A1_calcSol {solaR} R Documentation

## Apparent movement of the Sun from the Earth

### Description

Compute the apparent movement of the Sun from the Earth with the functions fSolD and fSolI.

### Usage

calcSol(lat, BTd, sample = 'hour', BTi,
EoT = TRUE, keep.night = TRUE,
method = 'michalsky')


### Arguments

 lat Latitude (degrees) of the point of the Earth where calculations are needed. It is positive for locations above the Equator. BTd Daily time base, a POSIXct object which may be the result of fBTd. It is not considered if BTi is provided. sample Increment of the intradaily sequence. It is a character string, containing one of ‘"sec"’, ‘"min"’, ‘"hour"’. This can optionally be preceded by a (positive or negative) integer and a space, or followed by ‘"s"’. It is used by seq.POSIXt. It is not considered if BTi is provided. BTi Intradaily time base, a POSIXct object to be used by fSolI. It could be the index of the G0I argument to calcG0. EoT logical, if TRUE the Equation of Time is used. Default is TRUE. keep.night logical, if TRUE (default) the night is included in the time series. method character, method for the sun geometry calculations to be chosen from 'cooper', 'spencer', 'michalsky' and 'strous'. See references for details.

### Value

A Sol-class object.

### Author(s)

Oscar Perpiñán Lamigueiro.

### Examples

BTd = fBTd(mode = 'serie')

lat = 37.2
sol = calcSol(lat, BTd[100])
print(as.zooD(sol))

library(lattice)
xyplot(as.zooI(sol))

solStrous = calcSol(lat, BTd[100], method = 'strous')
print(as.zooD(solStrous))

solSpencer = calcSol(lat, BTd[100], method = 'spencer')
print(as.zooD(solSpencer))

solCooper = calcSol(lat, BTd[100], method = 'cooper')
print(as.zooD(solCooper))


[Package solaR version 0.46 Index]