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Depth profiling analysis of solar wind helium collected in diamond-like carbon film from Genesis
solar wind depth profile helium NASA Genesis mission post-ionization
2017/4/10
The distribution of solar-wind ions in Genesis mission collectors, as determined by depth profiling analysis, constrains
the physics of ion-solid interactions involving the solar wind. Thus, they pro...
Full revision of“单元纯系宇宙”and "Homogenous Cosmos Originated from Unique Genesis
PNT惠合系 单元纯系宇宙
2015/6/4
作为认识历史延续，“单元纯系宇宙”是从传统科学有关“物质微观结构趋同性”认识积蓄中延伸出来的“宇宙重认识和重定义”，——源自“宇宙单元纯系假设”、关于整个宇宙构造及其宇宙物质性存在与运动变化的“单一线性逻辑体系”。它将传统科学有关“物质微观结构趋同性”认识积蓄兑现至“宇宙单元纯系假设”，继而将宇宙内涵“时空”与“物质”代入“宇宙单元纯系假设”，导出时空与物质间的纯系性“PNT关系(或PNT行为)”...
Genesis of the dusty Universe: modeling submillimetre source counts
galaxies: evolution – galaxies: general – galaxies: starburst – infrared:galaxies – submillimetre: galaxies
2011/10/13
We model the evolution of IR galaxies using a phenomenological approach to match the observed source counts at different IR wavelengths. We introduce a new algorithm for reproducing source counts base...
We propose a unified theory of dark matter (DM) genesis and baryogenesis. It explains the observed link between the DM density and the baryon density, and is fully testable by a combination of collid...
The Genesis of an Impulsive Coronal Mass Ejection observed at Ultra-High Cadence by AIA on SDO
Impulsive Coronal Ultra-High Cadence AIA on SDO
2011/1/11
The study of fast, eruptive events in the low solar corona is one of the science objectives of the Atmospheric Imaging Assembly (AIA) imagers on the recently launched Solar Dynamics Observatory (SDO),...
Genesis and evolution of dust in galaxies in the early Universe I. Modeling dust evolution in starburst galaxies
galaxies high-redshift – galaxies starburst – galaxies evolution – ISM evolution – quasars general – stars massive
2010/11/16
Aims. The aim is to elucidate the astrophysical conditions required for generating large amounts of dust in massive starburst galaxies at high redshift.