Final Study Guide 9 Flashcards
Paleo Climate
What is Earth systems science?
Earth system science seeks to integrate various fields of academic study to understand the Earth as a system.Earth system science embraces chemistry, physics, biology, mathematics and applied sciences in transcending disciplinary boundaries to treat the Earth as an integrated system and seeks a deeper understanding of the physical, chemical, biological and human interactions that determine the past, current and future states of the Earth. Earth system science provides a physical basis for understanding the world in which we live and upon which humankind seeks to achieve sustainability.
What is the greenhouse effect?
trapping of the sun’s warmth in a planet’s lower atmosphere due to the greater transparency of the atmosphere to visible radiation from the sun than to infrared radiation emitted from the planet’s surface.
Why is albedo a critical factor in climate-related feedbacks?
- Albedo- used to define the percentage of solar energy reflected back by a surface
- Understanding local, regional, and global albedo effects is critical to predicting global climate change
- The following are some of the factors that influence the earth’s albedo: clouds, ice,snow,surface, oceans and forests
- It is a very strong “positive feedback” (increases an initial warming) that has been included in climate models since the 1970s
List some of the long-term climate variability
- solar
> changes in the intensity of solar radiation reaching earth - volcanic
> eruptions add aerosols to the atmosphere, increasing reflection of radiation
> adds CO2, which increases global warming - greenhouse gases
> adds CO2, which increases global warming
How do we know past climate before the instrumental era?
Historical records; change in growth (tree rings, speleothems, corals); changes in organism/plant distribution (pollen records); chemical records (changes in isotopic ratios, in ice and sediment cores); geological evidence (glacial sediments)
Weather
natural phenomena within the atmosphere at a given time (seconds to hours to days)
Climate
the average weather conditions, and their range of variability, over a long period of time (~30 years or more)
Radiative Balance
the solid earth + atmosphere receive heat energy from the sun but they also radiate the same amount of heat back into space
Frequency
the number of times that something happens during a particular period
Wavelength
distance from one wave of energy to another as it is travelling from one point to another point
Electromagnetic Spectrum
- is the range of all possible frequencies of electromagnetic radiation; the “electromagnetic spectrum” of an object has a different meaning, and is instead the characteristic distribution of electromagnetic radiation emitted or absorbed by that particular object
- Higher frequency = more energetic
Wien’s Law
- relationship between temperature of a black body and the wavelength at which it emits the most light
- wavelength of emitted radiation is shorter for bodies at higher temperatures
- Used to infer the temperature of the sun
- Sunlight wavelengths ~500 nm (UV radiation) 5500-6000 K
- Objects that are cooler radiate longer wavelengths – so Earth radiates long wavelengths (red)
Black body radiation
radiation emitted by non-reflective body held at constant temperature- used to approximate radiation from stars and planets
Absorption
is the way in which the energy of a photon is taken up by matter, typically the electrons of an atom; thus, the electromagnetic energy is transformed to other forms of energy for example, to heat
Spectrum
group of colors that a ray of light can be separated into including red, orange, green, blue, indigo, and violet: the colors can be seen in a rainbow
Greenhouse effect
Energy radiated by the sun converts to heat when it reaches earth. Some heat is reflected back through the atmosphere, while some is absorbed by atmospheric gases and radiated back to earth.
Solar constant
a measure of flux density, is the amount of incoming solar electromagnetic radiation per unit area that would be incident on a plane perpendicular to the rays, at a distance of one astronomical unit (AU) (roughly the mean distance from the Sun to the Earth)
Hadley cells
- a large-scale atmospheric convection cell in which air rises at the equator and sinks at medium latitudes
- Steps:
> Moist warm air expands, rises
> Cools, condenses, rain falls
> Dense air sinks in sub tropics
> Warmed, dry air spreads at surface
Great ocean conveyor
- refers to a part of the large-scale ocean circulation that is driven by global density gradients created by surface heat and freshwater fluxes (salt driven)
Climate proxies
preserved physical characteristics of the past that stand in for direct measurements (as statistical proxies), to enable scientists to reconstruct the climatic conditions that prevailed during much of the Earth’s history
El Nino (drought)
- refers to the climatic conditions associated with temperatures in the eastern south pacific - in years with weak trade winds, these waters wam, and the warmer water influence global climate
- hard to predict
La Nina
- Warm ocean temperature in western pacific
- Opposite of El Nino
Paleoclimatology
is the study of changes in climate taken on the scale of the entire history of Earth