From: owner-fractint-digest@lists.xmission.com (fractint-digest) To: fractint-digest@lists.xmission.com Subject: fractint-digest V1 #85 Reply-To: fractint-digest Sender: owner-fractint-digest@lists.xmission.com Errors-To: owner-fractint-digest@lists.xmission.com Precedence: bulk fractint-digest Wednesday, January 21 1998 Volume 01 : Number 085 ---------------------------------------------------------------------- Date: Tue, 20 Jan 1998 21:25:01 -0600 From: "Tim Wegner" Subject: Re: (fractint) simplegif Wizzle asked: > I've looked at what I have in my Fractint directory and I appear to have a > 1993 version of simplgif.exe. Is there a newer release and where is it > available? I checked at the Spanky site and didn't see it there for > download. Try ftp://ftp.phoenix.net/pub/USERS/twegner/simplgif.zip for a much improved version. Don't upload it anywhere, it's still experimental. I hope to finish making it reck solid in a few weeks. The encoder is rock solid but the decoder, while good, has a few flaws. I will do a decoder transplant. Tim - - - ------------------------------------------------------------ Thanks for using Fractint, The Fractals and Fractint Discussion List Post Message: fractint@xmission.com Get Commands: majordomo@xmission.com "help" Administrator: twegner@phoenix.net Unsubscribe: majordomo@xmission.com "unsubscribe fractint" ------------------------------ Date: Tue, 20 Jan 1998 21:25:01 -0600 From: "Tim Wegner" Subject: Re: (fractint) Lee's Truecolor PNG site Paul wrote: > PNG Live(tm) is a plugin for Netscape Navigator and Microsoft Internet > Explorer that allows you to see PNG (Portable Network Graphics) images > directly in your web browser. True, but the latest beta versions of both Netscape and Internet Explorer support PNG instrinsically. For example, I am using Netscape 4.04, which I can verify does support PNG. Tim - - - ------------------------------------------------------------ Thanks for using Fractint, The Fractals and Fractint Discussion List Post Message: fractint@xmission.com Get Commands: majordomo@xmission.com "help" Administrator: twegner@phoenix.net Unsubscribe: majordomo@xmission.com "unsubscribe fractint" ------------------------------ Date: Tue, 20 Jan 1998 19:59:56 -0800 From: Wizzle Subject: Re: (fractint) simplegif Tim... sounds painful....please let me know when it is ready as Bill in NY helped me understand the nifty things it could do. I very much want to experiment with having some of my fractals printed ......and would like to start "small" with a local printer and then move on to a more expensive processes. Being part of this email list is great ..... Angela At 09:25 PM 1/20/98 -0600, you wrote: >Wizzle asked: > >> I've looked at what I have in my Fractint directory and I appear to have a >> 1993 version of simplgif.exe. Is there a newer release and where is it >> available? I checked at the Spanky site and didn't see it there for >> download. > >Try ftp://ftp.phoenix.net/pub/USERS/twegner/simplgif.zip > >for a much improved version. Don't upload it anywhere, it's still >experimental. I hope to finish making it reck solid in a few weeks. >The encoder is rock solid but the decoder, while good, has a few >flaws. I will do a decoder transplant. > >Tim > > >- >------------------------------------------------------------ >Thanks for using Fractint, The Fractals and Fractint Discussion List >Post Message: fractint@xmission.com >Get Commands: majordomo@xmission.com "help" >Administrator: twegner@phoenix.net >Unsubscribe: majordomo@xmission.com "unsubscribe fractint" > > - - - ------------------------------------------------------------ Thanks for using Fractint, The Fractals and Fractint Discussion List Post Message: fractint@xmission.com Get Commands: majordomo@xmission.com "help" Administrator: twegner@phoenix.net Unsubscribe: majordomo@xmission.com "unsubscribe fractint" ------------------------------ Date: Tue, 20 Jan 1998 23:00:35 -0500 From: "Blake Hyde" Subject: (fractint) RandMap v0.51 I have finished RandMap 0.51, and it'll be the last release for a long while. (Life calls) It offers easily managed color bands (yes, they work now) as well as everything the old ones did -- greyscale, black background by default, etc. If you find any