Imitha Yokugrumba Amanzi Engaphantsi Komhlaba yeCGL-200

Imitha yamanzi yerula yentsimbi ye-CGL-200 sisixhobo sokulinganisa esichanekileyo kakhulu esenzelwe ngokukodwa ukujonga umgangatho wamanzi ekubholeni phantsi komhlaba. Ngoluhlu lokulinganisa lwe-0-1000M, inokubamba ngokuchanekileyo utshintsho emanzini angaphantsi komhlaba anzulu kwaye ivumelane neendawo ezahlukeneyo zokubhola ezintsonkothileyo. Ngokusekelwe kulawulo lombane lomgaqo wokusebenza kwamanzi, xa iprobe yentsimbi engagqwaliyo idibana nomphezulu wamanzi, unxibelelwano lokumelana namanzi luvala isekethe, kwaye inkqubo yokwamkela ngoko nangoko ivuselela i-alamu evakalayo kunye nokukhanya kwesalathisi se-LED. Kwangaxeshanye, ubunzulu bomgangatho wamanzi bunokufunyanwa ngokufunda isikali kwirula yentsimbi, ngexesha lokuphendula le-≤1 ms kunye nokuchaneka kokulinganisa kwe-±0.5 mm. Esi sixhobo sinoyilo olusebenziseka lula, olunika iindlela ezimbini zezinto zereyile—i-ABS kunye nediski yentsimbi. Izinto ze-ABS zilula kwaye azinamhlwa, zifanelekile ukuhlolwa rhoqo kokubhola; izinto zediski yentsimbi zinamandla aphezulu, okwenza ukuba zilungele ukujonga ixesha elide phantsi kweemeko zokusebenza ezinzima.