Phu Xuan University Library
Fundamentals of Atmospheric Science

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Fundamentals of Atmospheric Science

This text prepares students by laying a solid foundation in the application of physical, chemical, and mathematical principles to a broad range of atmospheric phenomena. Students are introduced to fundamental concepts and applications of atmospheric thermodynamics, radiative transfer, atmospheric chemistry, cloud microphysics, atmospheric dynamics, and the atmospheric boundary layer.

Author
William Brune
Publisher
The Pennsylvania State University
Source
LibreTexts
License
CC BY-NC-SA
Language
EN
Category
Basic Sciences
Contents· 108 sections
  1. 01: Getting Started
  2. 1.01: The atmosphere is
  3. 1.02: You will not believe what you can do with math
  4. 1.03: If you thought practice makes perfect you could be right
  5. 1.04: Are you ready to get with the programming
  6. 1.05: Summary and Final Tasks
  7. 02: Thermodynamics
  8. 2.01: Gas Laws
  9. 2.02: The Atmospheres Pressure Structure - Hydrostatic Equilibrium
  10. 2.03: First Law of Thermodynamics
  11. 2.04: The higher the temperature the thicker the layer
  12. 2.05: Adiabatic Processes - The Path of Least Resistance
  13. 2.06: Stability and Buoyancy
  14. 03: Moist Processes
  15. 3.01: Ways to Specify Water Vapor
  16. 3.02: Condensation and Evaporation
  17. 3.03: Phase Diagram for Water Vapor - Clausius Clapeyron Equation
  18. 3.04: Solving Energy Problems Involving Phase Changes and Temperature Changes
  19. 3.05: The Skew-T Diagram- A Wonderful Tool
  20. 3.06: Understanding the Atmospheres Temperature Profile
  21. 3.07: Summary and Final Tasks
  22. 04: Atmospheric Composition
  23. 4.01: Atmospheric Composition
  24. 4.02: Changes in Atmospheric Composition
  25. 4.03: Other Trace Gases
  26. 4.04: Stratospheric Ozone Formation
  27. 4.05: The Story of the Atmosphere's PAC-MAN
  28. 4.06: Where do Cloud Condensation Nuclei (CCN) come from
  29. 4.07: Summary and Final Tasks
  30. 05: Cloud Physics
  31. 5.01: Looking at the Whole Cloud
  32. 5.02: Do you recognize these clouds drops and snowflakes
  33. 5.03: What are the requirements for forming a cloud drop
  34. 5.04: How can supersaturation be achieved
  35. 5.05: Curvature Effect - Kelvin Effect
  36. 5.06: Solute Effect - Raoults Law
  37. 5.07: Vapor Deposition
  38. 5.08: Did you know most precipitation comes from collision-coalescence
  39. 5.09: An Unusual Way to Make Precipitation in Mixed-Phase Clouds
  40. 5.10: Summary and Final Tasks
  41. 06: Atmospheric Radiation
  42. 6.01: Prelude to Atmospheric Radiation
  43. 6.02: Atmospheric Radiation - Why does it matter
  44. 6.03: Start at the Source - Earth Rotating Around the Sun
  45. 6.04: How is energy related to the wavelength of radiation
  46. 6.05: The Solar Spectrum
  47. 6.06: What is the origin of the Planck Function
  48. 6.07: Which wavelength has the greatest spectral irradiance
  49. 6.08: What is the total irradiance of any object
  50. 6.09: Kirchhoffs Law explains why nobody is perfect
  51. 6.10: Why do objects absorb the way that they do
  52. 07: Applications of Atmospheric Radiation Principles
  53. 7.01: Prelude to Applications of Atmospheric Radiation Principles
  54. 7.02: Applications of Atmospheric Radiation
  55. 7.03: Atmospheric Radiation and Earths Climate
  56. 7.04: What does the energy balance of the real atmosphere look like
  57. 7.05: Applications to Remote Sensing
  58. 7.06: What is the math behind these physical descriptions of the GOES data products
  59. 7.07: Summary and Final Tasks
  60. 08: Math and Conceptual Preparation for Understanding Atmospheric Motion
  61. 8.01: Prelude to Math and Conceptual Preparation for Understanding Atmospheric Motion
  62. 8.02: This is why partial derivatives are so easy...
  63. 8.03: What you dont know about vectors may surprise you
  64. 8.04: Describing weather requires coordinate systems.
  65. 8.05: Do you need a weathervane to see which way the wind blows
  66. 8.06: Gradients - How to Find Them
  67. 8.07: What You Experience Depends on Your Point of View - Eulerian vs. Lagrangian
  68. 8.08: Can the Eulerian and Lagrangian frameworks be connected
  69. 8.09: Summary and Final Tasks
  70. 09: Kinematics
  71. 9.01: Streamlines and trajectories arent usually the same.
  72. 9.02: Watch these air parcels move and change.
  73. 9.03: Five Air Motion Types You Must Get to Know
  74. 9.04: How does divergence relate to the air parcels area change
  75. 9.05: How is the horizontal divergence convergence related to vertical motion
  76. 9.06: How fast is the vertical wind and which way does it blow
  77. 9.07: Summary and Final Tasks
  78. 10: Dynamics - Forces
  79. 10.01: What does turbulent drag do to horizontal boundary layer flow
  80. 10.02: Why are midlatitude winds mostly westerly (i.e. eastward)
  81. 10.03: Why We Like Conservation
  82. 10.04: What are the important real forces
  83. 10.05: Effects of Earths Rotation- Apparent Forces
  84. 10.06: Equations of Motion in Spherical Coordinates
  85. 10.07: Are all the terms in these equations equally important Let's use scale analysis.
  86. 10.08: Why do weather maps use pressure surfaces instead of height surfaces
  87. 10.09: Natural coordinates are better horizontal coordinates.
  88. 10.10: A Closer Look at the Four Force Balances
  89. 10.11: See how the gradient wind has a role in weather.
  90. 10.12: Overview
  91. 10.13: Summary and Final Tasks
  92. 11: Atmospheric Boundary Layer
  93. 11.01: How do these fluxes look
  94. 11.02: Turbulent Eddies - A Cascade of Energy
  95. 11.03: The Surface Layers Energy Budget
  96. 11.04: The atmospheric boundary layer is your home.
  97. 11.05: A Day in the Life of the Boundary Layer
  98. 11.06: The Story of Diurnal Boundary Layer Growth Told in Vertical Profiles of Virtual Potential Temperature
  99. 11.07: Frozen - The Taylor Hypothesis
  100. 11.08: Heres How Reynolds Did Averaging
  101. 11.09: How Kinematic Fluxes Move Air Vertically
  102. 11.10: Can we relate this turbulent flux to a molecular flux
  103. 11.11: Lets see how vertical turbulent transport can be quantified.
  104. 11.12: What other fluxes are important
  105. 11.13: Summary and Final Tasks
  106. 12: The Atmosphere - A Holistic View
  107. 12.01: An Integrated View of the Atmosphere
  108. 12.02: The Final Project