Navigational algorithms

Comparison between manual calculation methods and the use of calculators

• The traditional methods require bulky and expensive nautical tables (which must be uSmartphoneted), pencil and paper, and calculation time, following the working algorithms.
• Calculators (and the like) do not need books (they have tables and ephemeris integrated) and, with their own algorithms, allow quick and error-free calculation of navigation problems.

Types of algorithms

• Celestial navigation: Sight reduction, circle of equal altitude, Line Of Position, Fix...
• Positional astronomy: RA, GHA, Dec
• Coastal navigation: Range, Bearing, Horizontal angles, IALA...
• Sailings: Rhumbs, Loxodromic, Orthodromic, Meridional parts...
• Weather, tides
• Software PC- Smartphone: Nautical Almanac, Sailings, Variation, Sextant corrections

Programs for general navigation

Programs on the nautical chart, directions, coastal navigation and beacons, nautical publications. The astronomical navigation section includes the resolution of the position triangle, the usefulness of a height line, the recognition of stars and the determinant of the height line, in addition to other topics of interest in nautical: tides, naval kinematics, meteorology and hurricanes, and oceanography. All heading measurements made with a magnetic compass or compass must be corrected for magnetic declination or local variation.

Coordinate conversion subroutine

sub Rectang2Polar (a () as double, b () as double) static '----- Subprograma para convertir un vector de estado coord.cartesianas '----- En vector de estado en coord.polars. '----- De entrada: vector de estado en coord.cartesianes '----- De salida: vector de estado en coord.polars. '----- NOTA: El vector de velocidad polar es el de la velocidad total, '----- Corregido por el efecto de la latitud. '------------------------------------------------- ------------------------ mar x as double mar y as double mar z as double mar x_dot as double mar y_dot as double mar z_dot as double mar rho as double mar r as double mar lambda as double mar beta as double mar lambda_dot as double mar beta_dot as double mar r_dot as double x = a (1) y = a (2) z = a (3) x_dot = a (4) y_dot = a (5) z_dot = a (6) rho = sqr (x * x+y * y) r = sqr (rho * rho+z * z) lambda = atan2 (y, x) beta = atan2 (z, rho) if (z yf rho = 0 # then lambda_dot = 0 # beta_dot = 0 # else lambda_dot = (x * y_dot - y * x_dot)/(rho * rho) beta_dot = (z_dot * rho * rho - z * (x * x_dot+_ y * y_dot))/(r * r * rho) end if r_dot = (x * x_dot+y * y_dot+z * z_dot)/r '----- Componentes del vector de posición b (1) = lambda if b (1) = TWOPI then b (1) = b (1) - TWOPI b (2) = beta b (3) = r '----- Componentes del vector velocidad total b (4) = r * lambda_dot * cuerpo (beta) b (5) = r * beta_dot b (6) = r_dot end sub

Programs for astronomical navigation

Advanced navigation algorithms include piloting and astronomical navigation: loxodromia and orthodromia. Height correction of the sextant . Astronomical position with calculator, template and blank mercantile chart. Position by 2 Lines of Height. Position from n Height Lines. Vector equation of the Height Circle. Position for vector solution from two observations. Position by Height Circles: matrix solution. And articles related to ancient procedures such as obtaining latitude by the pole star, the meridian, the method of lunar distances, etc.

Programs for the "Nautical Almanac"

• GHA - Greenwich Hour Angle
• Dec - Declination
• SD - Semidiameter
• HP - Horizontal Parallax
• s the solution for course and SOG.

CelestialFix

They solve the problem of calculating the position from observations of the stars made with the sextant in Astronomical Navigation.

Algorithm implementation:

For n = 2 observations

• An analytical solution of the two star sight problem of celestial navigation, James A. Van Allen.
  • Vector Solution for the Intersection of two Circles of Equal Altitude. Andrés Ruiz. For n ≥ 2 observations
• DeWit/USNO Nautical Almanac/Compac Data, Least squares algorithm for n LOPs
• Kaplan algorithm, USNO. For n ≥ 8 observations, gives the solution for course and SOG.

Magnetic declination

Any measure of course made with a magnetic compass must be corrected because of the magnetic declination or local variation.

References

References

1. An analytical solution of the two star sight problem of celestial navigation. James A. Van Allen. NAVIGATION Vol. 28, No. 1, 1981
2. [http://journals.cambridge.org/action/displayAbstract?fromPage=online&aid=1814560&fileId=S0373463307004602 Vector Solution for the Intersection of Two Circles of Equal Altitude. Andrés Ruiz González. Journal of Navigation, Volume 61, Issue 02, April 2008, p. 355-365.The Royal Institute of Navigation]
3. Determining the Position and Motion of a Vessel from Celestial Observations, Kaplan, G. H. Navigation, Vol. 42, No. 4, 1995, pp. 631–648