Vaguery + astrophysics 3
[1110.4876] REBOUND: An open-source multi-purpose N-body code for collisional dynamics
january 2012 by Vaguery
REBOUND is a new multi-purpose N-body code which is freely available under an open-source license. It was designed for collisional dynamics such as planetary rings but can also solve the classical N-body problem. It is highly modular and can be customized easily to work on a wide variety of different problems in astrophysics and beyond.
simulation
computational-science
astrophysics
numerical-methods
simulator
library
open-source
nudge-targets
january 2012 by Vaguery
[1007.2774] Where is everybody? -- Wait a moment ... New approach to the Fermi paradox
july 2010 by Vaguery
"The Fermi Paradox is the apparent contradiction between the high probability extraterrestrial civilizations' existence and the lack of contact with such civilizations. In general, solutions to Fermi's paradox come down to either estimation of Drake equation parameters i.e. our guesses about the potential number of extraterrestrial civilizations or simulation of civilizations development in the universe. We consider a new type of cellular automata, that allows to analyze Fermi paradox. We introduce bonus stimulation model (BS-model) of development in cellular space (Universe) of objects (Civilizations). When civilizations get in touch they stimulate development each other, increasing their life time. We discovered nonlinear threshold behaviour of total volume of civilizations in universe and on the basis of our model we built analogue of Drake equation."
aliens
Fermi-Paradox
complexology
agent-based
astrophysics
SETI
july 2010 by Vaguery
[1006.4354] Empirical Modeling of Radiative versus Magnetic Flux for the Sun-as-a-Star
june 2010 by Vaguery
"…We find that a well-defined temporal component exists and accounts for some of the variance in the data. This temporal component arises because active regions with high magnetic field strength evolve, breaking up into small-scale magnetic elements with low field strength, and radiative and magnetic fluxes are sensitive to different active-region components. We generate empirical models that relate radiative flux to magnetic flux, allowing us to predict spectral-irradiance variations from observations of disk-averaged magnetic-flux density. In most cases, the model reconstructions can account for 85-90% of the variability of the radiative flux from the chromosphere and corona. Our results are important for understanding the relationship between magnetic and radiative measures of solar and stellar variability."
astronomy
astrophysics
modeling
learning-from-data
statistics
nudge-targets
june 2010 by Vaguery
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