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Useful tips for vidders (fan video makers) for converting your video for YouTube, or for preparing clips for editing. Please note: All these tutorials show you how to convert your clips to a file format that is good for editing. If you wish to, trim down your clip to just the scene you want by picking in and out points. Under a€?Sound,a€? you can pick MPEG-4 AAC and select 128 kbps or above, or can select a€?No Sounda€? (like I have in this screenshot) and eliminate sound from your clip. Like with the tutorial above, open your file (this time an H.264 MOV file) in MPEG Streamclip.
In most cases you will have no sound, so Select a€?No Sound.a€? Otherwise, go with a€?Uncompresseda€? for sound. Quality can be a 100% but Apple Intermediate Codec only has one quality setting, so it doesna€™t seem to change anything when you fiddle with the quality setting. Then click on a€?Make Moviea€? and wait for MPEG Streamclip to convert your whole video over! You will follow the same process as outlined above, only instead of Apple Intermediate Codec, youa€™ll select some flavor of a€?ProResa€? from the Compression drop-down menu. If you have Final Cut Pro 6, youa€™ll probably only get to choose from ProRes 422 and ProRes 422 (HQ).
Choose the same settings for Frame Size and Sound as are used in the Apple Intermediate Codec tutorial. Please note again that when you convert your clips over to DV or MJPEG, that the files will be larger in size, and this is GOOD for editing. If you are downsizing a large HD clip to Standard Definition DV, then CHECK the a€?Better Downscalinga€? box. In most cases, pick a€?Progressivea€? as a€?Scan Modea€? (at least this is what I always do) and pick your Aspect Ratio. If you are converting some other kinds of clips, odds are (that if you are converting clips from a film or recent TV show) that the aspect ratio is still 16:9, but you need to confirm this. Then return to MPEG Streamclipa€™s main window, and click on the a€?Make AVIa€? or a€?Make Moviea€? button (bottom right corner) to have MPEG Streamclip convert the clip over to DV MOV or AVI. If you are converting some other type of clips, consult the aspect ratio tutorial for more help determining what aspect ratio to choose.
Click on a€?Better Downscaling,a€? since you are converting HD clips down to a smaller size. If you are converting some kind of non-HD clip and you know that they are fullscreen (4:3) then pick the numbers 640x480.
Click on the a€?Make Moviea€? or a€?Make AVIa€? button and wait for MPEG Streamclip to convert your clips over! So, leta€™s say that you have a lot of little clips and you want to convert them all over to some other format.
Click on the a€?Add Filesa€? button, then navigate through your computera€™s files for the clips that you want to convert over. Find the folder where the clips are, and then select one from the top of the list, HOLD DOWN THE SHIFT KEY and then select the clip at the bottom of the list. Check on the a€?Join all the filesa€? if you want all your clips to be joined into one long clip. Then youa€™ll be asked to a€?Select a Destination Folder.a€? This is where you want all your converted clips to be placed after MPEG Streamclip has finished making them. Then youa€™ll be asked all the familiar questions that you should know by now if youa€™ve followed the other MPEG Streamclip tutorials: Compression, frame size, and so forth. If this is all you want to convert over, click on the a€?Goa€? button and wait for MPEG Streamclip to do its thing. When you click on the a€?Converta€? button, wait while MPEG Streamclip converts, converts, converts! Tutorial keywords: MPEG Streamclip, MJPEG AVI, HD, converting video tutorial, fanvideos, fanvids, vidding tutorial, vids, vidders.
Once you pick your compression, MPEG Streamclip will automatically select a frame size which corresponds (either DV-NTSC or DV-PAL). A large body of experimental data now exists for (e,2e) differential cross section (DCS) ionisation studies in which the scattered and ejected electrons are detected with the same energy and at the 'same' asymptotic scattering angles with respect to the incident electron direction.
A detection plane spanned by the scattered and ejected electron momenta ka and kb is initially defined. The energy region from around 3eV to 100eV excess energy is defined here as the 'intermediate energy' region. Studies at lower energies are considered to lie in the threshold region where correlation effects between outgoing electrons dominate the reaction. Differential cross section studies at energies in excess of 100eV are predominantly governed by single binary collisions between the incident and ejected electrons, the core playing a decreasing role in the reaction as this energy increases. Common to all these models is the importance of correlations between the outgoing electrons brought about through electrostatic coupling as they emerge from the reaction zone (see figure 2). As the excess energy above ionisation decreases, the outgoing electrons have more time to mutually interact and so the probability that they will emerge asymptotically at a mutual angle of p radians increases, whereas their 'memory' of the incident electron direction correspondingly decreases. In this page a model-independent parameterisation of the ionisation differential cross section is discussed. The parameterisation is in terms of a complete orthogonal set of irreducible tensorial angular functions which define correlation between any three vectors in space.