bugs, send them to me. I think this utility can actually help people... www.connectu.net/bhyde/rm051.zip Or go to my fractal homepage and click the first link in the body of that page. Blake Hyde ~ Casper ~ Novan Dragon Homepage: www.connectu.net/bhyde Fractals: www.connectu.net/bhyde/fractal.htm Email: bhyde@connectu.net - - - ------------------------------------------------------------ Thanks for using Fractint, The Fractals and Fractint Discussion List Post Message: fractint@xmission.com Get Commands: majordomo@xmission.com "help" Administrator: twegner@phoenix.net Unsubscribe: majordomo@xmission.com "unsubscribe fractint" ------------------------------ Date: Tue, 20 Jan 1998 20:06:53 -0800 From: Wizzle Subject: Re: (fractint) Lee's Truecolor PNG site I have to stand with Rich on this one......and say that plugins are NOT the same as support for a format. I have the required software to view PNG....not the issue. I think the issue is....correct me here Rich......we will be hampered with web posting until Netscape takes that next step and gives the same support to png as it does to gif and jpg. I recall reading early last year about how png was the coming thing.....but it wasn't incorporated into Netscape version 4.0. Should we lobby Netscape?? can we leverage the Great Browser Wars?? Angela At 08:48 PM 1/20/98 -0600, you wrote: >Rich Thomson wrote: >> >> It is my understanding that both the current release of >> Netscape and Internet Exploder can display PNG files. >> > >PNG Live(tm) is a plugin for Netscape Navigator and Microsoft Internet >Explorer that allows you to see PNG (Portable Network Graphics) images >directly in your web browser. The PNG image format represents the next >generation of image standards. Better compression, higher resolution, >and multiple layers of transparency are just some of its benefits. >Download a copy of PNG Live for use with Windows 95, Windows NT, and >Power Macintosh platforms at: > http://codelab.siegelgale.com/solutions/ > > >Various inline plug-ins for Netscape browsers, under the following >platform: > Macintosh 68K, PPC > Windows 3.x > Windows 95 > Windows NT > OS/2 > IRIX > Sun Solaris > HP-UX > OSF1 > AIX > Linux >may be found by going to the following: > >http://search.netscape.com/comprod/products/navigator/version_2.0/plugins/b y_platform.html > >- >------------------------------------------------------------ >Thanks for using Fractint, The Fractals and Fractint Discussion List >Post Message: fractint@xmission.com >Get Commands: majordomo@xmission.com "help" >Administrator: twegner@phoenix.net >Unsubscribe: majordomo@xmission.com "unsubscribe fractint" > > - - - ------------------------------------------------------------ Thanks for using Fractint, The Fractals and Fractint Discussion List Post Message: fractint@xmission.com Get Commands: majordomo@xmission.com "help" Administrator: twegner@phoenix.net Unsubscribe: majordomo@xmission.com "unsubscribe fractint" ------------------------------ Date: Mon, 19 Jan 1998 15:33:46 -0600 (CST) From: pjcarlsn@ix.netcom.com (Paul and/or Joyce Carlson) Subject: Re: (fractint) Re: fractint-digest V1 #81 Well, I tried responding to Kerry's message a couple of hours ago and it bounced back to me. I'll try responding to this one (which doesn't have "lists" in the email address and see what happens. >Paul Carlson wrote: >> Also, I had no TSR running when my colormaps got messed up. > >Hmmm. Might be your graphics card, then. Have you tried running fractint >with nothing in your AUTOEXEC.BAT or CONFIG.SYS files? I think I tried just about everything. I was using DOS 6.22 and booting directly into DOS (at the time I had Windows 3.1 on the machine). Now here's the message that I tried to send in response to Kerry's message about bubbles: After almost a month I can finally send email to this list again!!! Kerry wrote: >I didn't originate the bubble method, but that didn't stop me from writing >about it, and adding some of my own variations to the collective. [snip] >The Bubble Method > >The bubble method is an extension of Fractint's bof60 scheme. In >bof60, the interior of the fractal is colored by how closed the iterate >comes to the origin. In the bubble method, a specific value is set as >the