# Cube Maths#

The section Navigating a Cube highlighted that every cube has a data attribute; this attribute can then be manipulated directly:

```
cube.data -= 273.15
```

The problem with manipulating the data directly is that other metadata may become inconsistent; in this case the units of the cube are no longer what was intended. This example could be rectified by changing the units attribute:

```
cube.units = 'celsius'
```

Note

`iris.cube.Cube.convert_units()`

can be used to automatically convert a
cube’s data and update its units attribute.
So, the two steps above can be achieved by:

```
cube.convert_units('celsius')
```

In order to reduce the amount of metadata which becomes inconsistent, fundamental arithmetic operations such as addition, subtraction, division and multiplication can be applied directly to any cube.

## Calculating the Difference Between Two Cubes#

Let’s load some air temperature which runs from 1860 to 2100:

```
filename = iris.sample_data_path('E1_north_america.nc')
air_temp = iris.load_cube(filename, 'air_temperature')
```

We can now get the first and last time slices using indexing (see Cube Indexing for a reminder):

```
t_first = air_temp[0, :, :]
t_last = air_temp[-1, :, :]
```

And finally we can subtract the two. The result is a cube of the same size as the original two time slices, but with the data representing their difference:

```
>>> print(t_last - t_first)
unknown / (K) (latitude: 37; longitude: 49)
Dimension coordinates:
latitude x -
longitude - x
Scalar coordinates:
forecast_reference_time 1859-09-01 06:00:00
height 1.5 m
Attributes:
Conventions 'CF-1.5'
Model scenario 'E1'
source 'Data from Met Office Unified Model 6.05'
```

Note

Notice that the coordinates “time” and “forecast_period” have been removed from the resultant cube; this is because these coordinates differed between the two input cubes.

## Calculating a Cube Anomaly#

In section Cube Statistics we discussed how the dimensionality of a cube
can be reduced using the `Cube.collapsed`

method
to calculate a statistic over a dimension.

Let’s use that method to calculate a mean of our air temperature time-series, which we’ll then use to calculate a time mean anomaly and highlight the powerful benefits of cube broadcasting.

First, let’s remind ourselves of the shape of our air temperature time-series cube:

```
>>> print(air_temp.summary(True))
air_temperature / (K) (time: 240; latitude: 37; longitude: 49)
```

Now, we’ll calculate the time-series mean using the
`Cube.collapsed`

method:

```
>>> air_temp_mean = air_temp.collapsed('time', iris.analysis.MEAN)
>>> print(air_temp_mean.summary(True))
air_temperature / (K) (latitude: 37; longitude: 49)
```

As expected the *time* dimension has been collapsed, reducing the
dimensionality of the resultant *air_temp_mean* cube. This time-series mean can
now be used to calculate the time mean anomaly against the original
time-series:

```
>>> anomaly = air_temp - air_temp_mean
>>> print(anomaly.summary(True))
unknown / (K) (time: 240; latitude: 37; longitude: 49)
```

Notice that the calculation of the *anomaly* involves subtracting a
*2d* cube from a *3d* cube to yield a *3d* result. This is only possible
because cube broadcasting is performed during cube arithmetic operations.

Cube broadcasting follows similar broadcasting rules as NumPy, but the additional richness of Iris coordinate meta-data provides an enhanced capability beyond the basic broadcasting behaviour of NumPy.

As the coordinate meta-data of a cube uniquely describes each dimension, it is possible to leverage this knowledge to identify the similar dimensions involved in a cube arithmetic operation. This essentially means that we are no longer restricted to performing arithmetic on cubes with identical shapes.

This extended broadcasting behaviour is highlighted in the following examples. The first of these shows that it is possible to involve the transpose of the air temperature time-series in an arithmetic operation with itself.