This parameterisation was first proposed for the (e,2e) process by Klar and Fehr (1992), and has a long and distinguished history in the field of nuclear particle interactions proceeding through sharply defined states, where the analysis gives information about the angular momenta carried into and out of the reaction. By contrast, in the (e,2e) reaction the intermediate state is not normally sharply defined, and so the parameters do not directly reveal the angular momenta associated with the reaction, but rather indicate the degree of correlation between ingoing and outgoing electrons. The (e,2e) differential cross section is parameterised as a coherent superposition of partial waves up to L = 2 defining scattering in the reaction zone which is modulated by a Gaussian function modelling correlations between the outgoing electrons.
There is no evidence of the complex structure discussed above for the intermediate energy regime.
Comprehensive experimental data exists for ionisation of helium in the intermediate energy region over a very wide range of scattering geometries. In these results the DCS is assumed to be zero when x = 0 and x = p since the probability of detection of two electrons of equal energy emerging in the same direction is very small.
At 1eV excess energy a single structure is observed due to strong outgoing electron correlation, as previously noted. At 3eV and 5eV above ionisation both a forward and a backward structure start evolving from the central peak at low incident electron angles y, whereas at higher angles y the DCS is still approximately Gaussian.
Backward scattering, probably dominated by elastic scattering of the incoming electron from the atom into the backward direction in the detection plane followed by a binary collision with a valence electron, is the dominant contribution to the overall DCS structure. At the higher excess energy (30 - 50eV) forward scattering starts to dominate, reflecting the importance of single binary collisions. Only the central peak is attainable through a single collision process and there will additionally be significant contributions to this peak through outgoing electron correlations at the lower energies.
Indistinguishability of the outgoing electrons requires the DCS at (y,x) to be equated to that at (y, 2mp-x) where m is an integer.
Reflection symmetry is necessary in the detection plane since no preferred direction is defined with respect to this plane, and hence s(y,x) = s(-y,x). When electron spin is not considered the (e,2e) differential cross section is a function only of the momenta of the ingoing and outgoing electrons.

The choice of angular functions Ilalbl0 required to characterise the (e,2e) DCS is restricted by the symmetries inherent in the ionisation process. Here the set for which la = lb when l0 is even and (la,A l0)A < lb when l0 is odd is chosen.
It is clear that plotting the absolute magnitude of the I110 function as a radial vector when scanning over all possible values of theta and phi produces a 3-D surface which represents the function. Since the magnitude can be positive as well as negative, it is important to represent this facet when describing the function in this way. It is necessary to consider the magnitude and sign of the functions as the (e,2e) Differential Cross Section is parameterised as a linear sum of the angular functions (see equation 6), and so for various values of theta and phi the functions can cancel each other to allow zeroes in the cross section. The complete set of 3-D images of the 44 Angular Functions Ila,lb,l0 required to parameterise the symmetric (e,2e) Differential Cross Section over the energy range from 1eV to 50eV above the Helium ionisation threshold have been generated.
The summation is over the experimental data points i each with an associated weight wi evaluated from the uncertainty in the data. This linear fitting was fast and reliable, yielding excellent starting parameters for the second non-linear fitting method. A Simplex method was used to minimise the c2 function by adjusting the Blalbl0 parameters (see figure 7). Any trial for which the fitting function did not obey the assumptions was rejected and the Simplex routine was reset to explore alternative regions of the c2 surface.
This method converges far more slowly than the linear fitting method but requires no inferred data. The maximum significant values of la, lb and l0 were established using a statistical F-test. At 1eV excess energy only l0 = 0 to 4 contribute, and the la and lb terms are all of the same sign, reinforcing each other in each l0 manifold.
The relative magnitudes of the terms in each manifold combine to produce the lobe structure at the mutual angle of p radians. As the energy increases this regular pattern quickly disappears as the forward and backward lobes evolve from the central 'Gaussian' profile. Higher order l0 correlation terms become significant as the intermediate energy region is entered, indicating an increasing contribution of higher order partial waves to the DCS. Additionally the la and lb terms start to compete in magnitude and sign to produce the more complex structures observed. At excess energies above about 30eV the parameters tend to stabilise in sign and vary smoothly with energy. The maximum significant number of la and lb terms in each l0 manifold also decreases as the energy increases, indicating that the number of partial waves required in the outgoing channel decreases with increasing energy. Figure 9 shows 3-D representations of the (e,2e) differential cross sections at each energy from 1eV to 50eV excess energy as obtained from fitting the data to the parameterisation. The 3-D surface is generated from a vector whose length is given by the magnitude of the differential cross section as the surface is generated throughout space for all angles (q,f). The backward scattering region is towards the viewer, whereas the forward scattering region is away from the viewer. The results shown in figure 9 show 3 dimensional representations of the (e,2e) differential cross sections derived from the parameterisation at the energies where experiments were conducted. It is useful to establish a technique which allows interpolation between these results at the eight discrete excess energies, to enable the differential cross section to be estimated as a function of the three angular and one energy variables over the complete range of energies from threshold to 50eV excess energy.