threshold. [snip] As far as I know, I developed the "bubble" method about 2 1/2 years ago. I haven't translated the method into a Fractint formula because, as originally developed, the method involved two passes over the image. I haven't had a chance yet to try Kerry's formula, but I thought you might be interested in how I came to develop the method. This method, as well as a couple others, is described in my paper, "PSEUDO-3D RENDERING METHODS FOR FRACTALS IN THE COMPLEX PLANE" that was published in the journal _Computers & Graphics_, Vol. 20, No. 5, pp. 751-758, 1996. Here is a short excerpt from it: - -------------------------------------------------------------------------- BUBBLE METHOD The Bubble Method is so named because it produces images which consist of elements with a spherical appearance. The method was inspired by the illustration preceding Chapter 4 of Pickover[3] which shows contours of the minimum absolute value of z for points within the Mandelbrot set. Because the contours end at the edge of the Mandelbrot set, many of the contours in the illustration are incomplete. To see what the image would look like if all the contours were complete, a program was written in which the contours of the minumum absolute value of z were plotted for all points, whether or not they were within the Mandelbrot set. This had the desired effect of completing the contours but also filled the entire image with contours. The method described below was developed to eliminate unwanted contours in the final image. Unlike the other methods described above, the Bubble Method requires that the image be plotted in two passes, with the user interacting with the program after the first pass. Colormap: The colormap has one color range. Bailout Criteria: Bailout occurs when z exceeds a specified value. Color Computations: The minimum value of z in the orbit is saved as minz. The colormap index is computed from: pcolor = (F * minz) MOD numcolors. The best value for F will vary from image to image, but a good first guess is five times numcolors. The value of F should be such that most of the colors occur within the bubbles without any color being repeated within a bubble. After the first pass is complete the image will have no background color. The entire image will consist of concentric bands of color, many of which will need to be changed to the background color in the final image to achieve the desired effect. To allow this, the program pauses after the first pass and allows the user to select a pixel in the image using the mouse pointer. minz is computed for the selected pixel and the entire image is replotted, this time using the background color for any pixel with minz less than the selected pixel's minz. The resulting image may need to be edited with a palette editing program to make the colors within each bubble span the range from lightest to darkest. REFERENCES 3. C. A. Pickover, Computers, Pattern, Chaos and Beauty, St. Martin's Press, New York (1990). - -------------------------------------------------------------------- I'll try and see what I can do to implement this in a Fractint formula in the near future. Paul Carlson - - - ------------------------------------------------------------ Thanks for using Fractint, The Fractals and Fractint Discussion List Post Message: fractint@xmission.com Get Commands: majordomo@xmission.com "help" Administrator: twegner@phoenix.net Unsubscribe: majordomo@xmission.com "unsubscribe fractint" ------------------------------ Date: Tue, 20 Jan 1998 21:54:24 -0800 From: "Jay Hill" Subject: Re: (fractint) Lee's Truecolor Fractals Hi Kathy, Are you sure you used my copy of Lee's par file?? It has not the missing \ problems. Now you need to put the formula part in a .frm file, the rest in a par file. What I like to do as a quickie is stick frm: in front of the formula. frm:carr2821 ........ Then save the file as a par and let Fractint find the formula in the par file. I changed (sorry Lee) the copy on my site so it has the frm: in it. Just down load it with no =3D and so on. Just save as a .par and it should run. http://home.san.rr.com/jayrhill/skinner.par I just ran it again - no problem. Jay PS another image follows....... - ---------- > From: Gedeon Peteri > To: fractint@lists.xmission.com > Subject: Re: (fractint) Lee's Truecolor Fractals > Date: Tuesday, January 20, 1998 2:28 PM > > > > kathy roth wrote: > > > On all the images I have tried (5 or > > 6) it says "oops I couldn't understand the argument > > colors = 000EHO<7>....." (quotes one line of color parameter) > > Exactly the same problem I ran into with Lee's image, and others. I > corrected it by editing the par in Notepad. I found that the end of the > line cited did not have a backslash. Also, make sure there are no double > spaced lines. I sometimes get them too, especially with Lee's postings. > When editing them out, one must take great care that nothing else is > deleted. Perhaps this is your problem too. > Gedeon FGZ-J_823z1 { ; (c) Jay Hill, 1998 ; generalization of formula by Michael G. Wareman ; p1 is focus of Julia set reset=1960 type=formula formulafile=fgz.frm formulaname=fgz-julia passes=1 center-mag=0.645915/0/10/1/90 params=3/0/3/0/-0.823/0 float=y maxiter=25600 inside=0 colors=00000e<9>Lzz<18>wzzzzzzzz<220>KKK000000 } FGZ-Julia { ; (c) Jay Hill, 1998 ; generalization of formula by Michael G. Wareman ; p3 is focus of Julia set z=pixel, c=p3: z1=z*z + c; z = p1*z1*z1/(z1 + p2) + c; |z| <= 64 } - - - ------------------------------------------------------------ Thanks for using Fractint, The Fractals and Fractint Discussion List Post Message: fractint@xmission.com Get Commands: majordomo@xmission.com "help" Administrator: twegner@phoenix.net Unsubscribe: majordomo@xmission.com "unsubscribe fractint" ------------------------------ Date: Tue, 20 Jan 1998 22:54:30 -0700 (MST) From: Kerry Mitchell Subject: (fractint) Explanation, parameters, formula--field (long) comment { ; narrative copyright Kerry Mitchell Field In the Mandelbrot set, field lines are roughly perpendicular to the dwell bands (bands of constant escape iteration number). The lines are not directly related to the iteration level, nor to the decomposition rays, but are associated with the behavior of the orbits as the iterates approach infinity. Field lines of period "n" separate the period n disks from the main cardioid of the Mandelbrot set. The points that make up these lines have the characteristic that, as the magnitude of the orbit approaches infinity, the polar angle is fieldangle = 2 * pi * m / (2^n - 1), where n is the period of the line, and m = (1, 2, ... 2^n-1) is the order of the line. For example, there are 3 period 2 field lines, for m = 1, 2, and 3. (The m=3 case is simply the positive real axis, whose fieldangle is always 0.) For m=1, the fieldangle = 2/3 pi radians, or 120 degrees. Each successive iteration squares the previous iterate (neglecting adding c, since c is very small relative to the iterate), which doubles the fieldangle. Twice 120 degrees is 240 degrees, or 4/3 pi radians. Twice that is 8/3 pi radians, or 2/3 pi radians (since 6/3 pi radian or 2 pi is a full circle). So, the field line has the same angle again in 2 iterations, or is periodic with period n=2. The same thing happens with the m=2 line. Finding the field lines directly is not an easy task. What this coloring method does is to show approximations to the field lines, and show some cases that aren't field lines at all. It does this by computing the polar angle of the iterate at each step, and comparing it to the angle for the user-specified field line. By coloring according to the smallest error in angles (current vs. field line), lines are drawn that come close to the specified field line. (For the actual field line, the error would be zero.) However, many other lines have polar angles equal to that of the specified field line, so they show up as well. The result is not necessarily a mathematically accurate illustration of the Mandelbrot field lines, but it is another interesting way to render the set. } solar-flare { ; copyright Kerry Mitchell ; ; sample parameter file for field2_man ; reset=1960 type=formula formulafile=fractint.frm formulaname=field2_man passes=1 center-mag=-1.1/0/2.55/1/-90 params=1e+030/1 float=y maxiter=256 inside=0 decomp=256 periodicity=0 colors=000<35>x00z00z10<34>zx0zz0zz1<36>zzz<51>\ zz2zz0zy0<51>y20x00w00<30>200000000000000 cyclerange=0/255 } another-flare { ; copyright Kerry Mitchell ; ; sample parameter file for field2_jul ; reset=1960 type=formula formulafile=fractint.frm formulaname=field2_jul passes=1 center-mag=0.21045/0.224515/5.