Research article Special Issues

Kinematic-geometry of lines with special trajectories in spatial kinematics

  • This paper derives the expressions for kinematic-geometry of lines with special trajectories in spatial kinematics by means of the E. Study map. A particular assurance goes to the 2nd order movement characteristics for extracting a new proof of the Disteli formulae of the axodes. Meanwhile, a new height dual function is defined and utilized to investigate the geometrical properties of the Disteli-axis. Consequently, as an implementation, the spatial equivalent of the cubic of stationary curvature is established and researched. Finally, Disteli formulae of a line-trajectory are extracted and inspected in detail.

    Citation: Nadia Alluhaibi, Rashad A. Abdel-Baky. Kinematic-geometry of lines with special trajectories in spatial kinematics[J]. AIMS Mathematics, 2023, 8(5): 10887-10904. doi: 10.3934/math.2023552

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  • This paper derives the expressions for kinematic-geometry of lines with special trajectories in spatial kinematics by means of the E. Study map. A particular assurance goes to the 2nd order movement characteristics for extracting a new proof of the Disteli formulae of the axodes. Meanwhile, a new height dual function is defined and utilized to investigate the geometrical properties of the Disteli-axis. Consequently, as an implementation, the spatial equivalent of the cubic of stationary curvature is established and researched. Finally, Disteli formulae of a line-trajectory are extracted and inspected in detail.



    Line geometry possesses a close relationship to spatial kinematics and has thence found implementations in robot kinematics and mechanisms [1,2,3,4]. Spatial kinematics considers the intrinsic properties of the line trajectory from the notions of ruled surfaces in differential line geometry. As we know, in spatial kinematics, the instantaneous screw axis (ISA) of a moveable body forms a pair of ruled surfaces, i.e., the moveable and stationary axodes, with ISA as their generating line in the moveable space and in the stationary space, respectively. In the movement the axodes roll and slide relative to each other in a private way such that the tangential contact between the axodes is constantly maintained over the entire length of the two matting rulings (one being in each axode), which together define the ISA at any instant. It is considerable that not only does a private movement give rise to a unique set of axodes, but the converse also applies. This means that, should the axodes of any movement be known, the particular movement can be created without knowledge of the physical members of the mechanism, their configuration, specific dimensions, or the means by which they are fastened. The use of axodes in the process of synthesis becomes apparent when the axodes are intermediary between the physical mechanism and the actual movement of its members[5,6,7,8,9].

    Rather unexpectedly, dual numbers have been utilized to consider the movement of a line space; they appear even to be the more convenient tools for this end. In dual number and screw algebra, the E. Study map concludes that the family of the dual points on the dual unit sphere in the dual 3-space D3 is in one-to-one correspondence with the family of all oriented lines in Euclidean 3-space E3. According to this map, a one parameter family of points (a dual curve) on the dual unit sphere matches to a one-parameter family of oriented lines (ruled surface) in E3. Additional features of the E. Study's map can be found in [10,11,12,13,14,15,16,17,18,19].

    In this work, based on the axodes, the invariants and the features of a line trajectory in spatial kinematics are investigated. Meanwhile, a new height dual function is defined and utilized to extend the planar and spherical results to spatial kinematics. The classical results of spatial kinematics are obtained in this way, as well as new loci of lines which instantaneously generate special trajectories. The torsion line congruence is established and researched in detail, and the invariants of the axodes are utilized for establishing a new proof of the Disteli formulae.

    In this section, we give a brief outline of the theory of dual numbers and dual vectors [1,2,3,4,5,10,11,12,13,14,15,16,17,18]. If x,and x are real numbers, the number ˆx=x+εx is named a dual number. Here, ε is a dual unit subject to ε0,ε2=0,ε.1=1.ε=ε. The set of dual numbers, D, creates a commutative ring having the numbers εx(xR) as divisors of zero, not a field. No number εx has inverse in the algebra. However, the other laws of the algebra of dual numbers are the same as of the complex numbers. The set

    D3={ˆx:=x+εx=(^x1,ˆx2,ˆx3)}, (2.1)

    together with the Euclidean scalar product

    <ˆx,ˆy>=ˆx1ˆy1+ˆx2ˆy2+ˆx3ˆy3, (2.2)

    forms the so named dual 3-space D3. This yields

    <ˆf1,ˆf1>=<ˆf2,ˆf2>=<ˆf3,ˆf3>=1,ˆf1׈f2=ˆf3ˆf2׈f3=ˆf1ˆf3׈f1=ˆf2, (2.3)

    where ˆf1, ˆf2, and ˆf3, are the dual base at the origin point ˆ0(0,0,0) of the dual 3-space D3. Then, a dual vector ˆx=(ˆx1,ˆx2,ˆx3)t has coordinates ˆxi=(xi+εxi)D. If x0, the norm ˆx of ˆx is defined by

    ˆx=|<ˆx,ˆx>|=x(1+ε<x,x>x2).

