Title: | Mathematics at DEC |
Moderator: | RUSURE::EDP |
Created: | Mon Feb 03 1986 |
Last Modified: | Fri Jun 06 1997 |
Last Successful Update: | Fri Jun 06 1997 |
Number of topics: | 2083 |
Total number of notes: | 14613 |
.... .. .. .. .. .. .. . .. . .. . .. . .. . ... . ... . ... ---------------------------------------- Does this curve look familiar to anybody? Sort of a normal curve, but squashed left? I'm looking for a statistical distribution and "know" I've seen this before, but none of my college texts show this curve. (Of course, they -all- show the normal curve, then list all the others). If you can identify the curve, can you supply the generating equation? John
T.R | Title | User | Personal Name | Date | Lines |
---|---|---|---|---|---|
1677.1 | seems like a black body | BRSTR2::SYSMAN | Dirk Van de moortel | Wed Oct 21 1992 12:44 | 16 |
Seems like the radiation spectrum of a black body. I'll look up the generating equation and let you know tomorrow... Intensity ^ .... | .. .. | .. .. | .. .. | . .. | . .. | . .. |. .. |. ... . ... . ... +------------------------------------------------> frequency | |||||
1677.2 | or look at gamma densities | SGOUTL::BELDIN_R | D-Day: 161 days and counting | Wed Oct 21 1992 13:34 | 18 |
If you look at log-normal histograms, they will look like that, positive, unimodal, and tailing off to infinity. If X is log normal, then log X is normal. Let Y = log X. Assume Y is Normal(�,�). 2 2 f(y)dy = k exp(-(y-�) /2� )dy. 2 2 f(log x)dlog x = k' exp(-(log x-�) /2� )(1/x)dx where k and k' are defined so the integrals = 1. Is that what you're after? You can find all kinds of curves that give that shape, of course, but this is a common one in statistics. Dick | |||||
1677.3 | HERON::BUCHANAN | The was not found. | Wed Oct 21 1992 14:07 | 6 | |
Hey neat: � How d'you get that character? I don't spose there are any other Greek characters that we can get? (apart from �) Andrew. | |||||
1677.4 | kilroy was here and murphy too! | SGOUTL::BELDIN_R | D-Day: 161 days and counting | Wed Oct 21 1992 14:23 | 8 |
� is compose / u. and � is compose o /. and � is compose << There are more, but I can only find them by hacking and never when I want them. I don't where you can get documentation. I have seen alpha and sigma too, but I've broken my fingers trying to guess how. �j� | |||||
1677.5 | 3D::ROTH | Geometry is the real life! | Wed Oct 21 1992 14:41 | 4 | |
It may be a Rayleigh distribution, essentially a chi squared distribution of 2 degrees of freedom. - Jim | |||||
1677.6 | RUSURE::EDP | Always mount a scratch monkey. | Wed Oct 21 1992 15:22 | 94 | |
Here's a list of the compose sequences. -- edp � A" � a" � A' � a' � A^ � a^ � A' � a' � AE � ae � A~ � a~ � A* � a* � a_ @ aa � C, � c, � c/ � c0 � E" � e" � E' � e' � E^ � e^ � E` � e` � I" � i" � I' � i' � I^ � i^ � I` � i` � L- � N~ � n~ � O" � o" � O' � o' � O^ � o^ � O` � o` � OE � oe � O~ � o~ � O/ � o/ � OX � o_ � P! � SO � ss � U" � u" � U' � u' � U^ � u^ � U` � u` � Y" � y" � Y- � ^0 � ^1 � ^2 � ^3 � 12 � 14 [ (( { (- ] )) } )- � << � >> � ?? � !! � ^. | ^/ # ++ � +- \ // � /u | |||||
1677.7 | >2 df. | CADSYS::COOPER | Topher Cooper | Wed Oct 21 1992 15:58 | 18 |
RE: .5 (Jim) Chi� looks like that -- but only for 3 or more degrees of freedom. chi�[n](x) = x^((n-2)/2)*exp(-x/2)/(2^(n/2)*GAMMA(n/2)); The gamma distribution, for some choices of the parameters, will also work: gamma[a, b](x) = x^a*exp(-x/b)/(GAMMA(a+1)*b^(a+1)) which is hardly surprising since gamma[(n-2)/2, 2] = chi�[n]. So basically you get an extra parameter to play with in fitting, and there isn't even a hint that 'a' must be an integer. My best guess is that you are remembering the log-normal, though. Topher | |||||
