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Medições diárias de radiação solar global foram feitas, durante o período de junho de 2000 a janeiro de 2001, no interior de mata semidecídua e no ambiente exterior, tendo sido registrados valores médios de 1,1 e 19,3 MJ/m²/d, respectivamente.
José Luiz Hernandes +2 more
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SOHO – an Observatory to Study the Solar Interior and the Solar Atmosphere [PDF]
AbstractThe Solar and Heliospheric Observatory, Soho, is a joint venture of ESA and NASA. The main objectives of Soho are: a) the study and understanding of solar coronal phenomena; and b) the study of the solar structure and interior dynamics from its core to the photosphere.
A. I. Poland, V. Domingo
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Attenuation of glazing energy using linear patterns on the glass surface
Glazing energy resulting from solar radiation can be the main source to vary the thermal field inside of a building. As the glass material is loaded by intensive solar radiation, the glazing energy, greatly induced, will result in the drastic increase in
Shiang-Jiun Lin +3 more
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The sun being the nearest star, provides us a unique opportunity to study stellar processes in sufficient detail to test theories of stellar structure and evolution.
Antia, H. M.
core
Rotation of the solar interior
Helioseismology has allowed us to infer the rotation in the greater part of the solar interior with high precision and resolution. The results show interesting conflicts with earlier theoretical expectations, indicating that the the Sun is host to complex dynamical phenomena, so far hardly understood. This has important consequences for our ideas about
Christensen-Dalsgaard, J.; id_orcid 0000-0001-5137-0966 +1 more
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Effects of interior conductivity on solar wind proton precipitation on Mercury
Context. Mercury is an airless body where space weathering processes play a key role in modifying the surface and sustaining the exosphere. Some of these processes are thought to be linked to ion precipitation driven by solar wind–magnetosphere ...
Shi Z. +10 more
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Simulations of the Onset and Dynamical Evolution of Inertial Waves in Solar/Stellar Interior
Inertial modes have been recently detected in the Sun via helioseismology, yet their origin, evolution, and role in the dynamics of the solar plasma and magnetic field remain poorly understood.
M. D. Souza-Gomes +6 more
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This chapter introduces the reader to the solar interior, in particular the convection zone. The first section explores the solar cycle and the dynamo models that have been studied to explain this cycle. The second section explores helioseismology observations and analysis of the solar interior, and reviews the fundamental knowledge that has been ...
Linton, Mark +2 more
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Space weather and disturbances in the heliosphere are manifestations of the solar magnetic field, which is solely driven by the interior dynamo. Constraining the solar interior magnetic field and its oscillatory behavior is one of the major challenges in
Soumyadeep Chatterjee, Gopal Hazra
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Performance of a building integrated photovoltaic/thermal (BIPVT) solar collector [PDF]
The idea of combining photovoltaic and solar thermal collectors (PVT collectors) to provide electrical and heat energy is an area that has, until recently, received only limited attention.
Carson, James K. +3 more
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