diff --git a/docs/index.rst b/docs/index.rst
index 203d426..1d6bf80 100644
--- a/docs/index.rst
+++ b/docs/index.rst
@@ -28,6 +28,123 @@ API Reference
     iris
 
 
+Examples
+========
+
+Load an IRIS spectrograph raster sequence,
+and display as a false-color movie.
+
+.. jupyter-execute::
+
+    import IPython.display
+    import dataclasses
+    import numpy as np
+    import matplotlib.pyplot as plt
+    import astropy.units as u
+    import astropy.time
+    import astropy.visualization
+    import named_arrays as na
+    import iris
+
+    # Download a 320-step raster sequence
+    obs = iris.SpectrographObservation.from_time_range(
+        time_start=astropy.time.Time("2021-09-23T02:00"),
+        time_stop=astropy.time.Time("2021-09-23T03:00"),
+    )
+
+    # Crop the observation so readthedocs doesn't run out of memory.
+    # This is probably unnecessary on your machine
+    index = {obs.axis_wavelength: slice(75, 150)}
+    obs = dataclasses.replace(
+        obs,
+        inputs=na.TemporalSpectralPositionalVectorArray(
+            time=obs.inputs.time,
+            wavelength=obs.inputs.wavelength[index],
+            position=obs.inputs.position[index],
+        ),
+        outputs=obs.outputs[index],
+    )
+
+
+    # Calculate the mean rest wavelength of the
+    # brightest spectral line
+    wavelength_center = obs.wavelength_center.ndarray.mean()
+
+    # Define a tuple of the temporal and spatial axes
+    axis_txy = (obs.axis_time, obs.axis_detector_x, obs.axis_detector_y)
+
+    # Take the mean of the wavelength over the spatial
+    # and temporal axes since it is constant
+    wavelength = obs.inputs.wavelength.mean(axis_txy)
+
+    # Convert to Doppler velocity
+    velocity = wavelength.to(
+        unit=u.km / u.s,
+        equivalencies=u.doppler_optical(wavelength_center),
+    )
+
+    # Define velocity bounds
+    velocity_min = -100 * u.km / u.s
+    velocity_max = +100 * u.km / u.s
+
+    # Define the spectral normalization curve
+    spd_max = np.percentile(
+        a=obs.outputs,
+        q=99.5,
+        axis=axis_txy,
+    )
+
+    # Convert the spectral radiance to
+    # red/green/blue channels
+    rgb, colorbar = na.colorsynth.rgb_and_colorbar(
+        spd=obs.outputs,
+        wavelength=velocity,
+        axis=obs.axis_wavelength,
+        spd_min=0 * u.DN,
+        spd_max=spd_max,
+        wavelength_min=velocity_min,
+        wavelength_max=velocity_max,
+    )
+
+    # Isolate the angular position of each RGB point
+    position = obs.inputs.position.mean(obs.axis_wavelength)
+
+    # Display the result as an RGB movie
+    with astropy.visualization.quantity_support():
+        fig, ax = plt.subplots(
+            ncols=2,
+            figsize=(6, 6),
+            gridspec_kw=dict(width_ratios=[.9, .1]),
+            constrained_layout=True,
+        )
+        ani = na.plt.pcolormovie(
+            obs.inputs.time,
+            position.x,
+            position.y,
+            C=rgb,
+            axis_time=obs.axis_time,
+            axis_rgb=obs.axis_wavelength,
+            ax=ax[0],
+            kwargs_animation=dict(
+                interval=500,
+            )
+        )
+        na.plt.pcolormesh(
+            C=colorbar,
+            axis_rgb=obs.axis_wavelength,
+            ax=ax[1],
+        )
+        ax[0].set_aspect("equal")
+        ax[0].set_xlabel(f"helioprojective $x$ ({ax[0].get_xlabel()})")
+        ax[0].set_ylabel(f"helioprojective $y$ ({ax[0].get_ylabel()})")
+        ax[1].yaxis.tick_right()
+        ax[1].yaxis.set_label_position("right")
+        ax[1].set_ylim(velocity_min, velocity_max)
+
+    plt.close(fig)
+    IPython.display.HTML(ani.to_jshtml())
+
+
 Indices and tables
 ==================
 
diff --git a/iris/data.py b/iris/data.py
index ad93a8b..964abcf 100644
--- a/iris/data.py
+++ b/iris/data.py
@@ -229,7 +229,7 @@ def download(
         file = directory / url.name
 
         if overwrite or not file.exists():
-            r = requests.get(url)
+            r = requests.get(url, stream=True)
             with open(file, "wb") as f:
                 f.write(r.content)
 
diff --git a/pyproject.toml b/pyproject.toml
index f6355a8..e119d38 100644
--- a/pyproject.toml
+++ b/pyproject.toml
@@ -17,7 +17,7 @@ dependencies = [
     "astropy",
     "requests",
     "urlpath",
-    "named-arrays==0.7.1",
+    "named-arrays==0.8",
 ]
 dynamic = ["version"]