Results 31 to 40 of about 30,800 (166)
Stratospheric warming influence on the mesosphere/lower thermosphere as seen by the extended CMAM [PDF]
The response of the upper mesosphere/lower thermosphere region to major sudden stratospheric warming (SSW) is examined employing temperature, winds, NOX and CO constituents from the extended Canadian Middle Atmosphere Model (CMAM) with continuous ...
M. G. Shepherd +2 more
doaj +1 more source
We describe the baseline model configuration and simulation characteristics of the Geophysical Fluid Dynamics Laboratory (GFDL)'s Atmosphere Model version 4.1 (AM4.1), which builds on developments at GFDL over 2013–2018 for coupled carbon‐chemistry ...
Larry W. Horowitz +15 more
doaj +1 more source
Simulating whole atmosphere dynamics, chemistry, and physics is computationally expensive. It can require high vertical resolution throughout the middle and upper atmosphere, as well as a comprehensive chemistry and aerosol scheme coupled to radiation ...
N. A. Davis +13 more
doaj +1 more source
3-4 day Kelvin waves observed in the MLT region at 7.4o S, Brazil [PDF]
Meteor wind measurements obtained from São João do Cariri-PB (7.4° S, 36.5° W), Brazil, during 2005, have been used to examine the ultra-fast Kelvin wave characteristics in the mesopause and lower thermosphere region.
P. P. Batista +6 more
doaj
We present results of modeling of the effect of internal gravity waves (IGW), excited in the region of development of a sudden stratospheric warming (SSW), on upper atmospheric conditions.
Vasilyev P.A. +2 more
doaj +1 more source
Results of an interactively coupled atmospheric chemistry – general circulation model: Comparison with observations [PDF]
The coupled climate-chemistry model ECHAM4.L39(DLR)/CHEM is presented which enables a simultaneous treatment of meteorology and atmospheric chemistry and their feedbacks.
R. Hein +12 more
doaj +1 more source
Active upper-atmosphere chemistry and dynamics from polar circulation reversal on Titan [PDF]
Saturn's moon Titan has a nitrogen atmosphere comparable to Earth's, with a surface pressure of 1.4 bar. Numerical models reproduce the tropospheric conditions very well but have trouble explaining the observed middle-atmosphere temperatures, composition and winds.
Teanby, Nicholas +8 more
openaire +3 more sources
MANGO: An optical network to study the dynamics of the Earth’s upper atmosphere
The Mid-latitude All-sky-imaging Network for Geophysical Observations (MANGO) employs a combination of two powerful optical techniques used to observe the dynamics of Earth’s upper atmosphere: wide-field imaging and high-resolution spectral interferometry.
A. N. Bhatt +7 more
openaire +1 more source
MAPPING GLOBAL OCEAN SURFACE ALBEDO FROM SATELLITE OBSERVATIONS: MODELS, ALGORITHMS, AND DATASETS [PDF]
Ocean surface albedo (OSA) is one of the important parameters in surface radiation budget (SRB). It is usually considered as a controlling factor of the heat exchange among the atmosphere and ocean.
X. Li +5 more
doaj +1 more source
The effect of dynamics on the composition of Titan's upper atmosphere [PDF]
Using a global time‐dependent general circulation model, we calculate the distribution of constituents in Titan's thermosphere resulting from transport caused by winds and molecular and eddy diffusion. Our simulations reveal that thermospheric winds effectively mix constituents in Titan's upper atmosphere.
I. C. F. Müller‐Wodarg, R. V. Yelle
openaire +1 more source

