Injongo kukuba ii-sensors ziya kuphucula ukuqonda kwesayensi ngamandla e-atmosfera kunye nokuqhubela phambili kwimodeli yemozulu, uqikelelo lwemozulu kunye nokuqikelelwa kwe-satellite orbit.
Inkampani iyasebenzisana ne-STFC RALSpace kunye neDyunivesithi yaseBirmingham.
UTeledyne e2v ubhala athi:
Umoya ophezulu womhlaba ngummandla osebenzayo kakhulu odlala indima ebalulekileyo ekudlulisweni kwamandla eplanethi, echaphazela imozulu kunye nemozulu. Ukuqonda amandla e-atmosfera ephezulu yoMhlaba kuya kuxhomekeka kumlinganiso ocekeceke kakhulu wemikhosi esebenza kwisathelayithi eyilwe ngokukodwa njengoko idlula kumoya onqabileyo we-Orbit Earth Earth.
Ii-accelerometer ezintsha zisekwe kwindawo yetekhnoloji ye-quantum esebenzisa iiathom zealkali, ezipholileyo ngeelaser kufutshane ne-zero ngokupheleleyo, ngaphandle kokusebenzisa i-cryogenics.
Le projekthi iza kwakhela kwi-Teledyne e2v's yangaphambili yomsebenzi wokwakha i-CASPA CubeSat, ebonise ukubanjiswa kwe-athomu ebandayo kwaye imele inyathelo lokusebenzisa ii-atom ezibandayo kwizicelo zesithuba.
Isindululo sikaTeledyne e2v sesixhobo esisekwe esikhaleni sikhethwe kukhuphiswano oluvulekileyo lweTekhnoloji yeTekhnoloji yoNyaka ye-13 (Earth), eqhutywa liziko leZiko lokuJongwa koMhlaba (i-CEOI), eyindibaniselwano yeAirbus Ltd, QinetiQ Ltd, STFC Rutherford I-Appleton Laboratory kunye neYunivesithi yaseLeicester.
Unokufunda ngakumbi malunga neNkqubo yeTekhnoloji yeSizwe ye-Quantum ye-UK apha.
Umfanekiso: Teledyne e2v Umboniso weCASPA