    Then, the vector ˆx is named a dual unit vector if ˆx2=1. It is evident that

    ˆx2=1x2=1,<x,x>=0. (2.4)

    The six components xi,xi(i=1,2,3) of xand x are named the normed Plücker coordinates of ˆx. The dual unit sphere is:

    K={ˆxD3ˆx21+ˆx22+ˆx23=1}.

    Via this we have the E. Study map[1,2,3,4,5]: The set of points on dual unit sphere K in the dual 3-space D3 are in one-to-one correspondence with the set of oriented lines in the Euclidean 3-space E3.

    The representation of oriented lines in E3 by dual unit vectors brings sundry advantages, and from now on we do not distinguish between oriented lines and their corresponding dual unit vectors.

    Let Km and Kf be two dual unit spheres with ˆ0 as a mutual center in D3. Let {ˆe}={ˆ0;  ˆe1,ˆe2,ˆe3} and {ˆf}={ˆ0; ˆf1, ˆf2, ˆf3} be two orthonormal dual frames rigidly related with Km and Kf, respectively. If we set {ˆf} as stationary, whereas the elements of set {ˆe} are functions of a real parameter tR (say, the time), then we may say that Km moves with respect to Kf. This movement is named a one-parameter dual spherical movement and will be denoted by Km/Kf. According to the E. Study map, if Km and Kf represent to the line spaces Lm and Lf, respectively, then Km/Kf represents the one-parameter spatial movement Lm/Lf. Therefore, Lm is the moveable space with respect to the fixed space Lf in E3.

    Let us now introduce a further dual unit sphere Kr addressed by the orthonormal dual frame {ˆζ}={ˆ0;ˆζ1,ˆζ2,ˆζ3}, which is considered by the 1st order instantaneous properties of the movement as follows: ˆζ1(t)=ζ1(t)+εζ1(t) as the ISA of the movement Lm/Lf, and ˆζ2(t):=ζ2(t)+εζ2(t)=dˆζ1dtdˆζ1dt1 as the mutual central normal of two detached screw axes. A third dual unit vector is ˆζ3(t)=ˆζ1׈ζ2. {ˆζ} is named the relative Blaschke frame, and the lines ˆζ1,ˆζ2, and ˆζ3 intersect at the mutual striction (central) point s of πi(i=m,f) [5,6,7,8,9]. We have dˆsi=dsi+εdsi=dˆζ1dtdt=ˆp(t)dt as the dual arc length of ˆζ1(t). Since ˆp(t)=p+εp contains only first derivatives of ˆζ1(t), it is a first order estimate of the movement Km/Kf, in specific, its dual speed. We let dˆs=ds+εds to designate dˆsi, since they are equal to each other. The tangent vector of the striction curve s(s) is given by [10,11,12,13,14,15,16]:

    dsds=Γi(s)ζ1(s)+μ(s)ζ3(s). (2.5)

    The distribution parameter of πi is

    μ(s):=pp=dsds. (2.6)

    Proposition 1. In the movement Lm/Lf the axodes have the ISA of the position in common, that is, the moveable axode is fastened to the stationary axode over the ISA in the 1st order at any instant t (see Figure 1).

    Figure 1.  Typical portions of axodes.

    Furthermore, the dual arc-length derivative of Kr/Ki is governed by [11,12,13,14,15]:

    Kr/Ki:ddˆs(ˆζ1ˆζ2ˆζ3)=(01010ˆγi0ˆγi0)(ˆζ1ˆζ2ˆζ3), (2.7)

    where

    ˆγi(ˆs)=γi+ε(Γiμγi)=det(ˆζ1,dˆζ1dˆs,d2ˆζ1dˆs2), (2.8)

    is the dual spherical curvature of πi. Via Eq (2.7), the Disteli-axis (evolute or curvature axis) of πi is given by

    ˆbi(ˆs)=bi+εbi=dˆζ1dˆs×d2ˆζ1dˆs2dˆζ1dˆs×d2ˆζ1dˆs2=ˆγiˆζ1+ˆζ3ˆγ2i+1. (2.9)