\ 540202/1/-12.5 params=-0.745315595965/0.078886716126/1e+030/2 float=y maxiter=256 inside=0 decomp=256 periodicity=0 colors=0\ 00<35>x00z00z10<34>zx0zz0zz1<36>zzz<51>zz2zz0zy0<51>y20x00w00<\ 30>200000000000000 cyclerange=0/255 } frm:field2_jul { ; Kerry Mitchell ; ; Colors Julia sets by nearest approach to ; period 2 field lines ; ; use decomp=256 ; p1 = Julia parameter ; real(p2) = bailout (try 1e12) ; imag(p2) = number of field line to use: 0, 1, or 2 ; 2 iterations per pixel ; variable zc used for calculation, z for coloring ; zc=pixel, c=p1, maxr=real(p2), minr=maxr, iter=1 fieldangle=tan(imag(p2)*2*pi/3): ; ; iteration ; compare tangent of polar angle with desired ; field line angle, update minimum if needed ; iter=iter+2, zc=sqr(zc)+c, zc=sqr(zc)+c rzc=|zc|, tanangle=imag(zc)/real(zc), r=cabs(fieldangle-tanangle) if (rmaxr)||(iter>=maxit)) iter=-1 angle=log(minr) z=cos(angle)+flip(sin(angle)) end if iter>0 } frm:field3_jul { ; Kerry Mitchell ; ; Colors Julia sets by nearest approach to ; period 3 field lines ; ; use decomp=256 ; p1 = Julia parameter ; real(p2) = bailout (try 1e12) ; imag(p2) = number of field line to use: ; 0, 1, 2, 3, 4, 5, 6, 7 ; 3 iterations per pixel ; variable zc used for calculation, z for coloring ; zc=pixel, c=p1, maxr=real(p2), minr=maxr, iter=1 fieldangle=tan(imag(p2)*2*pi/7): ; ; iteration ; compare tangent of polar angle with desired ; field line angle, update minimum if needed ; iter=iter+3, zc=sqr(zc)+c, zc=sqr(zc)+c, zc=sqr(zc)+c rzc=|zc|, tanangle=imag(zc)/real(zc), r=cabs(fieldangle-tanangle) if (rmaxr)||(iter>=maxit)) iter=-1 angle=log(minr) z=cos(angle)+flip(sin(angle)) end if iter>0 } frm:field4_jul { ; Kerry Mitchell ; ; Colors Julia sets by nearest approach to ; period 4 field lines ; ; use decomp=256 ; p1 = Julia parameter ; real(p2) = bailout (try 1e12) ; imag(p2) = number of field line to use: 0 - 15 ; 4 iterations per pixel ; variable zc used for calculation, z for coloring ; zc=pixel, c=p1, maxr=real(p2), minr=maxr, iter=1 fieldangle=tan(imag(p2)*2*pi/15): ; ; iteration ; compare tangent of polar angle with desired ; field line angle, update minimum if needed ; iter=iter+4, zc=sqr(zc)+c, zc=sqr(zc)+c, zc=sqr(zc)+c zc=sqr(zc)+c, rzc=|zc|, tanangle=imag(zc)/real(zc), r=cabs(fieldangle-tanangle) if (rmaxr)||(iter>=maxit)) iter=-1 angle=log(minr) z=cos(angle)+flip(sin(angle)) end if iter>0 } frm:field2_man { ; Kerry Mitchell ; ; Colors Mandelbrot set by nearest approach to ; period 2 field lines ; ; use decomp=256 ; real(p1) = bailout (try 1e12) ; imag(p1) = number of field line to use: 0, 1, or 2 ; 2 iterations per pixel ; variable zc used for calculation, z for coloring ; zc=0, c=pixel, maxr=real(p1), minr=maxr, iter=1 fieldangle=tan(imag(p1)*2*pi/3): ; ; iteration ; compare tangent of polar angle with desired ; field line angle, update minimum if needed ; iter=iter+2, zc=sqr(zc)+c, zc=sqr(zc)+c rzc=|zc|, tanangle=imag(zc)/real(zc), r=cabs(fieldangle-tanangle) if (rmaxr)||(iter>=maxit)) iter=-1 angle=log(minr) z=cos(angle)+flip(sin(angle)) end if iter>0 } frm:field3_man { ; Kerry Mitchell ; ; Colors Mandelbrot set by nearest approach to ; period 3 field lines ; ; use decomp=256 ; real(p1) = bailout (try 1e12) ; imag(p1) = number of field line to use: ; 0, 1, 2, 3, 4, 5, 6, 7 ; 3 iterations per pixel ; variable zc used for calculation, z for coloring ; zc=0, c=pixel, maxr=real(p1), minr=maxr, iter=1 fieldangle=tan(imag(p1)*2*pi/7): ; ; iteration ; compare tangent of polar angle with desired ; field line angle, update minimum if needed ; iter=iter+3, zc=sqr(zc)+c, zc=sqr(zc)+c, zc=sqr(zc)+c rzc=|zc|, tanangle=imag(zc)/real(zc), r=cabs(fieldangle-tanangle) if (rmaxr)||(iter>=maxit)) iter=-1 angle=log(minr) z=cos(angle)+flip(sin(angle)) end if iter>0 } frm:field4_man { ; Kerry Mitchell ; ; Colors Mandelbrot set by nearest approach to ; period 4 field lines ; ; use decomp=256 ; real(p1) = bailout (try 1e12) ; imag(p1) = number of field line to use: 0 - 15 ; 4 iterations per pixel ; variable zc used for calculation, z for coloring ; zc=0, c=pixel, maxr=real(p1), minr=maxr, iter=1 