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Synoptic Lesson 1
This is form Sikora's Lesson 1 Notes
Term | Definition |
---|---|
Empiricism and Theoretical Dynamics | The two basic ways to group phenomena within the atmosphere? |
Empirical Method | The ability to sense a given phenomena. |
Mesoscale | Describes a phenomena sensed by weather radars that was smaller than the synoptic scale but larger than the microscale. (1950s) |
Theoretical Method | Based on Atmospheric forces/accelerations from the governing equations that have different importance at different scales. |
What can be disregarded in the synoptic scale? | Vertical accelerations and ageostrophic advenction. |
What can be disregarded for the microscale? | Coriolis acceleration. |
What cannot be simplified in the mesoscale? | Governing equations. |
Traits of Macro α (planetary scale) | - Hori spatial scales > 10,000 km - Ex: Small frequency waves |
Traits of Macro β (synoptic scale) | - Hori scales between 10,000 km and 2,000 km. - Ex: Extra-tropical cyclone |
Traits of Meso α | - Hori scales between 2,000 km and 200 km. - Ex: Hurricanes, polar mesoscale cyclones, frontal zones. |
Traits of Meso β | - Hori scales between 200 km and 20 km -Ex: Mesoscale convective complexes |
Traits of Meso γ | - Hori scales between 20 km and 2 km - Ex: T-storms, some larger atmo. gravity waves |
Traits of Micro α | - Hori scales between 2 km and 0.2 km - Ex: Boundary layer cumulus clouds, large scale tornadoes, short atmo. gravity waves |
Traits of Micro β | - Hori scales between 0.2 km and 0.02 km - Ex: Dust devils and thermals |
Traits of Micro γ | - Hori scales between 0.02 km and 0.002 km - Ex: Surface layer plumes |
Traits of Micro δ | - Hori scales < 0.002 km - Ex: Small-scale mechanical turbulence |
Most of Kinetic Energy exists where in the atmo.? | It exists in the planetary and synoptic scales are any given time. |
1. Larger scales of motion are what? 2. Smallest scales of motion are what? (Based on atmo. KE) | 1. Sources of atmo. KE 2. Sinks of KE. |