    Let ˆϕi(ˆs)=ϕi+εϕi be the radius of curvature between ˆζ1 and ˆbi. Then,

    ˆbi(ˆs)=ˆγiˆγ2i+1ˆζ1+1ˆγ2i+1ˆζ3=cosˆϕiˆζ1+sinˆϕiˆζ3, (2.10)

    where

    ˆγi(ˆs)=γi+ε(Γiμγi)=cotˆϕi. (2.11)

    Thus, we obtain

    ˆγf(ˆs)ˆγm(ˆs)=cotˆϕfcotˆϕm. (2.12)

    This is the dual equivalent of a well-known formula of the Euler-Savary equation from ordinary spherical kinematics[1,2,3,4,5,6]. This dual form is a relationship between the two axodes of the movement Lm/Lf. From the real and the dual parts of Eq (2.8), respectively, we get

    cotϕfcotϕm=γfγm, (2.13)

    and

    ϕmsin2ϕmϕfsin2ϕf=ΓmΓfμ(γfγm). (2.14)

    Equation (2.13) together with (2.14) are new Disteli formulae for the axodes of the movement Lm/Lf.

    Now, let us assume that the relative Blaschke frame is fixed in Km. Then,

    Km/Kf:ddˆs(ˆζ1ˆζ2ˆζ3)=ˆω×(ˆζ1ˆζ2ˆζ3), (2.15)

    where ˆω:=ˆωfˆωm=ˆωˆζ1 is the relative angular vector. ˆω=ˆω=ˆω+εˆω=γr+ε(Γrμγr) is the relative dual spherical curvature. It follows that ω=γfγm and ω=ΓfΓmμ(γfγm) are the rotational angular speed and translational angular speed of the movement Lm/Lf, as well as being both invariants in kinematics, respectively.

    Proposition 2. In the movement Lm/Lf, at any instant tR, the pitch h(s) is given by

    h(s):=<ω,ω>ω=ΓfΓmγfγmμ. (2.16)

    In this study, we disregard the pure translational movements, that is, ω0. Also, we omit zero divisors ω=0. Therefore, we shall think about only non-torsional movements, so that the axodes are skew ruled surfaces (μ0).

    For one-parameter spatial movement Lm/Lf, each stationary line ˆx linked with the movable axode, in general, will describe a ruled surface (ˆx) in the stationary space Lf. In kinematics, this ruled surface is referred to as line trajectory. Since all kinematic-geometric characteristics can then be derived with the invariants of the axodes of the movement Lm/Lf. Then, the line trajectory can be obtained in terms of these invariants. Therefore, we consider a dual unit vector ˆx such that its coordinates are

    ˆx(ˆs)=ˆxtˆζ(ˆs),ˆx=(ˆx1ˆx2ˆx3)=(x1+εx1x2+εx2x3+εx3),ˆζ=(ˆζ1ˆζ2ˆζ3), (3.1)

    where

    x21+x22+x23=1,x1x1+x2x2+x3x3=0. (3.2)

    The velocity ˆx and the acceleration ˆx of ˆx stationary in Lm, respectively, are

    dˆxdˆs=ˆω׈x=ˆω(x3ˆζ2+x2ˆζ3) (3.3)

    and

    d2ˆxdˆs2=ˆx3ˆωˆζ1+(ˆx2ˆω2x3dˆωdˆs)ˆζ2+(ˆx2dˆωdˆsˆx1ˆω+ˆx3ˆω2)ˆζ3. (3.4)

    Then,

    dˆxdˆs×d2ˆxdˆs2=ˆω2[(1ˆx21)ˆωˆζ1+ˆx3ˆx]. (3.5)

    The dual arc length dˆu=du+εdu of ˆx(ˆs) is

    dˆu=dˆxdˆsdˆs=ˆω1ˆx21dˆs. (3.6)

    The distribution parameter of (ˆx) is

    λ(u):=dudu=hx1x11x21. (3.7)

    In order to consider the features of (ˆx), the Blaschke frame is determined as:

    ˆx=ˆx(ˆu),ˆt(ˆu)=ˆxˆx1,ˆg(ˆs)=ˆx׈t, (=ddˆu). (3.8)

    The dual unit vectors ˆx, ˆt and ˆg match to three concurrent mutually orthogonal lines in E3. Their mutual point is the central point c on the ruling ˆx. ˆg(ˆu) is the mutual perpendicular to ˆx(ˆu) and ˆx(ˆu+dˆu), and it is considered the central tangent of (ˆx) at the central point. The trajectory of the central point is the striction curve. The line ˆt is the central normal of (ˆx) at the central point. The Blaschke formulae are

