3λt^2 + 2κt + 1 = 0

are numerically greater than 3 for all pairs of values of (λ, κ) lying

above the line

27λ - 6κ + 1 = 0

As statistically promising within the discriminant of the cubic we then

have the shaded area of the (λ, κ) plane.

=The Origin.= The generating curve is the symmetrical normal

probability curve with origin at its center. Since x = 0 when t = 0,

the origin of the translated curve coincides with that of the base or

generating curve. The translated curve may not be symmetrical so that

the mean ordinate may not coincide with the modal ordinate. Because of

the relation between corresponding areas the ordinate at the origin

must continue to divide the area under the curve into equal parts, that

is, the origin and median always coincide.

=Determination of the Constants.= Since the exact position of

the median can not ordinarily be determined by inspection or direct

computation there are in reality four constants to be determined: the

distance between the median and the mean, a, κ and λ.

In determining the constants it is usual to compute the value of the

first four moments. The third and fourth moments are extensions of

the idea of the well known formulas for the first and second moments.

Denoting the moments about the median by μ, we have

1 ⌠+∞

μ_{1}^´ = ——— │ xy dx

N ⌡-∞

1 ⌠+∞

μ_{2}^´ = ——— │ x^{2}y dx

N ⌡-∞

1 ⌠+∞

μ_{3}^´ = ——— │ x^{3}y dx

N ⌡-∞

1 ⌠+∞

μ_{4}^´ = ——— │ x^{4}y dx

N ⌡-∞

where N is the total area under the curve.

The values of the μ’s are computed from the data[8] and equated to the

corresponding integrals which of course involve the four constants.

In this way four equations are obtained from which the values of the

constants may be determined. Since it is our present object to discuss

the solution only of these equations, merely the principal results will

be given.

The general form for the moments about the median of the

area under the translated curve is

1 ⌠+∞

μ_{n}^´ = ——— │ x^{n}y dx

N ⌡-∞

1 ⌠+∞ a^n(t + κt^2 + λt^3)^n

= —————— │ ———————————————————————— e^{-t^2/2} a(1 + 2κt + 3λt^2) dt

√(2π)N ⌡-∞ a(1 + 2κt + 3λt^2)

1 ⌠+∞

= —————— │ a^n(t + κt^2 + λt^3)^ne^{-t^2/2} dt.

√(2π)N ⌡-∞

On applying the two well known formulas:

⌠+∞

│ x^{2n + 1}e^{-x^2} dx = 0

⌡-∞

⌠+∞ 2n + 1 ⌠+∞

│ x^{2n + 2}e^{-x^2} dx = —————— │ x^{2n}e^{-x^2} dx,

⌡-∞ 2 ⌡-∞

the determination of μ_1´, μ_2´, μ_3´ and μ_4´ is reduced to a matter

of algebraic detail. Then on transferring to the arithmetic mean as

origin the values of μ_2, μ_3, and μ_4 can be determined in terms

of a, κ and λ. It is most convenient however, to make use of the

quantities β_1 = μ_3^2/μ_2^3 and β_2 = μ_4/μ_2^2 or rather β = β_1/8

and ϵ = (β_2 - 3)/12 and express the constants in terms of these

quantities. It is to be noted that both ϵ and β are zero for a normal

distribution, that is, for λ = κ = 0.

Omitting the detailed reduction[9] which is straightforward and direct,

we have

(1) μ´ = aκ

(2) μ_2 = a^2(1 + 6x + 15x^2 + 2κ^2)

2κ^2(2κ^2 + Q)^2

(3) β = ——————————————————————

(2κ^2 + R)^3

4κ^4 + 4κ^2S + T

(4) ϵ = ——————————————————————

(2κ^2 + R)^2

where the symbols, S, R, Q and T are defined as follows:

S = 1 + 18λ + 90λ^2,

R = 1 + 6λ + 15λ^2,

Q = 1.5 + 18λ + 135/2λ^2,

T = 2λ + 36λ^2 + 270λ^3 + 810λ^4.

Obviously no algebraic solution can be obtained from equations (3) and

(4) for κ and λ in terms of the computed values β and ϵ, and hence a

resort to tables is necessary. The values of β and ϵ for values of κ

from 0 to 0.0335 and of λ from -0.040 to +0.100 have been computed.[10]

The process of determining the constants of the translated normal curve

consists first in computing β and ϵ from the given data, and then in

entering the table and interpolating for the corresponding values of

κ and λ.[11] On substituting these values in (2) the value of a can be

found and thence on multiplying a by κ the position of the median of

the distribution is obtained.