The (e,2e) differential cross section s is then projected onto a four dimensional space, whose axes are defined by the independant variables (s, q,f & Eexc). As this cannot be visualised as a single projection on these pages, it is instructive to map one of these variables onto the time co-ordinate.
In this case, we choose the excess energy to be varied in time, whereas the other 3 variables are mapped onto conventional 3-dimensional co-ordinate space, as has been done in the previous figures.a€?Hence, once the DCS is parameterised as a function of energy as well as a function of the scattering angle, this parameterisation can be used to derive 3-D images at discrete energy intervals. These images can then be projected as a moving film, where the time from the start to the end of the film depicts the energy change from 1eV to 50eV excess energy.
A cubic spline is interpolated through the parameters as a function of the ratio of excess energy to the ionisation energy of 24.6eV. These are fitted using a ninth order polynomial fit which closely emulates the cubic spline through the data.
Details of these cubic spline fits to the Blalbl0 parameters can be found by accessing the appropriate interlink page splinefit.htm. The b-parameters which define the normalised DCS as a function of energy and angle can be downloaded here as a text file. Although the b-parameters do not have a direct physical meaning, they allow the normalised DCS surfaces to be generated at any energy from 1eV to 50eV as has been discussed. 100 of these images have been generated at 0.5eV intervals, and compressed into a Quicktime movie. Note that these files are around 3MB in size, so may take some time to download should internet access be busy. Additionally the evolution of the 44.6eV DCS as successive angular functions are added together can be seen! MOV and QT formats will not be a problem anymore, regardless of the media player or Internet browser you are using. Once you install the QuickTime Alternative codec, you will also have the Media Player Classic application deployed on your computer. Another caution you need to take is uninstalling all previous QuickTime related products to prevent errors. In conclusion, this small-sized virtual item is a simple and fast solution for those who want to play QuickTime formats like MOV, QT or 3GP hassle-free and without deploying on their computers software they are not otherwise interested in. The only difference between the regular and lite versions is that the lite version does not include Media Player Classic. Avid Codecs Light Edition: allow systems to encode and decode QuickTime movies and references using Avid codecs. I did bootleg a couple of tracks, which aren’t of any quality to threaten ATF sales, but might give a wee flavour of the live sound.
There have been a few reviews of the gigs in their recent tour already, and I wouldn’t presume to be any great music critic.
I had heard Rob Halligan stand in for a couple of numbers at a largely accoustic set at Greenbelt a while back, and I wasn’t sure that it quite worked. You are *required* to use the date.timezone setting or the date_default_timezone_set() function.
To follow this tutorial, download the free video encoding app MPEG Streamclip (for both Mac and PC). This tutorial may be useful for some Windows users, particularly those using Sony Vegas and Corel VideoStudio.
Expect to use up approximately 1 GB of disk space for every 5 minutes of footage (more or less). If you need audio (and your clip has audioa€”some might not), then choose a€?Uncompresseda€? for Sound.
Well, if you are using software that doesna€™t support HD (like Sony Vegas Movie Studio, non-Platinum version) or you have a slower computer that might not deal with HD that well, then this might become necessary. Smaller clips (like DivX, XviD, H.264, WMV, MPEG) are compressed and do not play well in your video editor, and can eventually cause crashing or other quality issues. It works best if all the clips you want to batch convert are in the same folder (but they can be in various places if that works better for you).

Or, if you just want to convert select clips, hold down the Apple (Command) key (Mac) or the Control key (PC) to cherry-pick just the clips you want. If youa€™ve been following the above tutorials, you will know if you want to convert to MOV, AVI, or whatever. In this case, Ia€™m going to convert to Quicktime (MOV files) but you can convert to AVI, MP4, iPod, just whatever you need.
Select whatever options work best (consult the above instructions on this page if necessary). Otherwise, click on a€?Add Filesa€? and locate more clips you want to convert over, repeating the process until youa€™ve added as many files as you need to the list. You can leave your computer to convert overnight, or just be busy with other things as it finishes converting all your files.
It shows the quality differences between a€?regulara€? resolution, a clip made from HD (but converted a€?downa€? to DV MOV or DV AVIa€”as instructed on this page) and a real HD clip. These experiments have recently been carried out principally by two groups at Kaiserslautern group and at Manchester (see references for examples). This region is now successfully modelled to a large degree using the Born approximation and its associated derivatives.