    (ˆxˆtˆg)=(01010ˆγ0ˆγ0)(ˆxˆtˆg), (3.9)

    where

    ˆγ(ˆu)=γ+ε(Γλγ)=det(ˆx,ˆx,ˆx)=ˆx1ˆω(1ˆx21)+ˆx3ˆω(1ˆx21)32, (3.10)

    is the dual spherical curvature of ˆx(ˆu). The tangent of the striction curve is given by:

    dc(u)du=Γ(u)x(u)+λ(u)g(u). (3.11)

    The Serret-Frenet frame of ˆx(ˆu) is established through a rotation of (ˆx, ˆg) according to

    (ˆtˆnˆb)=(     01   0sinˆϕ0cosˆϕcosˆϕ0sinˆϕ)(ˆxˆtˆg), (3.12)

    with a certain dual angle ˆϕ=ϕ+εϕ, where ˆb is the binormal, and ˆn is the principal normal. It is clear that ˆb is the Disteli-axis (striction axis or curvature axis) of the ruled surface (ˆx). Thereby, the dual Serret-Frenet formulae are

    (ˆtˆnˆb)=(  0ˆκ0ˆκ 0ˆτ  0ˆτ0)(ˆtˆnˆb),

    where ˆκ(ˆu) is the dual curvature, and ˆτ(ˆu) is the dual torsion of the dual curve ˆx(ˆu)Kf. Also, we may write the following relationships:

    cotˆϕ:=cotϕεϕ(1+cot2ϕ)=ˆγ(ˆu),ˆκ(ˆu)=κ+εκ=1+ˆγ2=1sinˆϕ,ˆτ(ˆu)=τ+ετ=±ˆϕ=±11+ˆγ2ˆγ.} (3.13)

    In analogy with [18,19], a dual point ˆb0 of Kf will be said to be a ˆbk evolute of the dual curve ˆx(ˆu)Kf; for all i such that 1ik, <ˆb0,ˆxi(ˆu)>=0, but <ˆb0,ˆxk+1(ˆu)>≠0. Here, ˆxi indicates the i-th derivatives of ˆx with respect to the dual arc length of ˆx(ˆu)Kf. For the first evolute ˆb of ˆx(ˆu), we have <ˆb,ˆx>=±<ˆb,ˆt>=0, and <ˆb,ˆx>=±<ˆb,ˆx+ˆγˆg>≠0. So, ˆb is at least a ˆb2 evolute of ˆx(ˆu)Kf.

    We now address a differentiable dual function ˆh:I×KfD, by ˆh(ˆu,ˆb0)=<ˆb0,ˆx>. We call ˆh a height dual function on ˆx(ˆu)Kf. We use the notation ˆh(ˆu)=ˆh(ˆu,ˆb0) for any stationary point ˆb0Kf.

    Proposition 3. Under the above notations, the following holds:

    (1) ˆh will be stationary in the 1st approximation if and only if ˆb0Sp{ˆx, ˆg}, that is,

    ˆh=0⇔<ˆx,ˆb0>=0⇔<ˆt,ˆb0>=0ˆb0=ˆa1ˆx+ˆa2ˆg, (3.14)

    for some dual numbers ˆa1,ˆa2D, and ˆa21+ˆa22=1.

    (2) ˆh will be stationary in the 2nd approximation if and only if ˆb0 is ˆb2 evolute of ˆx(ˆu)Kf, that is,

    ˆh=ˆh=0ˆb0=±ˆb. (3.15)

    (3) ˆh will be invariant in the 3rd approximation if and only if ˆb0 is ˆb3 evolute of ˆx(ˆu)Kf, that is,

    ˆh=ˆh=ˆh=0ˆb0=±ˆb, andˆγ0. (3.16)

    (4) ˆh will be stationary in the 4th approximation if and only if ˆb0 is ˆb4 evolute of ˆx(ˆu)Kf, that is,

    ˆh=ˆh=ˆh=ˆh=0ˆb0=±ˆb,ˆγ=0, andˆγ0. (3.17)

    Proof. For the 1st derivative of ˆh we get:

    ˆh=<ˆx,ˆb0>. (3.18)

    So, we get

    ˆh=0⇔<ˆt,ˆb0>=0ˆb0=ˆa1ˆx+ˆa2ˆg; (3.19)

    for some dual numbers ˆa1,ˆa2D, and ˆa21+ˆa22=1, the result is clear.

