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Experiments to Control Atom Number and Phase-Space Density in ...

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The second card (NI6733) offers eight digital <strong>in</strong>/out <strong>and</strong> two 24 bit counters. This<br />

card will be used for acquir<strong>in</strong>g s<strong>in</strong>gle a<strong>to</strong>m detection data. For each detected pho<strong>to</strong>n<br />

the avalanche pho<strong>to</strong>diode (APD) generates a pulse. These pulses can then be counted<br />

with the help of this card.<br />

The last card (NI PCI-GPIB) is able <strong>to</strong> control GPIB-cabale devices <strong>and</strong> is used<br />

<strong>to</strong> <strong>in</strong>terface with GPIB devices. Thus far it was ma<strong>in</strong>ly used <strong>to</strong> communicate with an<br />

arbitrary function genera<strong>to</strong>r (Agilent 33250A).<br />

A second PC runs a program called Apogee Server. This program controls the<br />

two cameras <strong>in</strong> the experimental setup: The USB camera Apogee Alta U47+ <strong>and</strong> the<br />

FireWire camera St<strong>in</strong>gray F033B/C from Allied Vision Technologies. A third computer,<br />

runn<strong>in</strong>g the software Vision, also written by Florian Schreck, communicates both with<br />

<strong>Control</strong> <strong>and</strong> Apogee Server. If a picture is <strong>to</strong> be taken dur<strong>in</strong>g the experimental sequence,<br />

<strong>Control</strong> sends this <strong>in</strong>formation <strong>to</strong> Vision, which <strong>in</strong> turn tells Apogee Server <strong>to</strong> prepare<br />

the camera. <strong>Control</strong> then triggers the camera <strong>and</strong> Apogee Server downloads the picture<br />

<strong>in</strong>formation from the camera <strong>and</strong> sends the data <strong>to</strong> Vision.<br />

The ma<strong>in</strong> purpose of Vision is data evaluation. Depend<strong>in</strong>g on the type of image<br />

taken, Vision au<strong>to</strong>matically displays the fluorescence image, or uses the raw absorption,<br />

the probe, <strong>and</strong> the noise image of absorption imag<strong>in</strong>g <strong>to</strong> calculate the optical density.<br />

It also fits the data <strong>to</strong> determ<strong>in</strong>e a<strong>to</strong>m number, the spatial extent of the cloud, etc.<br />

Vision au<strong>to</strong>matically s<strong>to</strong>res all the images <strong>and</strong> all the variables with values used <strong>in</strong><br />

the experimental sequence. This allows a complete reconstruction of the experimental<br />

sequence at any time.<br />

7.5 Imag<strong>in</strong>g<br />

Imag<strong>in</strong>g of lithium a<strong>to</strong>ms us<strong>in</strong>g absorption imag<strong>in</strong>g techniques is more compli-<br />

cated than for rubidium, due <strong>to</strong> the differences <strong>in</strong> energy level structure. Corrections<br />

<strong>to</strong> the simple formulas given before are therefore required. In addition it can be very<br />

helpful <strong>to</strong> image the a<strong>to</strong>ms at a homogeneous magnetic field, <strong>and</strong> the presence of the<br />

field has <strong>to</strong> be taken <strong>in</strong><strong>to</strong> account dur<strong>in</strong>g the imag<strong>in</strong>g process.<br />

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