The global climate is determined by the exchange of energy between the earth, atmosphere, and space. Arriving from the sun, solar radiation is transformed by processes of absorption, scattering, and emission as it enters, interacts with, and eventually leaves the planet. Occurring dominantly through radiative and convective mechanisms, the upward motion of thermal energy gives the at- mosphere its structure and determines surface temperatures. Understanding radiative transfer and its dependence on atomic spectra gives insight on why minute changes in the composition of the atmosphere can have drastic effects on climate through the greenhouse effect
The basis for this study is the flow of energy from the Troposphere to space and the role that water...
We present detailed line-by-line radiation transfer calculations, which were performed under differe...
International audienceThe two main terms in the Earth's energy balance are the absorption of solar r...
Spectroscopy and radiative transfer are rapidly growing fields within atmospheric and planetary scie...
Temperature conditions and climate on Earth are controlled by the balance between absorbed solar rad...
The global climate system is driven by energy, almost all of which comes from the Sun. In this chap...
Solar radiation is the fundamental energy source for the atmosphere and the global average equilibri...
We present a radiative transfer model for Earth-Like-Planets (ELP). The model allows the assessment ...
A first-look at radiative transfer in planetary atmospheres with a particular focus on the Earth's a...
The Earth’ climate is a complex system consisting of the atmosphere, the ocean and the land surface....
Radiative energy is critical in controlling the heat and mass balance of sea ice, which significantl...
The study of physical and chemical properties of aerosol is of significant importance, because their...
in the Earth’s atmosphere, absorb thermal IR radiation emitted by the Earth’s surface and atmosphere...
Our planet is continuously bathed in solar radiation. Although we who are confined to a fixed locati...
Weather and climate on Earth is determined by the amount and distribution of incoming radiation from...
The basis for this study is the flow of energy from the Troposphere to space and the role that water...
We present detailed line-by-line radiation transfer calculations, which were performed under differe...
International audienceThe two main terms in the Earth's energy balance are the absorption of solar r...
Spectroscopy and radiative transfer are rapidly growing fields within atmospheric and planetary scie...
Temperature conditions and climate on Earth are controlled by the balance between absorbed solar rad...
The global climate system is driven by energy, almost all of which comes from the Sun. In this chap...
Solar radiation is the fundamental energy source for the atmosphere and the global average equilibri...
We present a radiative transfer model for Earth-Like-Planets (ELP). The model allows the assessment ...
A first-look at radiative transfer in planetary atmospheres with a particular focus on the Earth's a...
The Earth’ climate is a complex system consisting of the atmosphere, the ocean and the land surface....
Radiative energy is critical in controlling the heat and mass balance of sea ice, which significantl...
The study of physical and chemical properties of aerosol is of significant importance, because their...
in the Earth’s atmosphere, absorb thermal IR radiation emitted by the Earth’s surface and atmosphere...
Our planet is continuously bathed in solar radiation. Although we who are confined to a fixed locati...
Weather and climate on Earth is determined by the amount and distribution of incoming radiation from...
The basis for this study is the flow of energy from the Troposphere to space and the role that water...
We present detailed line-by-line radiation transfer calculations, which were performed under differe...
International audienceThe two main terms in the Earth's energy balance are the absorption of solar r...