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Weather Wonders: A Journey from Micro-Weather to Macro-Circulation
GEOG1001S-PEP-CNLesson 3
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This lesson aims to establish a holistic spatiotemporal perspective on atmospheric motion. We first establishsolar radiationas the fundamental driver of atmospheric motion. Due to uneven energy distribution between low and high latitudes, surface thermal differences ariseโ€”this is the root cause of all atmospheric motion.

Solar Radiation (Fundamental Driver)Solar Radiation (Fundamental Driver)Heat Difference โ†’ Atmospheric MotionAtmospheric Circulation System

Core Concepts

  • Atmospheric Circulation: Large-scale, regular atmospheric motion across the globe. It not only regulates heat and moisture balance but also forms the foundational backdrop of global climate patterns.
  • Understanding Geographic Distribution Across Scales: Geographical observation has spatiotemporal scale characteristics. For example, individual thunderstorms belong to micro- or mesoscale, while subtropical high-pressure belts are macro- or global-scale phenomena.
  • Definition of Direction: In geography, 'direction' has dual meaningโ€”it not only includes the motionโ€™sdirection(such as prevailing wind direction), but also its location in terms ofgeographical position(such as specific latitude zones).
Summary & Synthesis
Atmospheric circulation is not chaotic or random motion; it is a stable system formed by the combined effects of Coriolis force, friction, and thermal contrasts, maintaining global heat balance. Large-scale, regular atmospheric motion across the globe is commonly referred to as atmospheric circulation.