The sign of κ is determined by the sign of the third moment about the

mean μ_3, that is, by the direction of the skewness or asymmetry. For

positive skewness the mean must lie to the right of the median and

hence μ_1´, the first moment about the mean, must be positive which

necessitates a positive sign for κ. Therefore, the sign of κ is the

same as that of the skewness.

To fit a curve to the given data, after the constants have been

determined it is necessary to find, by solving a cubic equation for

each value, the values of t corresponding to the x’s of the respective

classes. The cubic is

aλt^3 + aκt^2 + at - x = 0.

Any of the various methods of approximating to the solution of a cubic

may be used in solving these equations.

The area of each class can now be obtained by computing the

corresponding areas under the standard normal curve from a table of the

probability integral.

=The Method of Interpolation.= The actual fitting of the curve can

now be readily accomplished.[12] The distinctively geometrical operation

is the interpolation for the values of λ and κ for a given pair of

values of β and ϵ.

Within the limits of the table[13] the curves resulting from the

assignment of a constant value to β are practically straight lines,

β = 0 is the λ-axis; β = 1 is a line parallel to the λ-axis.

Hence we may safely assume that the variation from one column

to the next and from one line to the next is linear for

values of β. That is, ordinary first difference interpolation

methods are applicable.

As regards the system of ϵ curves we have for instance ϵ = .128 at (λ

= .050, κ = 0); again, at approximately (.045, .060) and (.40, .085).

We are therefore warranted in assuming the applicability of first

difference methods to interpolation between the ϵ curves.

As an illustration let us find the values of λ and κ for ϵ = 0.112 and

β = 0.044. On inspection of the table it is seen that λ lies between

0.30 and .035 and κ between .090 and .095. When κ = .090, λ = .033 for

ϵ = .112. When κ = .095, λ = .031 for ϵ = .112. For β = .042 and

κ = .090, λ = .033 and for β = .046 and κ = .095, λ = .031, ϵ = .112 in

each case. Hence, to first differences, λ = .032 and κ = .093 for

ϵ = .112 and β = .044. For interpolation in parts of the table showing

more rapid variations appropriate methods will suggest themselves.

Taken geometrically the table represents two distinct systems of

curves, with each curve of one system intersecting all the curves of

the other system. Therefore, a pair of values for λ and κ can always be

found for values of ϵ and β within the range of the table.

Department of Mathematics, Ohio State University.

TABLE OF ϵ AND β.

(ϵ is the first and β the second number of each pair.)

λ

───┬────────────────────────────────────────────

κ │-040 -035 -030 -025 -020 -015 -010 -005 000

───┴────────────────────────────────────────────

000 -061 -056 -050 -043 -035 -027 -019 -010 000

000 000 000 000 000 000 000 000 000

005 -055 -049 -042 -035 -027 -019 -010 000

000 000 000 000 000 000 000 000

010 -055 -049 -042 -035 -027 -018 -010 000

000 000 000 000 000 000 000 001

015 -049 -042 -035 -027 -018 -009 001

001 001 001 001 001 001 001

020 -048 -041 -034 -026 -017 -008 002

001 002 002 002 002 002 002

025 -047 -040 -033 -025 -016 -007 003

002 002 002 003 003 003 003

030 -046 -039 -032 -024 -015 -006 004

003 003 004 004 004 004 004

035 -045 -038 -031 -023 -014 -005 005

004 005 005 005 005 005 006

040 -037 -030 -022 -013 -004 006

006 006 007 007 007 007

045 -036 -028 -020 -011 -002 008

008 008 008 009 009 009

050 -034 -026 -018 -009 -000 010

009 010 010 011 011 011

055 -032 -024 -016 -007 002 012

011 012 012 013 013 013

060 -022 -014 -005 004 014

014 015 015 016 016

065 -020 -012 -003 006 017

016 017 018 018 019

070 -018 -009 000 009 019

019 020 020 021 022

075 -015 -007 002 012 022

022 023 023 024 025

080 -013 -004 005 015 025

025 026 026 027 028

085 -001 008 018 028

029 030 031 032

090 002 011 021 032

032 033 034 036

095 005 015 025 035

036 037 038 039

100 009 018 028 039

039 041 042 044

(ϵ is the first and β the second number of each pair.)

