在PowerPoint演示文稿中轻松插入Flash动画

用PowerPoint制作出的幻灯片简洁明快、条理清晰,而且PowerPoint简单易用,非常适合教师上课使用,成为教师制作多媒体课件的工具之一(在我校大部分教师采用PowerPoint制作多媒体课件).在制作多媒体课件过程中,结合适当的媒体技术(动画、声音、文字)不仅能提高课件的直观生动性,激发学生学习兴趣,同时有助于学生对课堂知识的当堂消化和理解,加深记忆.通过我校开展多媒体教学多年的实践发现:对医科学生的基础课、专业基础课和专业课教学中广泛涉及的机能性、原理性的知识适当采用动画其教学效果是传统教学方法无法比拟的.在众多的动画媒体中(avi、mov、mpg、swf、gif、ram等),Flash动画(swf文件)以其作品容量小(单个swf文件通常不到100 K)、质量高和丰富的交互性,特别是近年推出的Flash5同时能结合视频和音频,成为目前最为流行的二维动画.不仅为网页制作增添了活力,同时也为多媒体制作提供了有效的手段,既精巧又实用,素有"闪客"、"动画精灵"之美誉,越来越受到人们的青睐.如果要把Flash制作好的动画插入到PowerPoint制作的课件中,将会使PowerPoint单调的动画增色不少,使课件更具魅力.为此,我校专门开展了一系列Flash动画制作讲座,广大教师都能结合本专业制作Flash动画.如何将Flash动画加入到PowerPoint中,不少教师都是直接通过"超级连接"导入Flash课件,放映时总会出现讨厌的警告信息和警告声音提示,点击确定后打开Flash课件,有时打开的Flash课件窗口还要重新调整,使用十分不便.如何才能更恰当地引入Flash动画呢?不少杂志刊物和网上发表过类似文章,但大都比较复杂,而且在使用中特别是在PowerPoint中放映Flash动画偶尔会出现这样和那样的问题,这也是我们教学工作中经常遇到的问题,具有一定的普遍性.经过与教师们的众多交流和笔者平时反复摸索,找到了较为简便有效的方法,写出来与大家分享.     

简易动画机的制作

青少年都非常喜欢动画片,为了使他们了解电影、电视中动画的视觉暂留原理,并且能够自己动手制作简易动画机,自行设计创作各种动画,进而培养学生的创新精神和实践能力.因此,开发研制了一种主要利用可乐瓶制作的“科教简易动画机”.1　原理结构科教简易动画机主要根据人眼对图象可以停留0.1s的视觉暂留原理和巧妙的顶针式转动机构设计研制的.该作品由转桶部分、底座部分、动画部分构成.具体结构如图1所示.图1　简易动画机的结构示意图1.长条孔带2.竖直条形动画3.水平圆形动画4.圆盘5.粘接剂6.底板7.瓶底8.顶针轴9.车条帽10.转桶1.1　转桶部分…     

光学实验网络课件的设计

实验类教学的网络多媒体课件制作是目前多媒体课件制作中的一个难点，本将介绍光学实验的迈克尔逊干涉仪实验教学的FLASH制作，通过该介绍提出作制作实验类网络教学软件的思路。     

用Authorware制作日食、月食的动画

物理教学中常用三球仪演示地球、月球绕太阳运行的情况,由于三球仪水平放置,教室里坐在后排的学生不易看清,演示效果不理想.笔者试用Authorware制作日食、月食的动画,演示效果很好.下面介绍该动面的制作及演示方法.     

大学物理波动光学仿真演示实验的设计与实现

根据波动光学的实验原理 ,利用Flash动画制作仿真虚拟演示实验 ,然后导入Authorware设计的系统框架中 ,该虚拟实验系统特别适合实验设备条件较差的学校在课堂教学中使用。     

大学物理演示实验的价值重构

在创新教育的视角下审视物理演示实验,从创新教育、情境教学设计、创新能力评价和科学普及4个方面对演示实验的价值进行重构.学生制作和创作并重,结合内部动机和外部激励,逐步培养学生动手能力和创新能力;优化已有的演示实验,根据情境教学法编制系列情境演示实验;为选拔具有创新意识学生,设计评价性实验;利用演示实验的独特优势进行科学...     

Flash在示波器实验教学中的应用

通过介绍利用FLASH制作仿真示波器实验时的特点,说明FLASH可以作为一个非常有用的工具,在电磁学实验教学中起到重要的辅助作用.     

