Towards an Improved Understanding of the Global Energy Balance: Temporal Variations of Solar Radiation in the Climate System
dc.contributor.author
Schwarz, Matthias
dc.contributor.supervisor
Wild, Martin
dc.contributor.supervisor
Schär, Christoph
dc.contributor.supervisor
Folini, Doris
dc.contributor.supervisor
Kinne, Stefan
dc.date.accessioned
2019-07-17T13:24:32Z
dc.date.available
2019-07-17T12:27:37Z
dc.date.available
2019-07-17T13:24:32Z
dc.date.issued
2019
dc.identifier.uri
http://hdl.handle.net/20.500.11850/353615
dc.identifier.doi
10.3929/ethz-b-000353615
dc.description.abstract
The spatiotemporal distribution of absorbed solar radiation in the Earth’s climate system is a fundamental driver of the Earth’s climate. Today, the global long-term annual mean energy fluxes of the global energy balance are reasonably well known. In this thesis, we go beyond the long-term annual mean perspective and focus on temporal variations in the energy balance. Specifically, we study annual cycles and multidecadal changes of the shortwave fluxes of the energy balance in an observation-based framework.
To this end, we combine observations of top-of-the-atmosphere (TOA) radiative fluxes and surface albedo, both obtained from satellites, with surface flux observations. The latter are available from in-situ or satellite observations. In-situ observations are the most robust and accurate way to determine surface solar radiation but their spatial availability is limited. Satellite-derived surface radiation is less accurate but has greater spatial coverage. In this thesis, we use both data sources depending on whether accuracy or spatial coverage is needed.
Using in-situ data – which from a spatial perspective is point data – in combination with other gridded data products requires a thorough assessment of potential methodological uncertainties which arise when combining those two data sets. In Chapter 2 and Chapter 3 of this thesis, different aspects of spatiotemporal representativeness of monthly mean records of surface solar radiation point observations are assessed globally. Although large regional differences in the representativeness of point measurements occur, in most regions they can be considered representative of a larger surrounding. Therefore, examining temporal variations in the shortwave energy fluxes by combining in-situ and colocated gridded flux data is feasible. However, additional uncertainties must be taken into account.
Due to the Earth’s celestial movement around the Sun, large seasonal cycles in the amount and geographic distribution of solar insolation occur. These variations play a key role in the distribution of energy in the climate system and ultimately drive the seasonality of Earth’s general circulation systems, climate, and weather. Nevertheless, as recently shown by Hakuba et al. (2014b), the fraction of the incoming shortwave radiation at the top-of-the-atmosphere which is absorbed within the atmosphere does not substantially vary with season or latitude in Europe. An astonishing result, when considering that various climate elements which potentially influence the shortwave radiative fluxes have notable annual cycles. In Chapter 4 we go beyond Europe and identify several regions with large annual cycles in fractional atmospheric absorption. We find that they are driven mainly by annual cycles of water vapor and different aerosol species. The largest annual cycles in fractional atmospheric absorption are
apparent in regions with large annual cycles in aerosol loading related to seasonal biomass burning, which is a strong indication that these annual cycles are anthropogenically intensified or even entirely forced. We also show that the skill of global climate models to simulate the observed patterns in the annual cycles of atmospheric shortwave absorption is limited.
It is well known from observations that significant widespread variations in the amount of solar radiation reaching the Earth’s surface occurred on decadal time scales, known as global dimming and global brightening. According to the principle of energy conservation – the foundation of the energy balance – such changes in surface solar radiation must go along with a change in surface absorption, the TOA net flux, or the atmospheric absorption. In the observation-based energy balance framework, we find that changing atmospheric shortwave absorption is a major cause for the observed trends in Europe and China. The simultaneous trend analysis for surface, atmospheric, and TOA fluxes suggests that changes in aerosols – and in particular absorbing ones – are responsible for the observed trends.
Taken together, this thesis demonstrates that an integrative approach to the shortwave energy balance, in which TOA, atmospheric and surface fluxes are simultaneously analyzed, can lead to valuable insights into key aspects of the climate system.
en_US
dc.format
application/pdf
en_US
dc.language.iso
en
en_US
dc.publisher
ETH Zurich
en_US
dc.rights.uri
http://rightsstatements.org/page/InC-NC/1.0/
dc.subject
climate
en_US
dc.subject
RADIATION (METEOROLOGY)
en_US
dc.subject
Energy balance
en_US
dc.subject
Shortwave radiation
en_US
dc.subject
Temporal variations
en_US
dc.subject
Representativity analysis
en_US
dc.subject
Surface observations
en_US
dc.subject
Satellite observations
en_US
dc.subject
Dimming and brightening
en_US
dc.subject
Atmospheric absorption
en_US
dc.subject
atmosphere
en_US
dc.title
Towards an Improved Understanding of the Global Energy Balance: Temporal Variations of Solar Radiation in the Climate System
en_US
dc.type
Doctoral Thesis
dc.rights.license
In Copyright - Non-Commercial Use Permitted
dc.date.published
2019-07-17
ethz.size
170 p.
en_US
ethz.code.ddc
DDC - DDC::5 - Science::550 - Earth sciences
ethz.code.ddc
DDC - DDC::5 - Science::520 - Astronomy, cartography
ethz.code.ddc
DDC - DDC::5 - Science::550 - Earth sciences
en_US
ethz.code.ddc
DDC - DDC::5 - Science::500 - Natural sciences
en_US
ethz.grant
Towards an improved understanding of the Global Energy Balance: temporal variation of solar radiation in the climate system
en_US
ethz.identifier.diss
25942
en_US
ethz.publication.place
Zurich
en_US
ethz.publication.status
published
en_US
ethz.leitzahl
ETH Zürich::00002 - ETH Zürich::00012 - Lehre und Forschung::00007 - Departemente::02350 - Dep. Umweltsystemwissenschaften / Dep. of Environmental Systems Science::02717 - Institut für Atmosphäre und Klima / Inst. Atmospheric and Climate Science
en_US
ethz.grant.agreementno
159938
ethz.grant.fundername
SNF
ethz.grant.funderDoi
10.13039/501100001711
ethz.grant.program
Projekte MINT
ethz.date.deposited
2019-07-17T12:27:43Z
ethz.source
FORM
ethz.eth
yes
en_US
ethz.availability
Open access
en_US
ethz.rosetta.installDate
2019-07-17T13:25:28Z
ethz.rosetta.lastUpdated
2022-03-28T23:16:50Z
ethz.rosetta.versionExported
true
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Doctoral Thesis [30258]