    (2) Derivative of Eq (3.18) leads to

    ˆh=<ˆx,ˆb0>=<ˆx+ˆγˆg,ˆb0>. (3.20)

    By using Eq (3.19), we have

    ˆh=ˆh=0⇔<ˆx,ˆb0>=<ˆx,ˆb0>=0ˆb0=±ˆx׈xˆx׈x=±ˆb. (3.21)

    (3) Derivative of Eq (3.20) leads to

    ˆh=<ˆx,ˆb0>=(1+ˆγ2)<ˆt,ˆb0>+ˆγ<ˆg,ˆb0>. (3.22)

    Hence, we have

    ˆh=ˆh=ˆh=0ˆb0=±ˆb, and ˆγ0. (3.23)

    (4) By similar arguments, we can also have

    ˆh=ˆh=ˆh=ˆh=0ˆb0=±ˆbˆγ=0, and ˆγ0. (3.24)

    The proof is completed.

    Via the above proposition, we have the following:

    (a) The osculating circle S of ˆx(ˆu)Kf is determined by the equations

    <ˆb0,ˆx>=cosˆϕ, <ˆx,ˆb0>=0,<ˆx,ˆb0>=0, (3.25)

    which are obtained from the status that the osculating circle should have contact of at least 3rd order at ˆx(ˆu0) if and only if ˆγ0.

    (b) The osculating circle S and the curve ˆx(ˆu)Kf have at least 4th order at ˆx(ˆu0) if and only if ˆγ=0, and ˆγ0.

    In this way, by considering the evolutes of ˆx(ˆu)Kf we can get a sequence of evolutes ˆb2, ˆb3, ..., ˆbn. The properties and the relationships among these evolutes and their involute are very interesting problems. For example, it is easy to see that when ˆb0=±ˆb, and ˆτ(ˆu)=0(ˆγ=ˆϕ=0), ˆx(ˆu)Kf is located at ˆϕ=dualconst. relative to ˆb0.

    We now examine the line trajectories which are the spatial equivalent of the cubic of stationary curvature[1,2,3,4,5]. It is obvious that for all points with ˆτ(ˆu)=0, their trajectories lie on a dual great circle up to third order. Then,

    ˆτ(ˆu)=τ+ετ=0ˆγ=const. (3.26)

    Therefore, the spatial equivalent of the cubic of stationary curvature is defined by (a) the line complex defined by the torsion cone C:τ(u)=0, and (b) the line complex defined by the related plane of lines π:τ(u)=0. All the family of lines ˆx of the movable space Lm and also in the plane satisfy π:τ(u)=0 initiating the torsion line congruence. Therefore, the torsion line congruence consists of a family of planes π, each of which is related with a direction of the inflection cone C. Hence, we have proved the following theorem:

    Theorem 1. In one-parameter spatial movement Lm/Lf, consider a family of related lines of the movable axode, such that each one of these lines has analog of a cubic of stationary curvature. Then, this family of lines forms a torsion line congruence which is common lines of the two line complexes τ(u)=0, and τ(u)=0.

    However, from Eq (3.13), we have

    ˆτ(ˆu)=τ+ετ=0ˆϕ(ˆu)=ϕ+εϕ=ˆc(dualconst.). (3.27)

    This means that ϕ=c(realconst.), andϕ=c(realconst.). Hence, each ruled surface in the torsion line congruence is a stationary Disteli-axis ruled surface. Furthermore, from Eq (3.9) we have the ordinary differential equation; ODE, ˆt+ˆκ2ˆt=0. Without loss of generality, we may take ˆt(0)=(0,0,1), and the general solution of the ODE becomes

    ˆt(ˆu)=(a1sin(ˆκˆu),a2sin(ˆκˆu),cos(ˆκˆu)+a3sin(ˆκˆu)),

    for dual constants ˆa1, ˆa2 and ˆa3. Since ˆt2=1, we get ˆa3=0, and ˆa21+ˆa22=1. It follows that x(ˆu) is given by

    ˆx(ˆu)=(a1ˆκcos(ˆκˆu)+ˆb1,ˆa2ˆκcos(ˆκˆu)+ˆb2,1ˆκsin(ˆκˆu)),

    where ˆb1 and ˆb3 are dual constants satisfying ˆa1ˆb2+ˆa2ˆb2=0. We can change the coordinates by

    (ˆ˜x1ˆ˜x2ˆ˜x3)=(ˆa2ˆa10ˆa1ˆa20001)(ˆx1ˆx2ˆx3).

