse Effect (how atmosphere is transparent to insolation but opaque to terrestrial radiation).
- Bullet 3. [THE HORIZONTAL EXPANSION]: Memorize the 'Radiation Rules': 1) Solar = Shortwave (Visible/UV), Terrestrial = Longwave (IR). 2) Insolation Ratio: Equator (~320 W/mΒ²) is roughly 4x Poles (~70 W/mΒ²), not 10x. 3) Water Vapour Profile: 90% is within 6km of surface (Troposphere). 4) Albedo: Earth reflects ~30-35% (Clouds are the biggest reflector).
- Bullet 4. [THE STRATEGIC METACOGNITION]: When reading about 'Absorption', always ask: 'Absorbs WHAT?' Ozone absorbs UV (incoming); Water Vapour/CO2 absorb IR (outgoing/terrestrial). The exam traps you by swapping these targets.
Insolation per unit area decreases from equator to poles because solar rays become more oblique, are spread over a larger surface, and traverse more atmosphere at high latitudes.
High-yield for explaining temperature gradients, climate zones and poleward heat redistribution; connects to questions on latitude controls of climate, isotherms and seasonal contrasts. Mastering this helps answer comparative reasoning and cause-effect questions on temperature and radiation.
- Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 18: Latitudes and Longitudes > Temperature Falls as We Move From The Equator Towards The Poles > p. 242
- Exploring Society:India and Beyond ,Social Science-Class VII . NCERT(Revised ed 2025) > Chapter 3: Climates of India > a) Latitude > p. 49
Surface insolation magnitudes show that tropical values (~320 W/m2) are only a few times larger than polar values (~70 W/m2), not an order-of-magnitude higher.
Enables quantitative evaluation of claims about relative radiation (e.g., refuting exaggerated ratios); links to heat budget, energy balance and regional climate comparisons β useful for data-based reasoning and numerical options in UPSC geography questions.
- FUNDAMENTALS OF PHYSICAL GEOGRAPHY, Geography Class XI (NCERT 2025 ed.) > Chapter 8: Solar Radiation, Heat Balance and Temperature > Spatial Distribution of Insolation at the Earth's Surface > p. 68
The incoming solar flux at the top of the atmosphere (~1.94 cal/cm2/min or ~1350 W/m2) is reduced before reaching the surface by reflection and absorption, so TOA values differ from surface insolation.
Critical for separating top-of-atmosphere figures from surface measurements in questions on energy budgets, solar energy potential and climate forcing; helps avoid mixing global constants with surface-level comparisons.
- FUNDAMENTALS OF PHYSICAL GEOGRAPHY, Geography Class XI (NCERT 2025 ed.) > Chapter 8: Solar Radiation, Heat Balance and Temperature > SOLAR RADIATION > p. 67
- Certificate Physical and Human Geography , GC Leong (Oxford University press 3rd ed.) > Chapter 14: Climate > lnsolation > p. 131
- Environment and Ecology, Majid Hussain (Access publishing 3rd ed.) > Chapter 6: Environmental Degradation and Management > i) Solar Energy or Photovoltaic (Pv) Energy > p. 52
Solar radiation arrives mainly as short-wave (visible and UV) while Earth emits long-wave infrared; this distinction is central to any claim about what fraction of insolation is infrared.
High-yield: understanding the short-wave/long-wave split is essential for questions on Earth's energy balance, heat budget, and diurnal/seasonal temperature behaviour. It links radiation physics to topics like albedo, outgoing terrestrial radiation, and climate processes; mastering it helps answer questions about energy flow and greenhouse mechanisms.
- FUNDAMENTALS OF PHYSICAL GEOGRAPHY, Geography Class XI (NCERT 2025 ed.) > Chapter 8: Solar Radiation, Heat Balance and Temperature > SOLAR RADIATION > p. 67
- Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 21: Horizontal Distribution of Temperature > Insolation > p. 282
- Environment, Shankar IAS Acedemy .(ed 10th) > Chapter 17: Climate Change > Emission > p. 255
Atmospheric gases (water vapour, ozone) and particles selectively absorb or scatter certain solar wavelengths, so the composition of incoming solar bands at the surface differs from the top-of-atmosphere spectrum.
High-yield: explains why incoming solar spectrum at surface is altered (important for radiation budgets, climate, and observational interpretation). It connects chemistry (ozone, water vapour) to physical geography and climatology and supports reasoning about what portions of solar energy reach the surface.
- FUNDAMENTALS OF PHYSICAL GEOGRAPHY, Geography Class XI (NCERT 2025 ed.) > Chapter 8: Solar Radiation, Heat Balance and Temperature > The Passage of Solar Radiation through the Atmosphere > p. 68
- Environment and Ecology, Majid Hussain (Access publishing 3rd ed.) > Chapter 1: BASIC CONCEPTS OF ENVIRONMENT AND ECOLOGY > Structure of the Atmosphere > p. 8
- Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 20: Earths Atmosphere > Water Vapour > p. 272
Greenhouse gases absorb outgoing long-wave infrared from the surface and re-radiate it, which is distinct from the incoming short-wave solar radiation composition.
High-yield: central to questions on climate change, surface temperature regulation, and the planetary heat budget. It links radiative transfer to policy-relevant topics (warming, feedbacks) and enables tackling questions about causes and effects of atmospheric warming.
- Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 24: Hydrological Cycle (Water Cycle) > Explanation: > p. 337
- Environment and Ecology, Majid Hussain (Access publishing 3rd ed.) > Chapter 6: Environmental Degradation and Management > Greenhouse Effect and Global Warming > p. 7
- FUNDAMENTALS OF PHYSICAL GEOGRAPHY, Geography Class XI (NCERT 2025 ed.) > Chapter 8: Solar Radiation, Heat Balance and Temperature > Heat Budget of the Planet Earth > p. 69
Water vapour absorbs long-wave and near-infrared radiation and contributes strongly to the atmosphere's insulating (greenhouse) effect.
High-yield for questions on radiative forcing and greenhouse gases; links physical geography to climate change topics and helps answer why humid regions retain more heat. Mastery allows answering causeβeffect questions on surface warming and diurnal temperature ranges.
- Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 20: Earths Atmosphere > Water Vapour > p. 272
- FUNDAMENTALS OF PHYSICAL GEOGRAPHY, Geography Class XI (NCERT 2025 ed.) > Chapter 8: Solar Radiation, Heat Balance and Temperature > The Passage of Solar Radiation through the Atmosphere > p. 68
The 'Solar Constant' Variation. Since the question touched on insolation amounts, the next logical question is the variation due to distance. Earth receives ~7% more insolation at Perihelion (Jan 3) than at Aphelion (July 4). This is a sibling fact in the same NCERT chapter.
Use Etymology and Common Sense. Option D: 'Infra' means 'Below'. Infrared is 'Below Red'. It cannot be *part* of the visible spectrum by definition. Option A: If the Equator received 10x the energy of the Poles, the Poles would be near absolute zero or the Equator would be uninhabitable; the actual gradient is significant but not that extreme (approx 4x).
Link this to Environment (Climate Change): Water Vapour is actually the most potent 'Natural' Greenhouse Gas, but it is a 'Feedback' agent, not a 'Forcing' agent. Warmer air holds more moisture (Clausius-Clapeyron relation) β more IR absorption β more warming. This is the 'Water Vapour Feedback Loop' crucial for Mains GS-3.