λ

───┬────────────────────────────────────────

κ │ 005 010 015 020 025 030 035 040 045 050

───┴────────────────────────────────────────

000 010 021 033 045 057 071 084 098 113 128

000 000 000 000 000 000 000 000 000 000

005 010 021 033 045 057 071 084 098 113 128

000 000 000 000 000 000 000 000 000 000

010 011 022 033 045 058 071 085 099 113 128

001 001 001 001 001 001 001 001 001 001

015 011 022 034 046 058 071 085 099 114 129

001 001 001 001 001 001 001 001 001 001

020 012 023 034 046 059 072 086 100 115 130

002 002 002 002 002 002 002 002 002 002

025 013 024 035 047 060 073 087 101 116 131

003 003 003 003 003 003 003 003 003 003

030 014 025 036 049 061 074 088 102 117 132

004 004 004 005 005 005 005 005 005 005

035 015 026 038 050 063 076 089 104 118 133

006 006 006 006 006 006 007 007 007 007

040 017 028 039 052 064 077 091 105 120 135

007 008 008 008 008 008 008 009 009 009

045 019 030 041 053 066 079 093 107 122 137

009 010 010 010 010 011 011 011 011 011

050 021 032 043 055 068 081 095 109 124 139

012 012 012 012 013 013 013 013 014 014

055 023 034 045 057 070 083 097 111 126 141

014 014 015 015 015 016 016 016 016 017

060 025 036 048 060 073 086 100 114 129 144

017 017 017 018 018 019 019 019 019 020

065 028 039 050 062 075 089 102 116 131 146

019 020 020 021 021 022 022 022 023 023

070 030 041 053 065 078 091 105 119 134 149

022 023 024 024 025 026 026 026 026 027

075 033 044 056 068 081 094 108 122 137 152

026 026 027 028 028 029 029 030 030 031

080 036 047 059 071 084 097 111 125 140 155

029 030 031 031 032 033 033 034 034 035

085 039 050 062 075 088 101 115 129 144 159

033 034 034 035 036 037 037 038 039 039

090 043 054 066 079 092 105 119 133 148 163

037 038 039 039 040 041 042 042 043 044

095 046 058 070 083 096 109 123 137 152 167

041 042 043 044 045 046 046 047 048 049

100 050 062 074 087 100 113 127 141 156 171

045 046 047 048 049 050 051 052 053 054

[6] Pearson, Karl:—“Skew Variation in Homogeneous Material;” Phil.

Trans. 1895, Vol. CLXXXVI, A, pp. 253 et seq.

“On the Systematic Fitting of Curves to Observations and Measurements,”

Biometrika, I, pp. 265 et seq. and Biometrika II, pp. 1 et seq.

Elderton:—“Frequency Curves and Correlation,” pp. 1-105; C. & E.

Layton, 1906.

[7] Edgerton, F. Y.:—“On the Representation of Statistics by Means of

Analytical Geometry,” Jour. Roy. Stat. Soc., 1914, Feb., Mar., May,

June and July.

[8] Elderton, 1. c.

[9] Compare Edgeworth, “A Method of Representing Statistics by

Analytical Geometry,” Proceedings Fifth International Congress of

Mathematicians, Cambridge, 1912.

[10] Only a part of the original table appears in the accompanying

table. The original values were computed to four places of decimals,

but three place numbers are sufficient to illustrate the method of

approximating to the solution.

[11] Compare “Tables for Statisticians and Biometricians,” Cambridge

University Press, 1914.

[12] For the statistical details see Elderton, 1. c.

[13] As may be seen on examining the Table.

A PRELIMINARY LIST OF THE JASSOIDEA OF MISSOURI

WITH NOTES ON SPECIES.

By EDMUND H. GIBSON and ERIC S. COGAN,

U. S. Bureau of Entomology.

The following preliminary list of the Jassoidae of Missouri is mainly

the result of collections and notes made by the authors during the

summer months of 1915. On account of the lack of records for this

state the authors were prompted to undertake such a survey. As far

as possible collections were made so as to embrace all conditions in

different sections, giving some attention to ecological relations. The

list comprises some 98 species.

The Ohio Journal of Science. Vol. XVI., No. 2 (December, 1915) · 第 63 / 76 题