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Скачать или смотреть Global Climate Change | Chapter 21 - Earth: An Introduction to Physical Geology

  • Last Minute Lecture
  • 2025-08-24
  • 29
Global Climate Change | Chapter 21 - Earth: An Introduction to Physical Geology
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Описание к видео Global Climate Change | Chapter 21 - Earth: An Introduction to Physical Geology

Chapter 21 of Earth: An Introduction to Physical Geology (12th Edition) investigates the complexity of global climate change, examining how Earth’s climate system functions, how scientists detect past changes, and how both natural and human factors drive today’s warming. The climate system integrates the atmosphere, hydrosphere, geosphere, biosphere, and cryosphere, with interactions across these spheres shaping conditions over time. Climate differs from weather in its long-term patterns and variability, and it strongly influences geologic processes such as weathering, flooding, and glaciation.

To understand past climates, scientists use proxy data—indirect evidence from natural archives like seafloor sediments, oxygen isotope ratios, glacial ice cores, tree rings, fossil pollen, corals, and even historical documents. These records reveal alternating “greenhouse” and “icehouse” conditions through the Phanerozoic eon, multiple ice ages during the Quaternary, and abrupt shifts like the Younger Dryas. Oxygen isotope analysis of shells and ice provides precise records of glacial expansion and retreat, while ice cores preserve atmospheric gases such as CO₂ and methane, showing their correlation with temperature. Tree-ring chronologies, pollen analysis, and coral growth bands extend climate reconstructions back thousands of years.

The atmosphere’s composition and structure underpin modern climate science. Clean dry air is mostly nitrogen (78%) and oxygen (21%), but variable gases like water vapor, carbon dioxide, ozone, and aerosols play outsized roles in absorbing, reflecting, and transmitting radiation. Pressure decreases rapidly with altitude, while temperature defines vertical layers: the weather-filled troposphere, the ozone-heated stratosphere, the mesosphere, and the thermosphere. Heating of the atmosphere is governed by solar radiation, reflection (albedo), and re-radiation of long-wave energy absorbed by greenhouse gases. The natural greenhouse effect makes Earth habitable, but human activity is intensifying it.

Natural causes of climate change include plate tectonics (shifting landmasses altering circulation), orbital variations (Milankovitch cycles of eccentricity, tilt, precession), explosive volcanism (aerosols cooling the troposphere), and solar variability (sunspot cycles). These forces explain past shifts but cannot account for modern rapid warming. Since 1750, human impacts have transformed atmospheric composition through fossil fuel combustion and deforestation, driving a sharp rise in CO₂ levels unprecedented in 650,000 years. Trace gases—methane, nitrous oxide, and CFCs—amplify warming, while aerosols have a short-lived cooling effect by reflecting sunlight, though black carbon (soot) increases warming when deposited on snow and ice.

Climate-feedback mechanisms complicate predictions. Positive feedbacks, like water vapor increase, sea ice loss, and permafrost thaw (releasing CO₂ and methane), magnify warming, while negative feedbacks, like some cloud effects, can offset it. Climate models (general circulation models) simulate global patterns, confirming that observed 20th- and 21st-century warming cannot be explained without human greenhouse gas emissions.


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