搜索结果: 1-14 共查到“太阳与太阳系 models”相关记录14条 . 查询时间(0.13 秒)
Self-bound models of compact stars and recent mass-radius measurements
Self-bound models compact stars recent mass-radius measurements
2011/10/20
The exact composition of a specific class of compact stars, historically referred to as "neutron stars", is still quite unknown. Possibilities ranging from hadronic to quark degrees of freedom, includ...
Constraints on dark matter models from a Fermi LAT search for high-energy cosmic-ray electrons from the Sun
Cosmic Rays Electrons Fermi Sun
2011/10/13
During its first year of data taking, the Large Area Telescope (LAT) onboard the Fermi Gamma-Ray Space Telescope has collected a large sample of high-energy cosmic-ray electrons and positrons (CREs). ...
Dynamical Opacity-Sampling Models of Mira Variables. II: Time-Dependent Atmospheric Structure and Observable Properties of 4 M-Type Model Series
stars: AGB and post-AGB, stars: atmospheres, stars: variables: other, stars: mass loss
2011/10/11
We present 4 model series of the CODEX dynamical opacity-sampling models of Mira variables with solar abundances, designed to have parameters similar to $o$ Cet, R Leo and R Cas. We demonstrate that t...
Models of Solar Irradiance Variations: Current Status
Sun activity faculae plages magnetic fields solar irradiance solar-terrestrial relations sunspots
2010/9/15
Regular monitoring of solar irradiance has been carried out since 1978 to show that solar total and spectral irradiance varies at different time scales. Whereas variations on time scales of minutes to...
Global Solar Dynamo Models: Simulations and Predictions
Sun magnetic fields solar cycle dynamo predictio
2010/9/15
Flux-transport type solar dynamos have achieved considerable success in correctly simulating many solar cycle features, and are nowbeing used for prediction of solar cycle timing and amplitude.We firs...
New numerical models on giant planet formation
giant planet formation New numerical models
2009/6/25
New numerical models on giant planet formation。
Photoionization models of NGC 346。
Effects of cspn models on pn shell modeling。
Implications of dust for the radiation spectrum of shell-type pn models
radiation spectrum shell-type pn models
2009/6/11
Implications of dust for the radiation spectrum of shell-type pn models。
Photoionization dusty models of the planetary nebula NGC 6302
Photoionization dusty models planetary nebula NGC 6302
2009/6/8
Photoionization dusty models of the planetary nebula NGC 6302。
MHD modeling of the Heliosphere：a critical evaluation of different models
Heliosphere critical evaluation
2009/5/27
The very complicated problem of the solar wind-interstellar medium interaction requires a very sophisticated numerical approach. To achieve such a goal first we need to understand very deeply the resu...
Excitation of Solar-like Oscillations：From PMS to MS Stellar Models
Turbulence convection oscillations excitation sun stars:α Cen A—stars:main and pre-main sequence stars
2009/5/12
The amplitude of solar-like oscillations results from a balance
between excitation and damping. As in the sun, the excitation is attributed
to turbulent motions that stochastically excite the p mode...
Models of Solar Irradiance Variations：Current Status
Sun: activity, faculae, plages, magnetic fields solar irradiance solar-terrestrial relations sunspots
2009/5/6
Regular monitoring of solar irradiance has been carried out
since 1978 to show that solar total and spectral irradiance varies at different
time scales. Whereas variations on time scales of minutes ...
Global Solar Dynamo Models：Simulations and Predictions
Sun magnetic fields: solar cycle dynamo prediction
2009/5/5
Flux-transport type solar dynamos have achieved considerable
success in correctly simulating many solar cycle features, and are nowbeing
used for prediction of solar cycle timing and amplitude.We fi...