2014
DOI: 10.1016/j.nima.2014.08.009
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Study of the inter-strip gap effects on the response of Double Sided Silicon Strip Detectors using proton micro-beams

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Cited by 21 publications
(9 citation statements)
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“…The front coincidence plot is characterized by the presence of negative signals, which have been already observed in previous works [1,2]. As it is discussed in details in [5,6], this type of response is due to an accumulation of charge in the insulating layer of SiO 2 producing an inverted electric field which modify charge collection for inter-strip events. In this case the inter-strip region is not a simple straight line joining the FEPs.…”
Section: Dsssd Efficiency For Full Energy Detectionsupporting
confidence: 54%
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“…The front coincidence plot is characterized by the presence of negative signals, which have been already observed in previous works [1,2]. As it is discussed in details in [5,6], this type of response is due to an accumulation of charge in the insulating layer of SiO 2 producing an inverted electric field which modify charge collection for inter-strip events. In this case the inter-strip region is not a simple straight line joining the FEPs.…”
Section: Dsssd Efficiency For Full Energy Detectionsupporting
confidence: 54%
“…Results confirmed that both front and back effective inter-strip widths, which are related to the efficacy for full energy detection, can be much larger than the nominal geometric width of the SiO 2 zone and depend on the operating conditions. All the experimental observations were qualitatively described by simulations based on the Shockley-Ramo-Gunn framework [6]. Therefore, for those experiments aiming at accurately measuring absolute cross-sections , especially if two or more DSSSD are used in coincidence, efficiency for full energy detection cannot be deduced from the geometric inter-strip width but a complete characterization of the used DSSSDs is necessary.…”
Section: Discussionmentioning
confidence: 99%
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“…Due to the large size of all detectors (50×50 mm 2 ) and their fine segmentation, telescopes covered rather large solid angle with good angular resolution. This same segmentation makes the analysis of obtained experimental data rather demanding -complications associated with dead layers [18] or interstrip gaps [19,20] are only part of the problem, the very basic one being a calibration of a large number of apparently independent detector channels. Several novel calibration improvements described in detail in ref.…”
Section: Introductionmentioning
confidence: 99%
“…Each strip is 3 mm wide and they are separated by a SiO 2 layer 1 μm wide that in the following is called interstrip. it is known that that particles entering the detector through the SiO 2 insulating interstrip region, can produce signals with an amplitude which is different than the full energy and also signals with an opposite polarity [1][2][3][4][5][6]. For this reason it is very important to be able to reject interstrip events by selecting only the events producing the correct full energy signals.…”
Section: Introductionmentioning
confidence: 99%