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GeolOil  Logging Scripting (GLS) Reference Manual and API Documentation
The GeolOil GLS is a simple and concise scripting programming language specifically designed to process petrophysics LAS files. It allows easy handling of well log curves without worrying too much about invalid blank, or missed 999.25 values. Some minimum exposure to elementary scripting is advised. Please read the GLS log scripting tutorial introduction before checking this reference material.
GLS Stream Operators
The operators +, , *, /, are normal binary operators that can take either a scalar or a log curve to the left or right side of the operator. The power operator is ^. For instance, x^y means x^{y}. Operators are evaluated from left to right according to standard operator precedence priority as any programming language. To change the evaluation order, just use enough parentheses.
The character or sigil @ is reserved for curve number references. For example, if deep resistivity is the curve number 13, the assignation Rt = @13 defines the variable Rt as a whole curve object. Measured depth should normally be the first curve on a LAS file, so MD = @1 defines MD as the curve 1. To separate instructions use ;. To start a remark or a comment to be omited use #.
The internal representation for missed, dummy, unknown, blank, invalid, infinite, not a number, or any irregular number is 999.25. GeolOil GLS handles all cases automatically in the stream mode (it compiles and executes for you all necessary depth loops on curves and if conditions), but some manual control is needed on the regular looping mode when using comparisons like ==, <, ≤, >, and ≥.
GLS Stream Functions
A stream function is automatically applied to a whole log curve. It internally takes care of all depth cells, looping, and properly handling of invalid dummy and 999.25 values. A special algebra handles automatically a whole curve without any need to loop inside individual depth values. All functions can be applied to either scalars (a single value), or log curve arguments:
 abs(x) Returns the absolute value or argument x
 exp(x) Returns e^{x}
 ln(x) Returns the natural logarithm (base e=2.71828...) of x
 log10(x) Returns the common logarithm (base 10) of x
 sin(x) Returns the sine of x, where x is in radians, not degrees.
 cos(x) Returns the cosine of x, where x is in radians.
 tan(x) Returns the tangent of x, where x is in radians.
 asin(x) Returns the inverse function sin^{1}(x). The returned result is in radians, not degrees.
 acos(x) Returns the inverse function cos^{1}(x). The returned result is in radians.
 atan(x) Returns the inverse function tan^{1}(x). The returned result is in radians.
 ind(x,y) Returns 1 if x < y. Returns 0 if x ≥ y. Returns 999.25 if either x or y are invalids or 999.25
 ind(x,y,z) Returns 1 if (x ≤ y) and (y < z). Returns 0 if condition is false. Returns 999.25 for invalid arguments
 blank(x,y) Returns 999.25 if x < y. Returns 1 if x ≥ y. Also returns 1 if either x or y are invalids or 999.25
 blank(x,y,z) Returns 999.25 if (x ≤ y) and (y < z). Returns 1 if condition is false. Also returns 1 for invalid args
 blankOutside(x,y,z) Returns 999.25 if y lies outside the interval: x ≤ y < z. Returns 1 if y lies in the interval, and also 1 for invalid arguments
 isValid(x) Returns 1 if x is a valid argument, 0 if x is invalid, blank, or missed like 999.25, NaN, infinite, etc.
 valueOrZero(x) Returns its original argument x, if x is valid. But returns 0 if x is invalid
 trim(left,x,right) Returns x, if left ≤ x < right. Returns left, if x < left. Returns right if x > right. Returns 999.25 for invalid arguments
 shiftCurve(x,n) Vertically shifts the curve x downwards n depth steps if n > 0, (producing a deeper curve), or upwards n depth steps if n < 0: It returns a new shifted curve
 shiftLeft (x,cutoff,replacement) Horizontally shifts the curve x: where (x < cutoff) set (x = replacement). It returns a new different curve
 shiftRight(x,cutoff,replacement) Horizontally shifts the curve x: where (x > cutoff) set (x = replacement). It returns a new different curve
 min(x,y) Returns the smaller of x and y, or 999.25 if either x or y are unknown, missed, invalid or 999.25.
 min(x1,x2,x3,...,xn) Returns the smallest of x_{1}, x_{2}, x_{3}, ..., x_{n}. Returns 999.25 if an argument is invalid, missed, or 999.25.
 max(x,y) Returns the larger of x and y, or 999.25 if either x or y are unknown, missed, invalid or 999.25.
 max(x1,x2,x3,...,xn) Returns the largest of x_{1}, x_{2}, x_{3}, ..., x_{n}. Returns 999.25 if an argument is invalid, missed, or 999.25.
 merge(x,y) Returns x, if x is known. Returns y, if x is missed, invalid, unknown or 999.25 (transparency): merge puts the x curve on top of y
 merge(x1,x2,x3,...,xn) Returns a new merged curve from x_{1}, x_{2}, x_{3}, ..., x_{n}. Top priority curve is x_{1}. If x_{1} is missed, x_{2} is taken and so on
 avg(x,y) Returns the arithmetic average of x and y. Any 999.25 missed value is skipped. Only returns 999.25 if both x and y are missed.
 avg(x1,x2,x3,...,xn) Returns the average of x_{1}, x_{2}, x_{3}, ..., x_{n}. Any missed value is skipped. Only returns 999.25 if all values are missed.
Three exponential and logarithmic functions:
Six trigonometric functions:
The next five functions are normally used as premultipliers to modify results: (See an example in the tutorial log scripting)
Special functions:
The merge() and avg() functions combine several curves into one. Let's suppose that a LAS file has two versions of Gamma Ray curves and it is wanted to combine them into a single one (instead of selecting one). If the curve GR1 is more reliable than the curve GR2, we would like to use the curve GR1 when it is available, and use GR2 only when GR1 is missed (999.25). If both curves have a similar behaviour and reliability, perhaps it would be preferred to average the curves to reduce noise, and yet produce an estimate even if only one curve is available:
User Defined Stream Functions
In some cases the builtin collection of GLS functions is not enough for some advanced computations. Custom specific functions can be defined by the user both in stream mode or regular depth looping mode. The defined functions are usually placed at the end of the script. As an example, the following user defined stream function has the same behaviour as the default builtin GLS avg(x,y) function:
GLS Regular Depth Looping Mode
The GLS stream mode normally handles most of the programmer's needs. However, in some cases an advanced user may want full control of the computations depth by depth step on a curve. Such custom scripts are usually unnecessarily verbose, long, complex, and prone to bugs, as the user has to take care of all cases, exceptions, if conditions, and looping.
While algebra with invalid numbers like NaN or 999.25 is handled correctly by GLS, the user must not use if and comparison operators like <, ≤, ==, ≥, or >. The reason for that is that an unknown number like NaN or 999.25 can't be compared against anything by definition. For instance, what is the logic result of the instructions: x=999.25; if (x<0) {x=x+1;}. Since 999.25 is a missed invalid number, don't expect the result to be true (yielding x=998.25). Likewise, the if() comparison should not be taken as false either!. How to treat this then?
There are two workarounds to deal with this problem. The first choice is prefer to script as much as possible in the GLS stream mode that takes those details correctly and automatically for you. The second choice is to explictly skip all invalid comparisons and continue to the next instruction or iteration in a depth loop using the isValid(x) function, or its logic negation !isValid(x)
Looping over all Depths
To build a loop over all depths in a LAS file, the user needs to take care of the followng details:

Define new void curves initialized to blank missed values (999.25) that can store computation results. Once any
curve is already defined, a new curve with 999.25 cell depths is easily assigned using the .blank()
instance method on the LasCurve. For instance:
MD = @1; workingResult = new LasCurve (MD.blank());  Find the LasCurve size. Which is the amount of elements or depths in the curve, for example: nDepths = MD.size();

Get for each LasCurve to be read, its scalar individual value at the target depth index. This is done with
the LasCurve instance method .get(i). For instance:

Continue to the next loop iteration if you plan to use comparators <, ≤, ==, ≥, or >, on variables
that might have missed 999.25 values which would behave unexpectedly during comparisons. Just use logical or on
negated !isValid() functions to skip those possibilities. (If any value is invalid, skip and continue to the next iteration)
For instance:
 Set the collected values of swValue in their corresponding whole SW LasCurve positions using the instance method .set (index, value):
All this large boilerplate code is equivalent (and safer, more intuitive and human readable) to just only three lines of scripting in the Stream Mode. So think twice before considering to write code on the Regular Looping Mode, or other petrophysical software under Python scripts. What about trying in Excel?
Notice that the former script last line does not end with the command return(SW). An explicit return() command is optional. If the script does not find a return() command, the value of the last expression evaluated is returned, in this case SW. This makes the script more concise.
Only if you really need to write complicated math code that involves the flow control statements: if, else, for, do, while, continue, and break, stick with the Stream Mode.
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