fieldangle=tan(imag(p1)*2*pi/15): ; ; iteration ; compare tangent of polar angle with desired ; field line angle, update minimum if needed ; iter=iter+4, zc=sqr(zc)+c, zc=sqr(zc)+c, zc=sqr(zc)+c zc=sqr(zc)+c, rzc=|zc|, tanangle=imag(zc)/real(zc), r=cabs(fieldangle-tanangle) if (rmaxr)||(iter>=maxit)) iter=-1 angle=log(minr) z=cos(angle)+flip(sin(angle)) end if iter>0 } - ------------------------------------------------------------------------------- Kerry Mitchell lkmitch@primenet.com - ------------------------------------------------------------------------------- - - - ------------------------------------------------------------ Thanks for using Fractint, The Fractals and Fractint Discussion List Post Message: fractint@xmission.com Get Commands: majordomo@xmission.com "help" Administrator: twegner@phoenix.net Unsubscribe: majordomo@xmission.com "unsubscribe fractint" ------------------------------ Date: Tue, 20 Jan 1998 22:55:50 -0700 (MST) From: Kerry Mitchell Subject: (fractint) Explanation, parameters, formulas--gaussian integers (long) comment { ; narrative copyright Kerry Mitchell Gauss In the Fractint method bof60, the question of interest is how close the orbit comes to the origin (0+0i). The origin is one of an infinity of "Gaussian integers." These are complex numbers such that both the real and imaginary parts are integers. Examples are: (0,0), (-2,3), (17,-5), and (1000000,123456789). The gaussian scheme is concerned with how close the orbit comes to a Gaussian integer. To find the gaussian integer which the orbit most closely approaches, the built-in function round() is used. Round(zc) returns a complex number whose components are the rounded components of zc. This is a Gaussian integer. The distance from zc to round(zc) is simply the magnitude of zc - round(zc). The gaussian method tracks this distance and records the value of zc for which the distance is the smallest. This value of zc is zmin. In the gaussintt methods (Julia and Mandelbrot variations), simply plots the polar angle of zmin, by assigning zmin to z and using the decomp coloring. Since zmin can occur at any point in the orbit, there's no clear connection between the pixel value and the resulting color. However, nearby points can often have similar orbits, so the spots of constant color (polar angle) can have a variety of sizes. Similar results are obtained with the gaussintr methods. Here, the log of the magnitude of zmin is used as the polar angle for decomposition. For particular combinations of parameter c and initial zc, the orbit may be all Gaussian integers, for example, starting with zc=1 and c = (0,1). For other combinations of zc and c, such as zc=0 and c=pi, the orbit will never be an integer. Thus, it is reasonable to assume that some orbits will tend to be closer to integers than others. This is illustrated with the gaussinttot methods. A running sum of the distances, r, is kept for all iterations in the orbit. The mean distance is then determined, and this is scaled into the decomposition angle. The result is a grid-like pattern superimposed on the basic fractal structure. } mushroom-cloud { ; copyright Kerry Mitchell ; ; sample parameter file for gaussintt_jul ; reset=1960 type=formula formulafile=fractint.frm periodicity=0 formulaname=gaussintt_jul passes=1 center-mag=0/0.75/1.333333 params=0.3/0/1e12/0 float=y maxiter=256 inside=0 decomp=256 colors=000<20>z00<19>\ zv0zy0zz1<20>zzz<20>0zz<20>00z<19>004001100<20>z00<20>\ zz0<19>zzwzzzxzz<18>4zz1zz0yz<20>00z<20>000 cyclerange=0/255 } nautilus { ; copyright Kerry Mitchell ; ; sample parameter file for gaussinttot_jul ; reset=1960 type=formula formulafile=fractint.frm cyclerange=0/255 formulaname=gaussinttot_jul passes=1 periodicity=0 center-mag=-0.524765/0.169456/40 params=0.28/0.005/1e12/100 float=y maxiter=1000 inside=0 decomp=256 colors=GTg<18>AJXA\ JWAIVAIU9HU<33>001000001<31>9GS9HT9HUAIUAIVAJW<25>IVjJWkJWk\ KXlKXl<18>RftSftSgtTgtThu<3>VjvVjvWkvXkw<14>dsyesyftygtyhuz\ <3>kwzlwznxzoxz<2>tzzzzztzzryz<4>kwzjvzivzhuzhuzgty<8>`px`o\ x_ox_nxZnx<5>WkvVjvVjvViv<12>PcrObqObqOapNap<17>HTh } splatter-paint { ; copyright Kerry Mitchell ; ; sample parameter file for gaussintr_man ; reset=1960 type=formula formulafile=fractint.frm cyclerange=0/255 formulaname=gaussintr_man