1677.8 | STAR::ABBASI | I love DECspell | Wed Oct 21 1992 16:38 | 8 | |
ref .6 Thanks EDP for that list, do you know if one can write vectors too? - like A , but the dash is close to the A ? /nasser | |||||
1677.9 | a little bit closer :-) | CSC32::D_DERAMO | Dan D'Eramo, Customer Support Center | Wed Oct 21 1992 22:14 | 10 |
re .-1, > - > like A , but the dash is close to the A ? _ How about this: A Dan 0:-) | |||||
1677.10 | not BB but x*exp(-x) | BRSTR2::SYSMAN | Dirk Van de moortel | Thu Oct 22 1992 05:42 | 80 |
re. 1 3 x It's not a black body spectrum: BB(x) = -------- x e -1 which must have an horizontal tangent in (0,0), while yours clearly has a vertical tangent... -x The simplest function I can think of with these properties is: x e Here's a plot (made with good old datatrieve!) of that function: If you have a graphics terminal (VT240,VT330,...) say EXTRACT TT: <[2JP1p s[0,0](EA[0,0][767,479] S1I(D))p[0,0] @:B@; T(A0S1)t(s1I0)w(vi(w)s0P1) L(A2) L"5"00FF8181818181FF L"6"0018244281422418 L"0"00FF814242242418 T(B) T(E) P[100,360]V[+600][,-350][100][,360] P[0,185]T(B)[0,25]"" T[15,0]P[133,460]T"x*exp(-x) -- Control_W to resume..."T(E) P[81,355]T"0" P[101,273]V(W(P4I(0)))[+598] P[45,268]T" .100" P[101,185]V(W(P4I(0)))[+598] P[45,180]T" .200" P[101,98]V(W(P4I(0)))[+598] P[45,93]T" .300" P[45,5]T" .400" P[96,375]T"0" P[200,359]V(W(P4I(0)))[,-348] P[196,375]T"1" P[300,359]V(W(P4I(0)))[,-348] P[296,375]T"2" P[400,359]V(W(P4I(0)))[,-348] P[396,375]T"3" P[500,359]V(W(P4I(0)))[,-348] P[496,375]T"4" P[600,359]V(W(P4I(0)))[,-348] P[596,375]T"5" P[696,375]T"6" T(BA2S[8,16]) P[105,318]W(I1) V[105,318]V[110,281]V[115,247]V[120,217]V[125,190]V[130,166]V[135,144]V[140,125] V[145,109]V[150,95]V[155,82]V[160,72]V[165,63]V[170,56]V[175,50]V[180,45] V[185,42]V[190,40]V[195,39]V[200,38]V[205,38]V[210,40]V[215,41]V[220,44] V[225,47]V[230,50]V[235,54]V[240,58]V[245,62]V[250,67]V[255,72]V[260,77] V[265,83]V[270,88]V[275,94]V[280,100]V[285,105]V[290,111]V[295,117]V[300,123] V[305,129]V[310,135]V[315,141]V[320,147]V[325,152]V[330,158]V[335,164]V[340,169] V[345,175]V[350,180]V[355,186]V[360,191]V[365,196]V[370,201]V[375,206]V[380,211] V[385,216]V[390,220]V[395,225]V[400,229]V[405,234]V[410,238]V[415,242]V[420,246] V[425,250]V[430,253]V[435,257]V[440,261]V[445,264]V[450,268]V[455,271]V[460,274] V[465,277]V[470,280]V[475,283]V[480,286]V[485,288]V[490,291]V[495,293]V[500,296] V[505,298]V[510,301]V[515,303]V[520,305]V[525,307]V[530,309]V[535,311]V[540,313] V[545,315]V[550,316]V[555,318]V[560,320]V[565,321]V[570,323]V[575,324]V[580,325] V[585,327]V[590,328]V[595,329]V[600,331]V[605,332]V[610,333]V[615,334]V[620,335] V[625,336]V[630,337]V[635,338]V[640,339]V[645,340]V[650,340]V[655,341]V[660,342] V[665,343]V[670,343]V[675,344]V[680,345]V[685,345]V[690,346]V[695,346]V[700,347] W(R) p[101,308]t"6" p[696,337]t"6" T(E) @:B W(I0S1)P[,-30]V[+56]W(I3S0) V[,+30][-56][,-30][+56]P(B) P(E)[-52,+20] P(B)[,+0] [,-16]W(I1)T(A2S[8,20]) "6"P[+4] W(I3)T(A0)[12,0]"Y1"P(E) @; P[102,40]@B W(I(W))P[,500]\[1;24r[24;0f [20;0f | |||||
1677.11 | AYOV11::IGILLESPIE | Thu Oct 22 1992 05:48 | 15 | ||
Looks like a Poisson distribution. -m x e m P(x)= ---------- x! Where m = average number of occurancies e = e ... (2.71828...) Iain |