Although theoretical interest in this region is increasing, no theory adequately explains the experimental data accumulated so far.
The Paris coplanar and Manchester Perpendicular plane results at an excess energy of 1eV ionising Helium as the target. In the experimentally inaccessible regions centred at x = 0A° and x = p the DCS is constrained to be positive and to have no points of inflection, and at the angles x = 0A° and p themselves the DCS is put equal to zero. The choice of la, lb and l0 used to define the subset is arbitrary within the constraint that the angular functions must be unrelated.
These images are established by plotting the magnitude of the angular function against the angles theta and phi that are defined in the function. These artificially generated points were given low weighting to minimise the constraints placed upon the fit. Consideration of the data sets at all excess energies established that 44 angular functions up to la, lb = 7 and l0 = 6 gave the best overall fit to the data. The fitting parameters can be downloaded as a TAB deliminated text file by linking to the file Blalbl0.dat. Further information can be obtained by linking from the figures to the appropriate WWW page. 3-D representations of the DCS calculated from the fitted parameters Blalbl0 for the 8 data sets from 1eV to 50eV.
The 3D Quicktime movie can be downloaded at the end of this page by linking to the appropriate file.
You can open a simple window for configuring QuickTime Alternative whenever it is necessary. I understand he has something in the pipeline to fill that gap in future – I look forward to hearing how that works out! Then again, that was fitting as it was a FairTrade, Stop the Traffik gig with a really very good support slot from Julie Hall. But was this a sort of high-class karaoke with a live band, or a sort of hybrid between a reformation and a tribute band? In case you used any of those methods and you are still getting this warning, you most likely misspelled the timezone identifier. Then move the slider bar to your out point, press the a€?Oa€? key to set where you want the clip to end. This is normal and expected and for a more seamless, stable editing experience, you WANT to edit in files of this size. The differences between the a€?regulara€? clip (from XviD source) and HD should be obvious. The Wannier model parameterisation transformed to the (y,x) geometry is shown as a fit to the data. The function can either be positive or negative depending upon the value of theta and phi, and the sign is therefore represented by two colours, PURPLE indicating a positive magnitude and RED representing a negative magnitude.
The example here shows the method for finding the minimum of a 3-D Gaussian function of the form z = - exp(-x^2 + y^2).
Higher resolution images together with a downloadable EPS file for each of the data sets can be obtained by linking to either of the above low resolution images. Can there be a genuine ATF without Andy Piercy – where even if he is 25 years absent in person, he is still present in the sound he created still being in essence ATF? For an explanation for why this is necessary (and why editing in the smaller-sized XviD AVI, DivX AVI, WMV, MPEG, MP4 or other compressed file types is a bad idea), read this tutorial. Smaller, more compressed video files (like DivX AVI, XviD AVI, WMV) will give your software problems (either now or later on down the road). The differences between the a€?reala€? HD clip and the a€?HD converted down to DV MOVa€? may not be quite as obvious, depending on how sharp your eye is and your monitor resolution. The differences between theA  a€?reala€? HD clip and the a€?HD converted down to DV MOVa€? may not be quite as obvious, depending on how sharp your eye is and your monitor resolution. This electron, and the incident electron that has lost almost all of its energy in the reaction have similar energies and therefore as they emerge from the reaction zone feel the Coulombic influence of each other and the ion core following ionisation. The scattering is more complex than in the threshold region, since the incident electron can penetrate deeper into the neutral target electron cloud, and therefore there is more complex interactions between the electrons and the core. The Simplex, in this case a 2-D triangle whose vertices are defined by points on the surface, proceeds by reflection, contraction, expansion or shrinking along the surface as shown. Rob Haligan is also more than just a Piercy mimic, adding in some of his own material to the sets, and just a little of his own inflections.
The low relative velocity of the electrons allows them to mutually interact for sufficient time to tightly correlate their respective asymptotic directions. There is now a finite probability of exchange, capture, ingoing and outgoing correlations between all charged particles in the reaction.
I think they tried that back at Greenbelt a few years ago – heroic, however, much as I love them, it really did not quite hit the mark.
ATF have re-worked an oldie (One Rule for you – Trade Justice), and have started to embark on some new material too. This leads to both forward and backward scattering possibilities, depending upon the complexity of these interactions. Whether deliberately or not, the band have managed to create a very authentic 80-F sound and feel. Keith Smith also joined the for a time, and whilst being a very competent singer, didn’t look or sound at ease in the role of lead singer.
And I love the way at recent gigs there have been new young fans evident amongst those of grey-ing hair and no hair. Double continuum wave functions and threshold law for electron atom ionisation, Physics Review A.

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