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SEIX 17-20 octobre 2005 - Atelier Calcium

SEIX 17-20 octobre 2005 - Atelier Calcium

SEIX 17-20 octobre 2005 - Atelier Calcium

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UNE NOUVELLE CAMÉRA PAR HAMAMATSU : ELECTRON MULTIPLYING<br />

CCD C9100 HIGH SPEED WITH LOW LIGHT LEVELS<br />

Bruno Combettes<br />

Hamamatsu Photonics France rue du saule trapu, parc du moulin de Massy, BP 229 91882<br />

MASSY Cedex<br />

• Sensor is designed based on the frame transfer back thinned CCD technology.<br />

• Multiplication register is added on the serial register.<br />

• In the multiplication register, up to 50 volts is applied to the one of charge transfer<br />

gate (GS) in order to get the multiplication gain.<br />

• Electrical field under the transfer gate (GS) accelerates the signal electron and<br />

energetic collision occurs in the silicon matrix.<br />

• Such collision will result in an occasional extra electron in the transferred charge.<br />

• This is called IMPACT IONIZATION<br />

• Every stage in the multiplication register has a statistical chance of 1.0% to 1.6% of<br />

creating an impact ionization event.<br />

• When multiplied by 500 steps ,for example, this generates several thousand times<br />

“gain”.<br />

• Mathematically gain is given by G=(1+g)N<br />

– where N is the stage number in the multiplication register and g is the<br />

probability of generating a secondary electron.<br />

– For example, N is 500 and g is 1.5%(0.015), then G is <strong>17</strong>10.<br />

• The normal read noise of a camera becomes “relatively” very small compared to this.<br />

• High speed readout at low intensity with low “relative read noise” is the main<br />

advantage of this technology.<br />

• Advantage<br />

– Readout noise is constant and fixed.<br />

– Gain is controllable.<br />

– When signal is gained up bigger than Readout noise, then it relatively readout<br />

noise becomes less than 1 electron.<br />

Cooling is the most important technology for EM-CCD.<br />

• Why?<br />

– Dark current is the part of signal.<br />

– At high gain, dark current becomes a main source of back ground noise.<br />

– EM Gain is the function of temperature. Need -50 degree C cooling to get<br />

<strong>20</strong>00 times gain.<br />

– Sensor gain is strongly affected by the sensor temperature and it must be very<br />

stable against ambient temperature movement.<br />

– Only very stable sensor temperature realizes the quantitative measurement.<br />

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