    Then ˆx(ˆu) turns into

    ˆx(ˆφ)=cosˆϑˆζ1+sinˆϑcosˆφˆζ2+sinˆϑsinˆφˆζ3, ˆφ=ˆκˆu, (3.28)

    for a dual constant ˆa2ˆb1+ˆa1ˆb2=cosˆϑ. This means that ϑ=c1(realconst.), andϑ=c1(realconst.). Here, ˆφ=φ+εφ is the dual angle among the projection of ˆx on the plane Sp{ˆζ2,ˆζ3}. This shows that a helical movement of angle φ on the ISA and distance φ over it turns ˆζ3 to be the central normal ˆt of ˆx (Figure 2). According to Eqs (3.11) and (3.28) we instantly find that:

    (ˆxˆtˆg)=(cosˆϑsinˆϑcosˆφsinˆϑsinˆφ   0   sinˆφ   cosˆφsinˆϑcosˆϑcosˆφcosˆϑsinˆφ)(ˆζ1ˆζ2ˆζ3). (3.29)
    Figure 2.  The line ˆx and its Disteli-axis ˆb.

    Consequently, from Eqs (3.11) and (3.29) we get

    ˆb=cosˆαˆζ1+sinˆαˆm, ˆm=cosˆφˆζ2+sinˆφˆζ3, (3.30)

    where

    ˆα=α+εα=ˆϑˆφ. (3.31)

    For more analysis of the torsion line congruence, from Eq (3.28), the Plücker coordinates of ˆx are:

    x1=cosϑx1=ϑsinϑ,x2=sinϑcosφ, x2=ϑcosϑcosφφsinφsinϑ,x3=sinϑsinφ, x3=φcosϑsinφ+φcosφsinϑ.} (4.1)

    Let η(η1,η2,η3) indicate a point on ˆx. Since x=η×x we have the system of linear equations in ηi for i = 1, 2, 3 (ηis are the coordinates of η):

    η2sinϑsinφη3sinϑcosφ=x1,η1sinϑsinφ+η3cosϑ=x2,η1sinϑcosφη2cosϑ=x3.} (4.2)

    The matrix of coefficients of unknowns ηi is the skew symmetric matrix

    (    0sinϑsinφsinϑcosφsinϑsinφ      0cosϑsinϑcosφcosϑ       0),

    and thus its rank is 2 with ϑ2πk (k is an integer). The rank of the augmented matrix

    (    0sinϑsinφsinϑcosφx1sinϑsinφ      0cosϑx2sinϑcosφcosϑ       0x2)

    is also 2. Thereby, this system has infinite solutions given by

    η2sinφη3cosφ=ϑ,η2=(η1φ)tanϑcosφϑsinφ,η3=(η1φ)tanϑsinφ+ϑcosφ. (4.3)

    Since η1can be set arbitrarily, we may set η1=φ. In this case, Eq (4.3) reduces to

    η1=φ, η2=ϑsinφ, η3=ϑcosφ. (4.4)

    If we set φ=hφ and φ as the movement parameter, then (ˆx) is a ruled in Lf-space. We now simply find the base curve as

    η(φ)=hφζ1ϑsinφζ2+ϑcosφζ3. (4.5)

    It can be shown that <η,x>=0, (=ddφ), so the base curve η(φ) of (ˆx) is its striction curve c. The curvature κc(φ) and torsion τc(φ) of c(φ) can be given by

    κc(φ)=ϑϑ2+h2τc(φ)=hϑ2+h2,

    which means that c(φ) is a circular helix. From Eqs (3.11), (3.29) and (4.5) it can be found that

    (Γλ)=(cosϑsinϑsinϑcosϑ)(hϑ).

    Let y(y1,y2,y3) be a point on the oriented line ˆx. Then,

    (ˆx):y(φ,v)=(hφ+vcosϑϑsinφ+vsinϑcosφϑcosφ+vsinϑsinφ), vR. (4.6)

    The constants h, ϑ and ϑ can control the shape of the surface (ˆx). Hence, the major geometrical characteristics of (ˆx) can be described as follows: (ˆx) is a stationary Disteli-axis ruled surface, <c,x>=Γ is constant, <c,g>=λ is constant, and c(φ) is a circular helix.

    Theorem 2. Let (ˆx) be any non-developable ruled surface in Euclidean 3-space E3. Then, (ˆx) is a ruled Weingarten surface if and only if (ˆx) is contained in a torsion line congruence.

    However, via Eq (4.6), the ruled surface can be classified into four types according to the forms of their striction curves.

    (1) Archimedes helicoid when its striction curve is a circular helix; for h=1,ϑ=1,ϑ=π4, 2.5v2.5, and 0φ2π (see Figure 3).

