Difference between revisions 2373220 and 2373246 on enwikiversity[[Image:Detectors summary 3.png|thumb|right|250px|This tree diagram shows the relationship between types and classification of most common particle detectors. Credit: [[commons:User:Wdcf|Wdcf]].]] '''Radiation detectors''' provide a signal that is converted to an electric current. The device is designed so that the current provided is proportional to the characteristics of the incident radiation. (contracted; show full) Similar to the way that a terrestrial gyrocompass uses a pendulum to sense local gravity and force its gyro into alignment with earth's spin vector, and therefore point north, an ''orbital gyrocompass'' uses a horizon sensor to sense the direction to earth's center, and a gyro to sense rotation about an axis normal to the orbit plane. Thus, the horizon sensor provides pitch and roll measurements, and the gyro provides yaw. See Tait-Bryan angles. ==Detector materials== ==Gadolinium oxysulfide is a promising luminescent host material, because of its high density (7.32 g/cm<sup>3</sup>) and high effective atomic number of Gd. These characteristics lead to a high stopping power for X-ray radiation.s== Gadolinium oxysulfide ({{chem|Gd|2|O|2|S}}: Pr, Ce, F powder complex) based ceramics exhibit final densities of 99.7% to 99.99% of the theoretical density (7.32 g/cm<sup>3</sup>) and an average grain size ranging from 5 micrometers to 50 micrometers in dependence with the fabrication procedure.<ref>Rossner, W., M. Ostertag, and F. Jermann. "Properties and Applications of Gadolinium Oxysulfide Based Ceramic Scintillators." Electrochemical Society Prceeedings, 98, 187-94.</ref> There are two main disadvantages to this scintillator; one being the hexagonal crystal structure, which emits only optical translucency and low external light collection at the photodiode and the other is the high X-ray damage to the sample.<ref name= Greskovich >{{cite journal|doi=10.1146/annurev.matsci.27.1.69|title=Ceramic Scintillators|date=1997|last1=Greskovich|first1=C.|last2=Duclos|first2=S.|journal=Annual Review of Materials Science|volume=27|pages=69–88|bibcode=1997AnRMS..27...69G }}</ref> The {{chem|Gd|2|O|2|S}} structure is a sulfur layer with double layers of gadolinium and oxygen in between.<ref name=Rossner>Rossner, W., M. Ostertag, and F. Jermann. "Properties and Applications of Gadolinium Oxysulfide Based Ceramic Scintillators." Electrochemical Society Prceeedings, 98, 187-94.</ref> Terbium-activated gadolinium oxysulfide is frequently used as a scintillator for x-ray imaging that emits wavelengths between 382-622 nm, though the primary emission peak is at 545 nm and is used as a green phosphor in projection cathode ray tubes, though its drawback is marked lowering of efficiency at higher temperatures.<ref>[http://www.freepatentsonline.com/5115306.html]</ref> When Gadolinium oxysulfide comes in contact with mineral acids, hydrogen sulfide can be produced.<ref>Gadolinium Oxysulfide; MSDS [online]; R.H. Mangels: Hackettstown, NJ, March 15, 1997. http://www.nonius.nl/manualspdf/msdsGadolinumOxysulfide.pdf (accessed October 17, 2011)</ref> ==Cadmium tellurides== Cadmium telluride (CdTe) doped with chlorine is used as a radiation detector for [X-rays], gamma rays, beta particles and alpha particles. CdTe can operate at room temperature allowing the construction of compact detectors for a wide variety of applications in nuclear spectroscopy.<ref name="Capper">{{cite book |title= Properties of Narrow-Gap Cadmium-Based Compounds | author = P. Capper | publisher = INSPEC, IEE | location= London, UK | date = 1994 | {{isbn=|0-85296-880-9}} }}</ref> The properties that make CdTe superior for the realization of high performance gamma- and x-ray detectors are high atomic number, large bandgap and high electron mobility ~1100 cm<sup>2</sup>/V·s, which result in high intrinsic μτ (mobility-lifetime) product and therefore high degree of charge collection and excellent spectral resolution. ==Entities== {{main|Radiation astronomy/Entities}} (contracted; show full)<!-- footer templates --> {{tlx|Radiation astronomy resources}}{{Principles of radiation astronomy}}{{Sisterlinks|Radiation detectors}} <!-- categories --> [[Category:Materials sciences/Lectures]] [[Category:Physics/Lectures]] [[Category:Radiation astronomy/Lectures]] [[Category:Technology/Lectures]] All content in the above text box is licensed under the Creative Commons Attribution-ShareAlike license Version 4 and was originally sourced from https://en.wikiversity.org/w/index.php?diff=prev&oldid=2373246.
![]() ![]() This site is not affiliated with or endorsed in any way by the Wikimedia Foundation or any of its affiliates. In fact, we fucking despise them.
|