用Flash动画和旋转矢量法模拟简谐振动

动作补间、形状补间和遮罩是Flash动画制作中几种常用的技术,本文基于Macromedia公司的动画制作软件Flash6．0,并利用这几种技术,设计完成了一种用旋转矢量法演示弹簧振子运动轨迹的动画制作方案．     

空气有害气体监测演示系统

设计和制作了空气常见有害气体的监测演示实验系统,介绍了有害气体实时监测的原理和过程.实验结果表明:监测结果迅速、准确,并提供了友好的人机交互界面和报警系统.     

磁流变液演示仪

为了清楚地演示磁流变现象,设计并制作了磁流变液演示仪.文章主要介绍了演示仪的工作原理、结构设计及演示方案.     

关于"太阳在银河系中所受引力与到银心距离r的关系"的讨论

讨论了银道面内的引力场强分布和太阳在银河系中所受引力与到银心距离r的关系，指出引力场强g并不是与r的平方成反比，这是由于银河系的大小和形状不能忽略造成的．强调了万有引力定律的适用条件．     

On the calculation of the bremsstrahlung in the region of the plasma frequency

On the basis of the classical theory of radiation produced in incomplete Coulomb interaction, a formula is derived for the coefficient of the bremsstrahlung of fully ionized plasma. In the region of rectilinear approximation a comparison is made with the results of the quantum formula derived from the Born approximation. Furthermore, the influence of dispersion upon the emission coefficient is taken into account; some relations for the region of dispersion are given.     

On the predictability of the positions of the convergence zones in the ocean

The disagreement between the experimental and calculated positions of the first convergence zone are known from many publications. The most probable cause for such a disagreement, namely, the incorrect specification of the input data for the calculations, is considered. The lack of simultaneity between the hydrological surveys of the region and the acoustic experiments is emphasized. The experimental data obtained by the author in five ocean regions are presented. These data characterize the diurnal variability of the distance from the source to the nearest boundary of the convergence zone. The relations proposed by different researchers for calculating the sound speed from the temperature, salinity, and hydrostatic pressure are analyzed. It is shown that these relations lead to a substantial difference in the estimated depth dependence of the hydrostatic gradient of the sound speed. The position of the first convergence zone is calculated for the propagation conditions determined by vertical temperature and salinity profiles with the subsequent recalculation of these profiles into sound speed profiles by using eight different formulas known from the literature. It is shown that different formulas lead to different values of the distance to the first zone; this difference is substantially greater than that between the calculations and experiment. The necessity of improving the recalculation relations in view of the experimental data on sound propagation in natural oceanic waveguides, including the data on the actual positions of the convergence zones, is emphasized.     

Dependence of the Intensity of the Spectral Lines and the Composition of the Sample and the Plasma Parameters of the Unipolar Arc

The investigation was made of the dependence of the intensity of Tl, Ga, Mo, Mg, Mn, Sn, Bi, Ni, Zn, Pt and Au spectral lines and the plasma parameters (temperature T, electron concentration n_e, degree of 6 ionnization α) from concentration of lithium additive.     

Extracting the wavefunction of the LSP at the LHC

We consider associated production of squarks and gluinos with the lightest supersymmetric particle (LSP), or states nearly degenerate in mass with it. Though sub-dominant to pair production of color SU(3)-charged superpartners, these processes are directly sensitive to the wavefunction composition of the lightest neutralinos. Exploiting event-shape variables - including some introduced here for the first time - we are able to identify the composition of the LSP by selecting events involving a single high-pT jet recoiling against missing transverse energy. We illustrate the proposed technique on a set of benchmark cases and propose methods for applying these results in more realistic experimental environments.     

Set the controls for the heart of the Sun

In this paper we describe experiments conducted with high-power lasers that are attempting to replicate, for a very short time and in miniature, conditions found in the Sun. Experiments to date have reached conditions in the outer part of the Sun. To reach the Sun's centre requires compression of material to very much greater than solid density and heating to over ten million degrees. To achieve this, a new class of experiments and a new generation of high-power lasers are required.     

On the Question of the Source of the Apokamp

Technical Physics - The object of this work is the apokamp—a new type of plasma jet, which is formed from a bright offshoot emerging at the bending point of a channel of a high-voltage...