    Figure 3.  General helicoid.

    (2) One-sheeted hyperboloid when its striction curve is a circle; for h=0,ϑ=1,ϑ=π4,2.5v2.5, and 0φ2π (see Figure 4).

    Figure 4.  One-sheeted hyperboloid.

    (3) Right helicoid when its striction curve is a line; for h=1, ϑ=0, ϑ=π2, 2.5v2.5, and 0φ2π (see Figure 5).

    Figure 5.  Right helicoid.

    (4) Circular cone when its striction curve is a fixed point; for h=ϑ=0, ϑ=π4, 2.5v2.5, and 0φ2π (see Figure 6).

    Figure 6.  Circular cone.

    In order to have a straightforward equation of the torsion line congruence, from Eqs (3.10), (3.13) and (3.28) we can write the equation

    ˆτ(ˆu)=±ˆω[3cosˆϑsinˆφ+(ˆωˆγ)sinˆϑ]cosˆφˆωsinˆϑsinˆφˆω2ˆκ2sin3ˆϑ.

    Hence, at any instant, it is apparent that

    ˆτ(ˆu)=0cotˆϑ=ˆacscˆφ+ˆbsecˆφ, (5.1)

    where

    ˆa=a+εa=ˆγˆω3, ˆb(u)=b+εb=ˆω3ˆω. (5.2)

    The real part of Eq (5.1) characterizes the torsion cone for the spherical part of the movement Lm/Lf and is given by

    cotϑ=acscφ+bsecφ,a(u)=γω3, and b(u)=b+εb=ω3ω.} (5.3)

    The intersection of the torsion cone with a unit sphere fastened at the cone's apex gives a spherical curve. Linked with the direction of a line L on the torsion cone, there is a plane π defined by the dual part of Eq (5.1). This plane is

    acscφ+bsecφ+φ(bsecφtanφacscφcotφ)+ϑcsec2ϑ=0. (5.4)

    So, for each direction of a line L of the torsion cone, there is an associated plane of lines parallel to L. The torsion cone and plane of lines defines the torsion line congruence. Hence, if Eq (5.3) is solved with respect to the angle ϑ, then we obtain

    ϑ=cot1(acscφ+bsecφ). (5.5)

    Then, from Eqs (4.1) and (5.5) it follows that

    x(φ)=11+(acscφ+bsecφ)2(acscφ+bsecφ,cosφ,sinφ) (5.6)

    From Eqs (4.6) and (5.5), we can also obtain that

    (ˆx):y(φ,v)=(hφ+v(acscφ+bsecφ)(acscφ+bsecφ)2+1ϑsinφ+vcosφ(acscφ+bsecφ)2+1ϑcosφ+vsinφ(acscφ+bsecφ)2+1), vR. (5.7)

    In the case of 0φ2π, and ϑ0, we get:

    (ˆx):Y21Λ2+y22ϑ2+y23ϑ2=1, (5.8)

    where Λ=ϑ(acscφ+bsecφ), and Y1=y1hφ. Then, (ˆx) is a one-parameter family of one-sheeted hyperboloids. The intersection of each hyperboloid and the corresponding plane y1=φ is one-parameter family of circular cylinders (c): y22+y23=ϑ2 which is the envelope of (ˆx). According to Eqs (5.6) and (5.7) we have the following:

    (1) Spherical torsion curve with its torsion ruled surface: for a=1,b=0.5,ϑ=3,h=1,0φ2π,0v4 (Figures 7 and 8).

    Figure 7.  Torsion curve.
    Figure 8.  Ruled surface.

    (2) Spherical torsion curve with its torsion ruled surface: for a=1, b=0.5, ϑ=3, h=1,0φ2π,0v4 (Figures 9 and 10).

    Figure 9.  Torsion curve.
    Figure 10.  Ruled surface.

    In 1914 Disteli[9] created a curvature axis for a ruled surface and generalized the planar Euler-Savary equation to line trajectories. There are several papers which deal with Euler-Savary formulae and classical geometric invariants of ruled surfaces for several kinds of geometry[4,5,6,7]. The Disteli formula may be given immediately as follows. From Eqs (3.10), (3.13) and (3.28), we obtain

    cotˆϕcotˆϑ=sinˆφˆωsin2ˆϑ. (5.9)