passes=1 center-mag=-0.8113020344287\ 9510/+0.20153444676409190/108.7713 params=4/0 float=y maxiter=1000 inside=0 decomp=256 periodicity=0 colors=000<3>zo0<3>zzz<3>PPz<3>\ 000<3>zo0<3>zzz<3>PPzJJjDDV66F110HE0XR0lc0zo1zrHztXzwlyyz<2>YYzPP\ yIIiCCU66E220<2>md0zo2<2>zwmyyzoozffzXXzOOx<2>66D330<2>ne0zo3zrJz\ uZzwnxxz<2>XXzOOw<2>55C440<2>of0zo4zrKzu_zxoxxznnzeezWWzOOv<2>55B\ 540<2>pf0zp5<2>zxpwwzmmzddzVVzNNu<2>44A650<2>qg0zp6<2>zxqvvzmmzcc\ zVVzNNt<2>449760<2>rh0zp7<2>zxrvvzllzcczUUzMMs<2>448870<2>si0zp8<\ 2>zxsuuzllzbbzUUzMMr<2>337980<2>tj0zp9<2>zxtuuz<2>TTzMMq<2>336A80\ <2>uj0zpA<2>zyuttz<2>SSzLLp<2>225B90<2>vk0zqB<2>zyvsszjjz``zSSzLL\ o<2>224CA0<2>wl0zqC<2>zywssz<2>RRzKKn<2>223DB0<2>xm0zqD<2>zyxrrzi\ iz__zRRzKKm<2>112EC0<2>yn0zqE<2>zyyrrz<2>QQzKKl<2>111 } frm:gaussintr_jul { ; Kerry Mitchell ; ; Gaussian integer coloring of Julia sets ; color by magnitude of nearest gaussian integer ; inside and outside handled the same way ; ; use decomp=256 ; p1 = Julia parameter ; real(p2) = bailout (try 1e12) ; variable zc used for calculation; coloring done with z ; zc=pixel, c=p1, iter=1, rmax=real(p2), rmin=1: ; ; iteration ; zr = gaussian integer ; r = distance to zr ; zmin = integer with minimum distance ; iter=iter+1, zc=sqr(zc)+c, zr=round(zc), r=|zc-zr|, if (rrmax)||(iter==maxit)) iter=-1 angle=log(cabs(zmin)+1) z=cos(angle)+flip(sin(angle)) end if iter>0 } frm:gaussintt_jul { ; Kerry Mitchell ; ; Gaussian integer coloring of Mandelbrot set ; color by polar angle of nearest gaussian integer ; inside and outside handled the same way ; ; use decomp=256 ; p1 = Julia parameter ; real(p2) = bailout (try 1e12) ; variable zc used for calculation; coloring done with z ; zc=pixel, c=p1, rmax=real(p2), rmin=1, iter=1: ; ; iteration ; zr = gaussian integer ; r = distance to zr ; zmin = integer with minimum distance ; iter=iter+1, zc=sqr(zc)+c, zr=round(zc), q=|zc-zr|, if (qrmax)||(iter==maxit)) iter=-1 z=zmin end if iter>0 } frm:gaussinttot_jul { ; Kerry Mitchell ; ; Gaussian integer coloring of Julia sets ; color by average distance to nearest integer ; inside and outside handled the same way ; ; use decomp=256 ; p1 = Julia parameter ; real(p2) = bailout (try 1e12) ; imag(p2) = scaling factor (try 30) ; variable zc used for calculation; coloring done with z ; zc=pixel, c=p1, rmax=real(p2), scale=imag(p2) iter=1, rmin=1, z=zc, tot=0: ; ; iteration ; zr = gaussian integer ; r = distance to zr ; zmin = integer with minimum distance ; tot = running sum of r's ; iter=iter+1, zc=sqr(zc)+c, rzc=|zc| zr=round(zc), r=|zc-zr|, tot=tot+r ; ; bailout ; scale average distance to decomp angle ; set "iteration done" flag (iter=-1) ; if ((rzc>rmax)||(iter==maxit)) angle=scale*tot/(iter-1) z=cos(angle)+flip(sin(angle)) iter=-1 end if iter>0 } frm:gaussintr_man { ; Kerry Mitchell ; ; Gaussian integer coloring of Mandelbrot set ; color by magnitude of nearest gaussian integer ; inside and outside handled the same way ; ; use decomp=256 ; real(p1) = bailout (try 1e12) ; variable zc used for calculation; coloring done with z ; zc=0, c=pixel, iter=1, rmax=real(p1), rmin=1: ; ; iteration ; zr = gaussian integer ; r = distance to zr ; zmin = integer with minimum distance ; iter=iter+1, zc=sqr(zc)+c, zr=round(zc), r=|zc-zr|, if (rrmax)||(iter==maxit)) iter=-1 angle=log(cabs(zmin)+1) z=cos(angle)+flip(sin(angle)) end if iter>0 } frm:gaussintt_man { ; Kerry Mitchell ; ; Gaussian integer coloring of Mandelbrot set ; color by polar angle of nearest gaussian integer ; inside and outside handled the same way ; ; use decomp=256 ; real(p1) = bailout (try 1e12) ; variable zc used for calculation; coloring done with z ; zc=0, c=pixel, rmax=real(p1), rmin=1, iter=1: ; ; iteration ; zr = gaussian integer ; r = distance to zr ; zmin = integer with minimum distance ; iter=iter+1, zc=sqr(zc)+c, zr=round(zc), q=|zc-zr|, if (qrmax)||(iter==maxit)) iter=-1 z=zmin end if iter>0 } frm:gaussinttot_man { ; Kerry Mitchell ; ; Gaussian integer coloring of Mandelbrot set ; color by average distance to nearest integer ; inside and outside handled the same way ; ; use decomp=256 ; real(p1) = bailout (try 1e12) ; imag(p1) = scaling factor (try 30) ; variable zc used for calculation; coloring done with z ; zc=0, c=pixel, rmax=real(p1), scale=imag(p1) iter=1, rmin=1, z=zc, tot=0: ; ; iteration ; zr = gaussian integer ; r = distance to zr ; zmin = integer with minimum distance ; tot = running sum of r's ; iter=iter+1, zc=sqr(zc)+c, rzc=|zc| zr=round(zc), r=|zc-zr|, tot=tot+r ; ; bailout ; scale average distance to decomp angle ; set "iteration done" flag (iter=-1) ; if ((rzc>rmax)||(iter==maxit)) angle=scale*tot/(iter-1) z=cos(angle)+flip(sin(angle)) iter=-1 end if iter>0 } - ------------------------------------------------------------------------------- Kerry Mitchell lkmitch@primenet.com - ------------------------------------------------------------------------------- - - - ------------------------------------------------------------ Thanks for using Fractint, The Fractals and Fractint Discussion List Post Message: fractint@xmission.com Get Commands: majordomo@xmission.com "help" Administrator: twegner@phoenix.net Unsubscribe: majordomo@xmission.com "unsubscribe fractint" ------------------------------ Date: Tue, 20 Jan 1998 22:22:38 -0800 From: "Jay Hill" Subject: (fractint) F.O.T.N. (Fractal of the Night) 20 Jan 1998 (Big Fatso) F.O.T.N. (Fractal of the Night) 20 Jan 1998 (Big Fatso) And now presenting another fractal distortion by Dr. J,=20 the mad scientist. Tonight, he has tried to eat one too=20 many fractal dark chocolates and then looked in the=20 mirror! =A0It is called Fractal of the Night (Big Fatso). =A0 Has Dr. J enjoyed too many games of fractal ball?=20 Tonight's fractal, in honor of the up-coming end of the=20 football season, takes a look at Dr. J after a few too=20 many weekends sitting in front of his fractal tube=20 watching fractal plays in his favorite game, fractal ball.=20 It is the MSet, only slightly distorted by the ingestion=20 of log sized chunks of chocolate, among other things.=20 Perhaps too many of last nights fractal potatoes? =20 The formula is the usual Mandelbrot set iteration=20 z =3D z^2 + c=20 with a transformation thrown in.=20 http://home.san.rr.com/jayrhill/FotN/FotN20.html Here are the Fractint parameter files.=20 Enjoy=20 Jay - ------------------------------------------------- frm:fatlog { ; by Jay Hill, 1998 c=3Dlog(pixel),z=3D0: z=3Dsqr(z)+c |z|<=3D100 }=20 bigfatso { ; Big Fatso (c) by Jay Hill, 1998 ; After collecting for himself all the chocolate ; in fractal land, only then did Dr. J look in the ; mirror! Good grief! reset=3D1960 type=3Dformula formulafile=3Dn.frm formulaname=3Dfatlog center-mag=3D0.862138/-0.0753769/1.009179/1/-90 float=3Dy maxiter=3D256 inside=3D0 decomp=3D256 colors=3Dz_G<2>UA0<153>YJ6YJ6ZK5<49>cK0cK0bK0<38>TB0<4>kP9 savename=3Dbigfatso }=20 - - - ------------------------------------------------------------ Thanks for using Fractint, The Fractals and Fractint Discussion List Post Message: fractint@xmission.com Get Commands: majordomo@xmission.com "help" Administrator: twegner@phoenix.net Unsubscribe: majordomo@xmission.com "unsubscribe fractint" ------------------------------ Date: Wed, 21 Jan 1998 02:50:14 -0600 From: "Paul N. Lee" Subject: Re: (fractint) Lee's Truecolor PNG site Tim Wegner wrote: > > Paul wrote: > > > > PNG Live(tm) is a plugin for Netscape Navigator and > > Microsoft Internet Explorer that allows you to see > > PNG (Portable Network Graphics) images directly in > > your web browser. > > True, but the latest beta versions of both Netscape and > Internet Explorer support PNG instrinsically. For example, > I am using Netscape 4.04, which I can verify does support PNG. > Also true, but until everyone that uses the two "big boys" decides to upgrade to the most current versions, they can use the plugin and view PNG files online. Support for PNG is there in the latest levels (which I have and use), but I still prefer to use my Navigator 3.04 Gold. Just thought I would pass on a helpful hint for individuals not using the "bleeding edge" software. - - - ------------------------------------------------------------ Thanks for using Fractint, The Fractals and Fractint Discussion List Post Message: fractint@xmission.com Get Commands: majordomo@xmission.com "help" Administrator: twegner@phoenix.net Unsubscribe: majordomo@xmission.com "unsubscribe fractint" ------------------------------ End of fractint-digest V1 #85 *****************************