diff options
Diffstat (limited to 'docs/source/operations')
| -rw-r--r-- | docs/source/operations/projections/calcofi.rst | 4 | ||||
| -rw-r--r-- | docs/source/operations/projections/cass.rst | 5 | ||||
| -rw-r--r-- | docs/source/operations/projections/ccon.rst | 4 | ||||
| -rw-r--r-- | docs/source/operations/projections/eqc.rst | 2 | ||||
| -rw-r--r-- | docs/source/operations/projections/gall.rst | 2 | ||||
| -rw-r--r-- | docs/source/operations/projections/merc.rst | 4 | ||||
| -rw-r--r-- | docs/source/operations/projections/mill.rst | 4 | ||||
| -rw-r--r-- | docs/source/operations/projections/qsc.rst | 12 | ||||
| -rw-r--r-- | docs/source/operations/transformations/deformation.rst | 2 | ||||
| -rw-r--r-- | docs/source/operations/transformations/molodensky.rst | 4 |
10 files changed, 21 insertions, 22 deletions
diff --git a/docs/source/operations/projections/calcofi.rst b/docs/source/operations/projections/calcofi.rst index 8a240ebd..8b2924de 100644 --- a/docs/source/operations/projections/calcofi.rst +++ b/docs/source/operations/projections/calcofi.rst @@ -82,8 +82,8 @@ Options Mathematical definition ################################################################################ -The algorithm used to make conversions is described in [EberHewitt1979]_ with -a few corrections reported in [WeberMoore2013]_. +The algorithm used to make conversions is described in :cite:`EberHewitt1979` with +a few corrections reported in :cite:`WeberMoore2013`. Further reading diff --git a/docs/source/operations/projections/cass.rst b/docs/source/operations/projections/cass.rst index dba6a7c4..2b2ebf01 100644 --- a/docs/source/operations/projections/cass.rst +++ b/docs/source/operations/projections/cass.rst @@ -30,7 +30,7 @@ Although the Cassini projection has been largely replaced by the Transverse Merc Usage ##### -There has been little usage of the spherical version of the Cassini, but the ellipsoidal Cassini-Soldner version was adopted by the Ordnance Survey for the official survey of Great Britain during the second half of the 19th century [Steers1970]_. +There has been little usage of the spherical version of the Cassini, but the ellipsoidal Cassini-Soldner version was adopted by the Ordnance Survey for the official survey of Great Britain during the second half of the 19th century :cite:`Steers1970`. Many of these maps were prepared at a scale of 1:2,500. The Cassini-Soldner was also used for the detailed mapping of many German states during the same period. @@ -67,7 +67,7 @@ Options Mathematical definition ####################### -The formulas describing the Cassini projection are taken from Snyder's [Snyder1987]_. +The formulas describing the Cassini projection are taken from :cite:`Snyder1987`. :math:`\phi_0` is the latitude of origin that match the center of the map (default to 0). It can be set with ``+lat_0``. @@ -162,5 +162,4 @@ Further reading ############### #. `Wikipedia <https://en.wikipedia.org/wiki/Equirectangular_projection>`_ -#. [Snyder1987]_ #. `EPSG, POSC literature pertaining to Coordinate Conversions and Transformations including Formulas <http://www.ihsenergy.com/epsg/guid7.pdf>`_ diff --git a/docs/source/operations/projections/ccon.rst b/docs/source/operations/projections/ccon.rst index f5ceed67..e267f271 100644 --- a/docs/source/operations/projections/ccon.rst +++ b/docs/source/operations/projections/ccon.rst @@ -39,7 +39,7 @@ conformal. An example of usage (and the main reason to implement this projection in proj4) is the ATPOL geobotanical grid of Poland, developed in Institute of Botany, -Jagiellonian University, Krakow, Poland in 1970s [Zajac1978]_. The grid was +Jagiellonian University, Krakow, Poland in 1970s :cite:`Zajac1978`. The grid was originally handwritten on paper maps and further copied by hand. The projection (together with strange Earth radius) was chosen by its creators as the compromise fit to existing maps during first software development in DOS era. Many years later @@ -51,7 +51,7 @@ The ATPOL coordinates can be achieved with with the following parameters: +proj=ccon +lat_1=52 +lon_0=19 +axis=esu +a=6390000 +x_0=330000 +y_0=-350000 -For more information see [Komsta2016]_ and [Verey2017]_. +For more information see :cite:`Komsta2016` and :cite:`Verey2017`. Parameters ################################################################################ diff --git a/docs/source/operations/projections/eqc.rst b/docs/source/operations/projections/eqc.rst index de463034..b81f9ded 100644 --- a/docs/source/operations/projections/eqc.rst +++ b/docs/source/operations/projections/eqc.rst @@ -89,7 +89,7 @@ Parameters Mathematical definition ####################### -The formulas describing the Equidistant Cylindrical projection are all taken from Snyder's [Snyder1987]_. +The formulas describing the Equidistant Cylindrical projection are all taken from :cite:`Snyder1987`. :math:`\phi_{ts}` is the latitude of true scale, that mean the standard parallels where the scale of the projection is true. It can be set with ``+lat_ts``. diff --git a/docs/source/operations/projections/gall.rst b/docs/source/operations/projections/gall.rst index bdb88895..1b0da9e8 100644 --- a/docs/source/operations/projections/gall.rst +++ b/docs/source/operations/projections/gall.rst @@ -69,7 +69,7 @@ Parameters Mathematical definition ####################### -The formulas describing the Gall Stereographical are all taken from Snyder's [Snyder1993]_. +The formulas describing the Gall Stereographical are all taken from :cite:`Snyder1993`. Spherical form ************** diff --git a/docs/source/operations/projections/merc.rst b/docs/source/operations/projections/merc.rst index 2d419c02..349de216 100644 --- a/docs/source/operations/projections/merc.rst +++ b/docs/source/operations/projections/merc.rst @@ -37,7 +37,7 @@ Applications should be limited to equatorial regions, but is frequently used for navigational charts with latitude of true scale (:option:`+lat_ts`) specified within or near chart's boundaries. Often inappropriately used for world maps since the regions near the poles -cannot be shown [Evenden1995]_. +cannot be shown :cite:`Evenden1995`. Example using latitude of true scale:: @@ -76,7 +76,7 @@ Parameters Mathematical definition ####################### -The formulas describing the Mercator projection are all taken from G. Evenden's libproj manuals [Evenden2005]_. +The formulas describing the Mercator projection are all taken from G. Evenden's libproj manuals :cite:`Evenden2005`. Spherical form ************** diff --git a/docs/source/operations/projections/mill.rst b/docs/source/operations/projections/mill.rst index 718d4b9b..fb2096c9 100644 --- a/docs/source/operations/projections/mill.rst +++ b/docs/source/operations/projections/mill.rst @@ -32,7 +32,7 @@ Usage ######## The Miller Cylindrical projection is used for world maps and in several atlases, -including the National Atlas of the United States (USGS, 1970, p. 330-331) [Snyder1987]_. +including the National Atlas of the United States (USGS, 1970, p. 330-331) :cite:`Snyder1987`. Example using Central meridian 90°W:: @@ -55,7 +55,7 @@ Parameters Mathematical definition ####################### -The formulas describing the Miller projection are all taken from Snyder's manuals [Snyder1987]_. +The formulas describing the Miller projection are all taken from :cite:`Snyder1987`. Forward projection diff --git a/docs/source/operations/projections/qsc.rst b/docs/source/operations/projections/qsc.rst index 56d4ea3f..e6b0d1b0 100644 --- a/docs/source/operations/projections/qsc.rst +++ b/docs/source/operations/projections/qsc.rst @@ -36,15 +36,15 @@ It is an equal-area projection, and at the same time introduces only limited ang distortions. It treats all cube sides equally, i.e. it does not use different projections for polar areas and equatorial areas. These properties make QSC projection a good choice for planetary-scale terrain rendering. Map data can be -organized in quadtree structures for each cube side. See [LambersKolb2012]_ for an example. +organized in quadtree structures for each cube side. See :cite:`LambersKolb2012` for an example. -The QSC projection was introduced by [ONeilLaubscher1976]_, -building on previous work by [ChanONeil1975]_. For clarity: The -earlier QSC variant described in [ChanONeil1975]_ became known as the COBE QSC since it +The QSC projection was introduced by :cite:`ONeilLaubscher1976`, +building on previous work by :cite:`ChanONeil1975`. For clarity: The +earlier QSC variant described in :cite:`ChanONeil1975` became known as the COBE QSC since it was used by the NASA Cosmic Background Explorer (COBE) project; it is an approximately equal-area projection and is not the same as the QSC projection. -See also [CalabrettaGreisen2002]_ Sec. 5.6.2 and 5.6.3 for a description of both and +See also :cite:`CalabrettaGreisen2002` Sec. 5.6.2 and 5.6.3 for a description of both and some analysis. In this implementation, the QSC projection projects onto one side of a circumscribed @@ -65,7 +65,7 @@ cube. The cube side is selected by choosing one of the following six projection +-------------------------+--------------------+ Furthermore, this implementation allows the projection to be applied to ellipsoids. -A preceding shift to a sphere is performed automatically; see [LambersKolb2012]_ for details. +A preceding shift to a sphere is performed automatically; see :cite:`LambersKolb2012` for details. Usage diff --git a/docs/source/operations/transformations/deformation.rst b/docs/source/operations/transformations/deformation.rst index 2e6f012d..13614f5c 100644 --- a/docs/source/operations/transformations/deformation.rst +++ b/docs/source/operations/transformations/deformation.rst @@ -38,7 +38,7 @@ writes both file formats. Using GDAL for construction of new grids is recommende Example ------------------------------------------------------------------------------- -In [Häkli2016]_ coordinate transformation including a deformation model is described. +In :cite:`Hakli2016` coordinate transformation including a deformation model is described. The paper describes how coordinates from the global ITRFxx frames are transformed to the local Nordic realisations of ETRS89. Scandinavia is an area with significant post-glacial rebound. The deformations from the post-glacial uplift is not accounted for in the diff --git a/docs/source/operations/transformations/molodensky.rst b/docs/source/operations/transformations/molodensky.rst index a90828cd..347165c8 100644 --- a/docs/source/operations/transformations/molodensky.rst +++ b/docs/source/operations/transformations/molodensky.rst @@ -16,7 +16,7 @@ differences between the semimajor axes and flattening parameters of the referenc ellipsoids. Due to its algorithmic simplicity, it was popular prior to the ubiquity of digital computers. Today, it is mostly interesting for historical reasons, but nevertheless indispensable due to the large amount of data that has -already been transformed that way [EversKnudsen2017]_. +already been transformed that way :cite:`EversKnudsen2017`. +---------------------+----------------------------------------------------------+ | **Alias** | molodensky | @@ -45,7 +45,7 @@ is that it is fairly simple to compute by hand. The ease of computation come at cost of limited accuracy. A derivation of the mathematical formulas for the Molodensky transform can be found -in [Deakin2004]_. +in :cite:`Deakin2004`. Examples |