    Equation (5.9) shows the correlations between ˆx(ˆu)Kf which corresponds to the ruled surface (ˆx), and its osculating dual cone, which is corresponding to the Disteli-axis, at any instant. It is comparable to the Euler-Savary equation of a point trajectory in planar and spherical movements in form[1,2,3,4,5]. By separating the real and the dual parts, we get

    cotϕ=cotϑ+sinφωsin2ϑ, (5.10)

    and

    ϕ=sin2ϕω[(h+2ϑcotϑ)sinφφcosϕ]+ϑsin2φsin2ϑ. (5.11)

    Equation (5.10) detects the correlations among the locations of the ruling ˆx in the movable space Lm and the Disteli-axis ˆb. Equation (5.11) depicts the distance from ˆx to the Disteli-axis ˆb. Their geometrical explanations are shown in Figure 2. The sign of ϕ(- or +) indicates that the location of the Disteli-axis ˆb is on the negative or positive orientation of the central normal ˆt of (ˆx). Equations (5.10) and (5.11) are new Disteli formulae of a line trajectory in the movement Lm/Lf. Since the central points of the ruled surfaces are on the normal plane, when the direction of their rulings is defined by the dual unit vector ˆx with (ˆφ,ˆϑ) according to Eq (3.28), the Disteli fomulae (5.10) and (5.11) can be displayed in the plane π:Sp{ζ1,ˆt}. Hence, any arbitrary point c(φ,ϑ) on the plane π is defined as central point of (ˆx) whose ruling is the oriented line ˆx, and the radius ϑ is the line segment from the point q to the point c on the plane π. Also, the vector from q to c is in the positive (resp. negative) orientation of ˆt if ϑ>0 (resp. ϑ<0). The central point c(φ,ϑ) can be on the ISA if ϑ=0 (α=φ) and on the Disteli-axis ˆb if ϕ=0α=ϑ. In the latter case the central point c(φ,ϑ) can be determined by setting ϕ=0 in Eq (5.11) which is clarified as

    L:φ=1cosφ(sin2φsin2ϑ+2cotϑ)ϑ+htanφ. (5.12)

    Equation (5.12) is linear in the position coordinates φand ϑ of ˆx. Hence, in one-parameter spatial movement Lm/Lf the fixed lines in Lm lie on a plane. The line L will change its location if the parameter ϑ is defined as a varying value, but φ=constant. However, a set of lines envelops a curve on the plane π. Meanwhile, the π has several positions if the parameter φ of a line has several values, but ϑ=constant. Therefore, the set of all lines L defined by Eq (5.12) is a line congruence for all values of (φ,ϑ).

    On the other hand, we can derive other dual version of the Euler-Savary equation as follows: Substituting Eq (3.5) into Eq (3.21), we have

    ˆb=ˆω2[(1ˆx21)ˆωˆζ1+ˆx3ˆx]ˆx׈x. (5.13)

    Thus, from Eqs (3.1), (3.30) and (5.13), one finds that:

    (1ˆx21)ˆω+ˆx1ˆx3cosˆα=ˆx2ˆx3sinˆαcosˆφ=ˆx23sinˆαsinˆφ. (5.14)

    Substituting Eq (3.28) into Eq (5.14), we obtain

    cotˆαcotˆϑ=ˆωsinˆφ. (5.15)

    This is exactly a second dual extension of the Euler-Savary equation. From the real and the dual parts, respectively, we get:

    cotαcotϑ=ωsinφ, (5.16)

    and

    φ(cotαcotϑ)cosφ(αsin2αϑsin2ϑ)sinφ=ωsinφ(hμ). (5.17)

    Once the angles α and ϑ are known, Eq (5.17) gives the correspondence between α and ϑ in terms of (φ, φ) and the 2nd order invariant ωsinφ(hμ). The spherical Euler-Savary Eq (5.16) and (5.17) are new Disteli formulae of spatial kinematics.

    For one-parameter spatial movement Lm/Lf, based on E. Study, expressions of the axodes and their invariants were derived, and then the geometric–kinematic meanings were revealed. By employing the Blaschke frames, the properties of a line trajectory and its Disteli axis were researched. Interestingly, the results slightly explain the analogies between point geometry of spherical curves in Euclidean 3-space E3 and point geometry of dual spherical curves in dual 3-space D3. Hence, the invariants of the axodes were utilized for obtaining new proof of the Disteli-formulae for a line trajectory in spatial kinematics.

    The study of spatial kinematics in Euclidean 3-space E3 via the geometry of lines may be adopted to research some problems and conclude new applications. For future research, we will attract with the design of ruled surfaces as tooth flanks for gears with skew axes, as offered in [7].

    The authors declare that there is no conflict of interests regarding the publication of this paper.



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