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conformal mapping sphere ↔ horn torus

Due to the hope that a geometrical solution for the conformal mapping between sphere and horn torus could be found, analogue to the Riemannian stereographic projection, it first seemed necessary to nest horn torus and sphere into one another, resulting in a bit confusing drawings and derivation. But until now the search came to no result (Vyacheslav Puha's ingenious method unfortunately is not conformal, and probably no geometrical method does exist), and so we study sphere and horn torus separately. We don't declare any appropriate stereographic projection and try to proof afterwards the conformality but we use instead the conditions of conformality to compile and establish the wanted mapping analytically:
 
One condition for conformal mapping is that small circles on the origin are mapped as small circles on the target surface and therefore we want to construct small circles on both surfaces that only are dependent on the position of points P on the surface, i. e. only dependent on the angles α = ∠NMP for the sphere resp. φ = ∠SMP for the horn torus. Due to rotation symmetry of both figures the rotation angle ω doesn't play any role and is arbitrary, and likewise, because of mirror symmetry, α can be exchanged by π - α (what corresponds to the exchange of north and south pole of the sphere) and φ can be exchanged by 2π - φ. Even the radii r of both figures turn out to be arbitrary and independent. Following drawing shows longitudes, spacing 10°, and latitudes, spacing 20°, P located at angles α = 50° resp. φ = 140°, ω = 35° on both figures:
 

sphere and horn torus

We consider the small circle around any point P and state the condition that the
radii dm (in direction of meridians) and dl (parallel to latitudes) have to be equal.
 
Lengths m of longitudes (meridians) on both figures, sphere and horn torus, are

m = 2π·r

Lengths l of latitudes are computed differently (* see supplement for derivation):

l = 2π·r·sinα on the sphere and   
l = 2π·r·(1 - cosφ) on horn torus *

The differentials dm - radii of the respective small circles on the longitude - are

dm = r·dα on the sphere and
dm = r·dφ on the horn torus.

The differentials dl - radii of the respective small circles on the latitude - are

dl = dω·r·sinα on the sphere and  
dl = dω·r·(1 - cosφ) on the horn torus.

After equalling dm and dl in both figures separately and cancelling r one has

dα = dω·sinα for the sphere and  
dφ = dω·(1 - cosφ) for horn torus.

By solving both equations to dω and equalling we get the differential equation

dα/sinα = dφ/(1 - cosφ)

and finally by integration we obtain the condition for conformal mapping

(1/sinα)dα  =  (1/(1 - cosφ))dφ
 
ln(|tan(α/2)|)  =  - cot(φ/2) + C  

sphere → horn torus:
φ  =  2·arccot(-ln(|tan(α/2)|) - C)
 
horn torus → sphere:
α  =  2·arctan(e^(-cot(φ/2) + C))
 

(0 < α < π, 0 < φ < 2π, C any real number)

C is a kind of 'zoom/diminishing factor' for the mapped figures and shifts them:
case α → φ: φ moves towards 2π with increasing C > 0, towards 0 with C < 0,
case φ → α: α moves towards  π  with increasing C > 0, towards 0 with C < 0,
conformality is given for C ≠ 0 as well, i. e. there is an infinite set of solutions -
but mappings are not bijective, when C ≠ 0 is the same in the inverse mapping
(likewise: Riemann stereographic projection is a special case amongst others)

© 2018 Wolfgang W. Daeumler, Perouse
 
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images: sphere, horn torus, latitude · remark on relevance · context
 


 

* supplement: length of horn torus latitude

 
horn torus latitude
 

The sketch shows details of a horn torus cross section, embedded in a slightly tilted perspective view, point P is positioned on longitude ω (rotation angle) 90° and latitude φ (torus bulge revolution angle) 135°, S is center of horn torus, M center of circle (half of cross section) with radius r, Q is center of selected latitude through P and lies on main symmetry axis, auxiliary line MR is perpendicular to QP, auxiliary line PL perpendicular to diameter of horn torus cross section circle through S and M. With these points and parameters we easily can calculate length l of the latitude with radius QP:
 
QP = QR + RP
    = SM + ML
    = r + r·cos(π - φ)
    = r − r·cosφ
    = r·(1 − cosφ)
 
  l = 2π·QP
 
  l = 2π·r·(1 − cosφ) 
 
 
 

 
remark on dynamic horn torus:  
the horn torus is an excellent graphic representation of complex numbers, a compactification with considerable more properties than the Riemann sphere has, it connects zero and infinity in an amazing way, can be dynamised by two independent turns, rotation around the axis and revolution around the torus bulge, what creates an incredible complexity and forms a coherent comprehensive entity, also explaining the self-interacting capability and fractal order of complex numbers, and finally - most important - horn tori can be interlaced into one another and so symbolise interactions between entities, easily interpretable as physical objects: 'space', 'time', 'particles', 'forces' ...   home