Difference between revisions of "Strip (generalized)"
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''surface strip (in the narrow sense)'' | ''surface strip (in the narrow sense)'' | ||
− | A one-parameter family of planes tangent to a surface. In the general sense, a strip is the union of a curve | + | A one-parameter family of planes tangent to a surface. In the general sense, a strip is the union of a curve $ l $ |
+ | and a vector $ \mathbf m $ | ||
+ | orthogonal to the tangent vector of the curve at each of its points. Suppose that $ l $ | ||
+ | is given in the space $ \mathbf R ^ {3} $ | ||
+ | by an equation $ \mathbf r = \mathbf r ( s) $, | ||
+ | where $ s $ | ||
+ | is the natural parameter of the curve and $ \mathbf r ( s) $ | ||
+ | is the position vector of the points of the curve. Along $ l $ | ||
+ | one has a vector-function $ \mathbf m = \mathbf m ( s) $, | ||
+ | where $ \mathbf m ( s) $ | ||
+ | is a unit vector orthogonal to the tangent vector $ \mathbf t = d \mathbf r / d s $ | ||
+ | at the corresponding points of the curve. One then says that a surface strip $ \Phi = \{ l , \mathbf m \} $ | ||
+ | with normal $ \mathbf m ( s) $ | ||
+ | is defined along $ l $. | ||
+ | The vector $ \pmb\tau = [ \mathbf m , \mathbf t ] $ | ||
+ | is called the geodesic normal vector of $ \Phi $; | ||
+ | together with $ \mathbf t $ | ||
+ | and $ \mathbf m $, | ||
+ | the vector $ \pmb\tau $ | ||
+ | forms the Frénet frame for the strip. Given the moving Frénet frame for a strip, one has the Frénet derivation formulas: | ||
+ | |||
+ | $$ | ||
+ | |||
+ | \frac{d \mathbf t }{ds} | ||
+ | = k _ {g} \pmb\tau + k _ {n} \mathbf m ; \ | ||
+ | |||
+ | \frac{d \pmb\tau }{ds} | ||
+ | = - k _ {g} \mathbf t + \kappa _ {g} \mathbf m ; | ||
+ | $$ | ||
− | + | $$ | |
− | + | \frac{d \mathbf m }{ds} | |
+ | = - k _ {n} \mathbf t + \kappa _ {g} \pmb\tau , | ||
+ | $$ | ||
− | where | + | where $ k _ {g} $ |
+ | denotes the geodesic curvature of the strip, $ k _ {n} ( s) $ | ||
+ | denotes its normal curvature and $ \kappa _ {g} ( s) $ | ||
+ | denotes its geodesic torsion, which are scalar functions of $ s $. | ||
− | If the vector | + | If the vector $ \mathbf m $ |
+ | is collinear with the [[Principal normal|principal normal]] at each point of $ l $, | ||
+ | then $ k _ {g} = 0 $ | ||
+ | and the strip is then called a geodesic strip. If $ \mathbf m $ | ||
+ | is collinear with the [[Binormal|binormal]] of the curve at each point, one has $ k _ {n} = 0 $ | ||
+ | and the strip is called an asymptotic strip. | ||
====References==== | ====References==== | ||
<table><TR><TD valign="top">[1]</TD> <TD valign="top"> W. Blaschke, "Einführung in die Differentialgeometrie" , Springer (1950)</TD></TR></table> | <table><TR><TD valign="top">[1]</TD> <TD valign="top"> W. Blaschke, "Einführung in die Differentialgeometrie" , Springer (1950)</TD></TR></table> |
Latest revision as of 08:23, 6 June 2020
surface strip (in the narrow sense)
A one-parameter family of planes tangent to a surface. In the general sense, a strip is the union of a curve $ l $ and a vector $ \mathbf m $ orthogonal to the tangent vector of the curve at each of its points. Suppose that $ l $ is given in the space $ \mathbf R ^ {3} $ by an equation $ \mathbf r = \mathbf r ( s) $, where $ s $ is the natural parameter of the curve and $ \mathbf r ( s) $ is the position vector of the points of the curve. Along $ l $ one has a vector-function $ \mathbf m = \mathbf m ( s) $, where $ \mathbf m ( s) $ is a unit vector orthogonal to the tangent vector $ \mathbf t = d \mathbf r / d s $ at the corresponding points of the curve. One then says that a surface strip $ \Phi = \{ l , \mathbf m \} $ with normal $ \mathbf m ( s) $ is defined along $ l $. The vector $ \pmb\tau = [ \mathbf m , \mathbf t ] $ is called the geodesic normal vector of $ \Phi $; together with $ \mathbf t $ and $ \mathbf m $, the vector $ \pmb\tau $ forms the Frénet frame for the strip. Given the moving Frénet frame for a strip, one has the Frénet derivation formulas:
$$ \frac{d \mathbf t }{ds} = k _ {g} \pmb\tau + k _ {n} \mathbf m ; \ \frac{d \pmb\tau }{ds} = - k _ {g} \mathbf t + \kappa _ {g} \mathbf m ; $$
$$ \frac{d \mathbf m }{ds} = - k _ {n} \mathbf t + \kappa _ {g} \pmb\tau , $$
where $ k _ {g} $ denotes the geodesic curvature of the strip, $ k _ {n} ( s) $ denotes its normal curvature and $ \kappa _ {g} ( s) $ denotes its geodesic torsion, which are scalar functions of $ s $.
If the vector $ \mathbf m $ is collinear with the principal normal at each point of $ l $, then $ k _ {g} = 0 $ and the strip is then called a geodesic strip. If $ \mathbf m $ is collinear with the binormal of the curve at each point, one has $ k _ {n} = 0 $ and the strip is called an asymptotic strip.
References
[1] | W. Blaschke, "Einführung in die Differentialgeometrie" , Springer (1950) |
Strip (generalized). Encyclopedia of Mathematics. URL: http://encyclopediaofmath.org/index.php?title=Strip_(generalized)&oldid=48872