Sir, we've arrived at the coordinates we calculated.

Everyone rendezvous at the standby coordinates.

Set Coordinate

Coordinates are locked.

The desired x position in pixels

The desired y position in pixels

Set Polar Coordinate System

Select Zoom Area

Set Euclidean Coordinate System

Set those new coordinates R2?

I initialized the robot my robot using the function robot.

Indicated here.

locations in our images, so that's pixel one location and pixel two location, and let's plot this car, you know, at the

Coordinates locked in.

Once again, this is in three dimensions, so you have to specify three coordinates.

In addition to the commonly used equatorial or ecliptic or galactic coordinates from astronomy, we now define so called supergalactic coordinates.

Plot them on a graph.

Coordinate

Coordinates

Copy coordinates

Paste coordinates

Edit Coordinates...

Remove Coordinates...

You remember a robot operating in a plane environment has usually 3 coordinates.

The camera now takes a 2 dimensional image which is 2 more dimensions. This camera keep the x and y and z positions fixed, and varies the remaining two variables.

Any drawlmage functions will follow this coordinate system and place the top left hand corner of the image at the location specified by the drawlmage call.

Then I just model a straight motion.

Polar Coordinates

X Coordinate

Y Coordinate

Coordinate System

X coordinate

Y coordinate

Coordinate Grid

Coord. grid

Catalog Coordinates

Cartesian

Cartesian Coordinates

Coordinate grid

Do you have everything?

We have progressed from a zero dimensional point, to a one dimensional line segment, to a two dimensional triangle.

Locked and floating. You can drop us any time now.

So I'll just write a is at the coordinate.

We find that along the main diagonal our uncertainty has shrunk substantially.

I think you're getting the hang of this.