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Tropical Cyclone Life Cycle
π A tropical cyclone progresses through three basic stages: origin/source, the mature stage, and dissipation (death).
π The stages are continuous; a cyclone can weaken over land, re-enter the sea, and strengthen again.
Conditions for Cyclone Formation
π Formation requires a large, still, warm ocean area where the surface temperature exceeds 26.5Β° Celsius over an extended period.
π¨ As warm air rises, it expands, cools, and condenses, forming clouds up to 10 kilometers high in the troposphere, releasing latent heat that powers the cyclone.
πͺοΈ The Coriolis effect (due to Earth's rotation) causes rising air currents to spiral, marking the mature stage and creating the eye of the storm.
Mature Cyclone Characteristics
π Cyclones rotate counter-clockwise in the Northern Hemisphere and clockwise in the Southern Hemisphere.
π¨ The eye wall has the strongest winds, while the eye itself is a calm, clear area formed by descending dense air.
π The lowest air pressure is at the center, typically 950 millibars (mb) or less, compared to the average surface pressure of about 1010 mb.
π¨ The largest pressure difference results in the strongest wind force; Typhoon Ida in 1958 recorded a low pressure of 877 mb with winds reaching 300 kilometers per hour.
Key Points & Insights
β‘οΈ Cyclone movement follows a track driven by global wind circulation away from its source, sustained by warm ocean waters providing heat and moisture.
β‘οΈ The release of latent heat during condensation is the critical energy source that makes the cyclone a self-sustaining heat cycle.
β‘οΈ The lowest recorded pressure for a tropical cyclone was 877 millibars during Typhoon Ida in 1958.
πΈ Video summarized with SummaryTube.com on Nov 14, 2025, 09:55 UTC
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Full video URL: youtube.com/watch?v=UKL9NIxLIIE
Duration: 7:07
Get instant insights and key takeaways from this YouTube video by ClickView.
Tropical Cyclone Life Cycle
π A tropical cyclone progresses through three basic stages: origin/source, the mature stage, and dissipation (death).
π The stages are continuous; a cyclone can weaken over land, re-enter the sea, and strengthen again.
Conditions for Cyclone Formation
π Formation requires a large, still, warm ocean area where the surface temperature exceeds 26.5Β° Celsius over an extended period.
π¨ As warm air rises, it expands, cools, and condenses, forming clouds up to 10 kilometers high in the troposphere, releasing latent heat that powers the cyclone.
πͺοΈ The Coriolis effect (due to Earth's rotation) causes rising air currents to spiral, marking the mature stage and creating the eye of the storm.
Mature Cyclone Characteristics
π Cyclones rotate counter-clockwise in the Northern Hemisphere and clockwise in the Southern Hemisphere.
π¨ The eye wall has the strongest winds, while the eye itself is a calm, clear area formed by descending dense air.
π The lowest air pressure is at the center, typically 950 millibars (mb) or less, compared to the average surface pressure of about 1010 mb.
π¨ The largest pressure difference results in the strongest wind force; Typhoon Ida in 1958 recorded a low pressure of 877 mb with winds reaching 300 kilometers per hour.
Key Points & Insights
β‘οΈ Cyclone movement follows a track driven by global wind circulation away from its source, sustained by warm ocean waters providing heat and moisture.
β‘οΈ The release of latent heat during condensation is the critical energy source that makes the cyclone a self-sustaining heat cycle.
β‘οΈ The lowest recorded pressure for a tropical cyclone was 877 millibars during Typhoon Ida in 1958.
πΈ Video summarized with SummaryTube.com on Nov 14, 2025, 09:55 UTC
Find relevant products on Amazon related to this video
Energy
Shop on Amazon
Productivity Planner
Shop on Amazon
Habit Tracker
Shop on Amazon
Journal
Shop on Amazon
As an Amazon Associate, we earn from qualifying purchases

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