| Elektromagnetisches
Spektrum, Strahlungsenergie und Absorption | |
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Abb.: Schema des elektromagnetischen Spektrums ("A schematic
of the Electromagnetic Spectrum") mit der Leistung der Sonnenenergie
in Beziehung zu den Wellenlängen. Im unteren Teil der Abbildung ausserdem
Charakteristiken der Strahlungsabsorption für Wasserdampf und Kohlenstoffdioxid.
("Radiation Absorption characteristics of Water Vapour and Carbon Dioxide").
Spektralbereiche von kurzwelliger bis langwelliger Strahlung.
Verändert nach
The
Greenhouse Effect and Climate Change Geoscience
Australia, by Chris Hepplewhite: "A
schematic of the electromagnetic spectrum, showing the Sun's energy output in
relation to wavelength"
Anmerkung:
Diese allzu schematische - und dadurch missverständliche - Kurve wurde
am 10.09.08 ersetzt aus: "Plasma
Redshift and the Astrophysics of the Non-Exploding Universe" (Fig.: Solar
disk center intensity) nach: Burlov-Vasiljev
K.A., Gurtovenko E.A., Matvejev Yu.B. (1995) New absolute measurements of the
solar spectrum 310685 nm.- Solar Phys. 15: 51-73. Burlov-Vasiljev
K.A., Matvejev Yu.B., Vasiljeva I.E. (1998) New Measurements of the Solar Disk-center
Spectral Intensity in the Near IR from 645 nm to 1070 nm.- Solar Phys. 177:
25-40. aus: http://www.mao.kiev.ua/sol_ukr/terskol/ters_all.html
"An
unexpected discovery could yield a full spectrum solar cell" by Paul
Preuss, Berkeley Lab. "Physical
Oceanography Animations" by Louis E. Keiner, Coastal Carolina University,
Marine Science, Electromagnetic
Spectrum The
Greenhouse Effect and Climate Change: "The radiation Absorption
characteristics of Water Vapour and Carbon Dioxide as a function of wavelength
(...) The percentage absorption of a vertical beam by representative atmospheric
concentrations of water vapour (H2O) and carbon dioxide (CO2)
are shown "
according to Australia
2007, Bureau of Meteorology (BOM) - Geoscience
Australia, by Chris Hepplewhite.
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| Zum
elektromagnetischen Spektrum vgl. Sie bitte auch: Elektromagnetisches
Spektrum, von K. Ziemke, Universität Kiel, Geographisches Institut,
Fernerkundung - neue Methoden und Medien für Geographie und Unterricht,
Prof. Hassenpflug, Material zur Vorlesung im Internet, 05.05.99.
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Abb.:
"Wasserdampf ist das wichtigste Treibhausgas der Atmosphäre,
da es in einem breiten Wellenlängenbereich langwellige Strahlung aufnehmen
kann. Die übrigen Treibhausgase spielen eine geringere Rolle, da der Wasserdampf
[siehe nächsten Abschnitt] bereits einen grossen Teil der Strahlungsenergie
aufgenommen hat." (aus
Berner & Streif 2000: 25) |
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Zur
solar-terrestrischen Strahlungsbilanz: | | |
| Tsushima,
Y., A. Abe-Ouchi, and S. Manabe, (2005) Radiative damping of annual variation
in global mean surface temperature: comparison between observed and simulated
feedback.- Climate dynamics, published online before print March 25, 2005
- Abstract:
"The
sensitivity of the global climate is essentially determined by the radiative damping
of the global mean surface temperature anomaly through the outgoing radiation
from the top of the atmosphere (TOA). Using the TOA fluxes of terrestrial and
reflected solar radiation obtained from the Earth radiation budget experiment
(ERBE), this study estimates the magnitude of the overall feedback, which modifies
the radiative damping of the annual variation of the global mean surface temperature,
and compare it with model simulations. Although the pattern of the annually varying
anomaly is quite different from that of the global warming, the analysis conducted
here may be used for assessing the systematic bias of the feedback that operates
on the CO2-induced warming of the surface temperature. In the absence
of feedback effect, the outgoing terrestrial radiation at the TOA is approximately
follows the Stefan-Boltzmanns fourth power of the planetary emission temperature.
