剩餘壓縮 的英文怎麼說
中文拼音 [shèngyúyāsuō]
剩餘壓縮
英文
supercompression-
So this part is dealt with separately. dcpm method is employed to improve the quality of image coding with making full of the relativity of the wavelet coefficients. according to the different importance degree and vision character of the high frequency wavelet coefficients, different thresholds are applied to remove small coefficients ; then mannos module are applied to remove the visual redundancy ; in order to produce more zero - tree, horizontal and vertical wavelet coefficients are transformed accordingly to improve the compression ratio
對于小波變換后的小波系數的高頻部分，根據其分佈特性和人眼的視覺特性，採用視覺模型對零樹量化過程的閾值進行修正，有效地去除視覺冗餘；對各高頻子圖採用多級樹集合分割的零樹編碼方法，有效地利用系數編碼剩餘符號，進一步提高壓縮比。Nature of the universe - chapter seventeen if the remnant of a supernova explosion is heavier than two or three solar masses, the neutron degenerate pressure is not strong enough to support the star. there does not exist stronger force up to our knowledge and we believe the remnant will collapse to a black hole
在超新星爆發后，如果恆星剩餘質量超過二或三個太陽質量，中子簡並壓力亦不足以抵抗向內的引力，這時在已知的物理理論裏面，再沒有更強的力能足以與引力一決雌雄，恆星只可以不斷塌縮，成為黑洞。If the mass of the core after a supernova explosion is more than 1. 4 but less than about 3 solar masses, then electron degenerate pressure is not strong enough to support the star. the star will contract to a size even smaller than the white dwarf. the electrons are squeezed into the nuclei and are combined with the protons to form neutrons
假若在超新星爆發后，剩餘核心質量介乎太陽質量的1 . 4至3倍，那麼核心中的電子簡並壓力便再不足以抵抗強大的引力，恆星會進一步收縮，直至電子亦被擠壓至原子核內，和質子結合成為中子。The compression experiment after impact is discussed in the paper. also, the compression damage force after different impact energy and the strain response of different position are presented. it is a satisfying method for experimental research to find the strain distributing in impact and cai, as well as the compression strength of cai
同時本文還進行了沖擊后的壓縮試驗，對編織型復合材料在不同沖擊能量下的壓縮破壞載荷，及損傷后不同位置的響應進行了記錄和討論，是一個全面考察沖擊和沖擊后壓縮的應力分佈和研究破壞載荷及剩餘強度的較為滿意的實驗研究方法。分享友人