Let’s first create the transpose of the air temperature time-series:

```
>>> air_temp_T = air_temp.copy()
>>> air_temp_T.transpose()
>>> print(air_temp_T.summary(True))
air_temperature / (K) (longitude: 49; latitude: 37; time: 240)
```

Now add the transpose to the original time-series:

```
>>> result = air_temp + air_temp_T
>>> print(result.summary(True))
unknown / (K) (time: 240; latitude: 37; longitude: 49)
```

Notice that the *result* is the same dimensionality and shape as *air_temp*.
Let’s check that the arithmetic operation has calculated a result that
we would intuitively expect:

```
>>> result == 2 * air_temp
True
```

Let’s extend this example slightly, by taking a slice from the middle
*latitude* dimension of the transpose cube:

```
>>> air_temp_T_slice = air_temp_T[:, 0, :]
>>> print(air_temp_T_slice.summary(True))
air_temperature / (K) (longitude: 49; time: 240)
```

Compared to our original time-series, the *air_temp_T_slice* cube has one
less dimension *and* its shape is different. However, this doesn’t prevent
us from performing cube arithmetic with it, thanks to the extended cube
broadcasting behaviour:

```
>>> result = air_temp - air_temp_T_slice
>>> print(result.summary(True))
unknown / (K) (time: 240; latitude: 37; longitude: 49)
```

## Combining Multiple Phenomena to Form a New One#

Combining cubes of potential-temperature and pressure we can calculate the associated temperature using the equation:

Where \(p\) is pressure, \(\theta\) is potential temperature, \(p_0\) is the potential temperature reference pressure and \(T\) is temperature.

First, let’s load pressure and potential temperature cubes:

```
filename = iris.sample_data_path('colpex.pp')
phenomenon_names = ['air_potential_temperature', 'air_pressure']
pot_temperature, pressure = iris.load_cubes(filename, phenomenon_names)
```

In order to calculate \(\frac{p}{p_0}\) we can define a coordinate which represents the standard reference pressure of 1000 hPa:

```
import iris.coords
p0 = iris.coords.AuxCoord(1000.0,
long_name='reference_pressure',
units='hPa')
```

We must ensure that the units of `pressure`

and `p0`

are the same,
so convert the newly created coordinate using
the `iris.coords.Coord.convert_units()`

method:

```
p0.convert_units(pressure.units)
```

Now we can combine all of this information to calculate the air temperature using the equation above:

```
temperature = pot_temperature * ( (pressure / p0) ** (287.05 / 1005) )
```

Finally, the cube we have created needs to be given a suitable name:

```
temperature.rename('air_temperature')
```

The result could now be plotted using the guidance provided in the Plotting a Cube section.

A very similar example to this can be found in Deriving Exner Pressure and Air Temperature.

## Combining Units#

It should be noted that when combining cubes by multiplication, division or
power operations, the resulting cube will have a unit which is an appropriate
combination of the constituent units. In the above example, since `pressure`

and `p0`

have the same unit, then `pressure / p0`

has a dimensionless
unit of `'1'`

. Since `(pressure / p0)`

has a unit of `'1'`

, this does
not change under power operations and so
`( (pressure / p0) ** (287.05 / 1005) )`

also has unit `1`

. Multiplying
by a cube with unit `'1'`

will preserve units, so the cube `temperature`

will be given the same units as are in `pot_temperature`

. It should be
noted that some combinations of units, particularly those involving power
operations, will not result in a valid unit and will cause the calculation
to fail. For example, if a cube `a`

had units `'m'`

then `a ** 0.5`

would result in an error since the square root of a meter has no meaningful
unit (if `a`

had units `'m2'`

then `a ** 0.5`

would result in a cube
with units `'m'`

).

Iris inherits units from cf_units
which in turn inherits from UDUNITS.
As well as the units UDUNITS provides, cf units also provides the units
`'no-unit'`

and `'unknown'`

. A unit of `'no-unit'`

means that the
associated data is not suitable for describing with a unit, cf units
considers `'no-unit'`

unsuitable for combining and therefore any
arithmetic done on a cube with `'no-unit'`

will fail. A unit of
`'unknown'`

means that the unit describing the associated data
cannot be determined. cf units and Iris will allow arithmetic on cubes
with a unit of `'unknown'`

, but the resulting cube will always have
a unit of `'unknown'`

. If a calculation is prevented because it would
result in inappropriate units, it may be forced by setting the units of
the original cubes to be `'unknown'`

.