中国科学技术大学学报
中國科學技術大學學報
중국과학기술대학학보
JOURNAL OF UNIVERSITY OF SCIENCE AND TECHNOLOGY OF CHINA
2006年
3期
320-327
,共8页
谢启源%张永明%袁宏永%赵建华%乔利锋%蒋亚龙
謝啟源%張永明%袁宏永%趙建華%喬利鋒%蔣亞龍
사계원%장영명%원굉영%조건화%교리봉%장아룡
感烟探测%非球形性%光散射%回转椭球模型%T矩阵法
感煙探測%非毬形性%光散射%迴轉橢毬模型%T矩陣法
감연탐측%비구형성%광산사%회전타구모형%T구진법
smoke detection%nonsphericity%light scattering%spheroid model%T-matrix method
针对火灾烟颗粒的链状结构特征,采用回转椭球模型,通过"T矩阵法",分析其非球形性对光散射模式的影响.分别在固定取向与随机取向条件下,分析了"扁长"形回转椭球、球体及"扁圆"形回转椭球的散射光强分布.结果表明,在固定取向情况下,半轴比值a/b=1.0的球体对应的散射光强度分布的等高线均为直线;然而,对于半轴比值a/b<1.0的"扁长"形椭球体对应的散射光强度分布的等高线为凸线,半轴比值a/b>1.0的"扁圆"形椭球体对应的散射光强度分布的等高线为凹线.在随机取向条件下,球体(a/b=1.0)对应的取向平均散射光强度分布曲线的震荡最为剧烈,而a/b=0.5,2.0,4.0对应的三条曲线表明,非球形性越强的颗粒对应的散射光强分布曲线越平滑.
針對火災煙顆粒的鏈狀結構特徵,採用迴轉橢毬模型,通過"T矩陣法",分析其非毬形性對光散射模式的影響.分彆在固定取嚮與隨機取嚮條件下,分析瞭"扁長"形迴轉橢毬、毬體及"扁圓"形迴轉橢毬的散射光彊分佈.結果錶明,在固定取嚮情況下,半軸比值a/b=1.0的毬體對應的散射光彊度分佈的等高線均為直線;然而,對于半軸比值a/b<1.0的"扁長"形橢毬體對應的散射光彊度分佈的等高線為凸線,半軸比值a/b>1.0的"扁圓"形橢毬體對應的散射光彊度分佈的等高線為凹線.在隨機取嚮條件下,毬體(a/b=1.0)對應的取嚮平均散射光彊度分佈麯線的震盪最為劇烈,而a/b=0.5,2.0,4.0對應的三條麯線錶明,非毬形性越彊的顆粒對應的散射光彊分佈麯線越平滑.
침대화재연과립적련상결구특정,채용회전타구모형,통과"T구진법",분석기비구형성대광산사모식적영향.분별재고정취향여수궤취향조건하,분석료"편장"형회전타구、구체급"편원"형회전타구적산사광강분포.결과표명,재고정취향정황하,반축비치a/b=1.0적구체대응적산사광강도분포적등고선균위직선;연이,대우반축비치a/b<1.0적"편장"형타구체대응적산사광강도분포적등고선위철선,반축비치a/b>1.0적"편원"형타구체대응적산사광강도분포적등고선위요선.재수궤취향조건하,구체(a/b=1.0)대응적취향평균산사광강도분포곡선적진탕최위극렬,이a/b=0.5,2.0,4.0대응적삼조곡선표명,비구형성월강적과립대응적산사광강분포곡선월평활.
A spheroid model was used to characterize the nonspherical morphology of smoke aggregates with an axis ratio a/b. Using the T-matrix method, the relative intensity distributions of the scattered light were analyzed for four spheroids with different a/b in a fixed orientation, as well as in a random orientation. The results indicate that the magnitude contours of the scattered light intensity distribution for spherical particles are straight lines. The corresponding magnitude contours of light scattering patterns would be convex for prolate spheroids (a/b < 1) and be concave for the oblate spheroids (a/b > 1) . The results also show that the orientation-averaged scattered light intensity distribution for a sphere (a/b= 1.0) oscillates much more strongly than those for the other spheroids with a/b of 0. 5, 2.0 and 4.0. The oscillation of orientation-averaged scattered light intensity distributions is an indication for nonspherical particles.