However, it deviates significantly from the blackbody radiation due to various
feedbacks involving water vapor and cloud cover. In addition, the reflected solar
radiation is altered by the feedbacks involving sea ice, snow and cloud, thereby
affecting the radiative damping of surface temperature. The analysis of ERBE reveals
that the radiative damping is weakened by as much as 70% due to the overall effect
of feedbacks, and is only 30% of what is expected for the blackbody with the planetary
emission temperature. Similar feedback analysis is conducted for three general
circulation models of the atmosphere, which was used for the study of cloud feedback
in the preceding study. The sign and magnitude of the overall feedback in the
three models are similar to those of the observed. However, when it is
subdivided into solar and terrestrial components, they are quite different from
the observation mainly due to the failure of the models to simulate individually
the solar and terrestrial components of the cloud feedback. It is therefore
desirable to make the similar comparison not only for the overall feedback but
also for its individual components such as albedo- and cloud-feedbacks.
Although the pattern of the annually-varying anomaly is quite different from that
of global warming, the methodology of the comparative analysis presented here
may be used for the identification of the systematic bias of the overall feedback
in a model. A proposal is made for the estimation of the best guess value of climate
sensitivity using the outputs from many climate models submitted to the Intergovernmental
panel on Climate Change." | | |
CERES:
Understanding the Earths Clouds and Climate | |
What
CERES Will Measure "CERES
will measure the energy at the top of the atmosphere, as well as estimate energy
levels in the atmosphere and at the Earths surface. Using information
from very high resolution cloud imaging instruments on the same spacecraft, CERES
also will determine cloud properties, including altitude, thickness, and the size
of the cloud particles. All of these measurements are critical for advancing
the understanding of the Earths total climate system and the accuracy of
climate prediction models." Cloud
Effects "One
of the most intriguing questions facing climate modelers today is how clouds affect
the Earths climate and vice versa. The U.S. Global Change Research Program
classifies understanding the role of clouds and the Earths energy budget
as one of its highest scientific priorities. Understanding cloud effects requires
a detailed knowledge of how clouds absorb and reflect sunlight, as well as how
they absorb and re-emit outgoing heat emitted by the planet. For example, low,
thick clouds primarily reflect incoming solar energy back to space causing cooling.
Thin, high clouds, however, primarily trap outgoing heat and produce warming.
To date, satellite studies have found that clouds have an overall cooling effect
on the Earth. Analyses
of satellite data also indicate that clouds which form over water are very different
from clouds which form over land. These differences affect the way clouds reflect
sunlight back into space and how much heat emitted from the Earth the clouds absorb
and re-emit. For example, over the equator in the eastern Pacific Ocean during
El Niño events, there is a significant decrease in the amount of energy
emitted by the Earth due to increased cloudiness. El Niño events occur
when portions of the eastern Pacific Ocean become considerably warmer than normal,
causing an increase in cloudiness over the region. These changes can affect weather
patterns around the world." Water
Vapor Effects
"Water
vapor in the atmosphere also impacts our daily weather and climate, though scientists
are only beginning to understand how this complex mechanism works. Water
vapor acts like a greenhouse gas and absorbs outgoing heat to warm the Earth.
Because water vapor also condenses to make clouds, additional water vapor in the
atmosphere also may increase the amount of clouds." |
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| | | Weiterführende
Links zum Thema "Global Warming" etc. innerhalb dieser Website (
nur
kurze Hinweise!): | | |
Kurzer
Überblick zur Klimageschichte
Literaturangaben zur Klimageschichte, kleine Auswahl
Klimaschwankungen
im Jungpleistozän und Holozän
Die
glaziale und postglaziale Vegetationsgeschichte Afrikas
Meeresspiegel
während des LGM (120m unter NN) u. Simulation um +5m ü.NN
Nordseegeschichte
Entwicklung
der Insel Sylt
Holozäne Optima und Pessima
2000
Jahre Temperaturentwicklung der nördlichen Hemisphäre
Der sogenannte Treibhauseffekt
Hurrikane
Die Bedeutung von Kohlendioxid
Der Kohlenstoffkreislauf |
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Copyright
© Harald Kehl TU-Berlin - Institut für Ökologie |
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