Ozone molecules absorb high-energy UV photons, converting that energy into heat. In the lower stratosphere, temperatures remain relatively stable or even increase due to the absorption of ultraviolet (UV) radiation by ozone.
How Stratopause Dynamics Reshape Air Pressure at the Edge of Space
This thermal inversion is the defining feature that separates it from the layers below, and it is directly responsible for the unique pressure profile observed at these elevations. As altitude climbs toward the stratopause, the pressure continues to fall, reaching values between 1 and 0.
According to the ideal gas law, pressure is directly proportional to temperature when volume is constant. Pressure Dynamics and the Role of Temperature To understand the air pressure in the stratosphere, one must first look at temperature.
How the Stratopause Governs Air Pressure Shifts
Understanding this specific pressure regime is essential for grasping everything from aviation safety to the physics of ozone protection. While the troposphere contains the bulk of the atmosphere's mass and weather phenomena, the stratosphere is characterized by stability and increasing temperatures with altitude.
More About What is the air pressure in the stratosphere
Looking at What is the air pressure in the stratosphere from another angle can help expand the discussion and give readers a second clear paragraph under the same section.
More perspective on What is the air pressure in the stratosphere can make the topic easier to follow by connecting earlier points with a few simple takeaways.
