1. Ukunqunywa ngesikhathi esisodwa kwe-Ag, Sn, B, Mo, Pb, Zn, Ni, Cu nezinye izakhi kumasampuli e-geological;ingase futhi isetshenziselwe ukuthola ukulandelela izakhi zensimbi eziyigugu kumasampula okwakheka komhlaba (ngemuva kokuhlukana nokunothisa);
2. Ukunqunywa kwezinto ezimbalwa kuya kweziningi zezinto ezingcolile ezinsimbi ezihlanzekile kakhulu kanye nama-oxide ahlanzekile, amasampula empushana njenge-tungsten, i-molybdenum, i-cobalt, i-nickel, i-tellurium, i-bismuth, i-indium, i-tantalum, i-niobium, njll.;
3. Ukuhlaziywa kwe-trace kanye ne-trace elements kumasampuli empuphu engancibiliki njengezitsha zobumba, ingilazi, umlotha wamalahle, njll.
Enye yezinhlelo ezibalulekile ezisekelayo zokuhlaziya amasampula okuhlola i-geochemical
Ilungele ukutholwa kwezingxenye zokungcola ezintweni ezihlanzeke kakhulu
I-Optical Imaging System Esebenzayo
Isistimu yokubona ye-Ebert-Fastic kanye nendlela yokubona yamalensi amathathu yamukelwa ukuze isuse ukukhanya okulahlekile, isuse i-halo ne-chromatic aberration, inciphise ingemuva, ithuthukise ikhono lokuqoqa ukukhanya, ukulungiswa okuhle, ikhwalithi yomugqa we-spectral efanayo, futhi izuze ifa ngokugcwele indlela yokubona eyodwa. -imitha grating spectrograph Izinzuzo.
Umthombo wokukhanya we-accitation we-AC ne-DC
Kulula ukushintsha phakathi kwe-AC ne-DC arcs.Ngokusho kwamasampuli ahlukene azohlolwa, ukukhetha imodi ethokozisayo efanele kunenzuzo ukuthuthukisa ukuhlaziya kanye nemiphumela yokuhlolwa.Kumasampuli angasebenzisi, khetha imodi ye-AC, futhi kumasampula e-conductive, khetha imodi ye-DC.
Ama-electrode angaphezulu naphansi ahamba ngokuzenzakalelayo endaweni ekhethiwe ngokusho kwezilungiselelo zepharamitha yesofthiwe, futhi ngemva kokuqedwa kwe-excitation, susa, futhi ubeke esikhundleni se-electrode, okulula ukusebenza futhi inokunemba okuphezulu kokuqondanisa.
Ubuchwepheshe bokuboniswa kwesithombe se-electrode okunelungelo lobunikazi bubonisa yonke inqubo yenjabulo efasiteleni lokubuka eliphambi kwethuluzi, elilungele abasebenzisi ukubuka isasasa lesampula egumbini lokuvusa, futhi lisiza ukuqonda izakhiwo nokuziphatha okujabulisayo kwesampula. .
Indlela ye-Optical | Uhlobo lwe-Ebert-Fastic oluma ngokulinganayo | Ibanga lamanje | 2~20A(AC) 2~15A(DC) |
Imigqa Yokugaya Indiza | 2400 izingcezu/mm | Umthombo wokukhanya ojabulisayo | I-AC/DC arc |
Ubude bokugxila bendlela yokubona | 600mm | Isisindo | Cishe 180Kg |
I-spectrum yetiyori | 0.003nm (300nm) | Ubukhulu (mm) | 1500(L)×820(W)×650(H) |
Isixazululo | 0.64nm/mm (isigaba sokuqala) | Izinga lokushisa eliqhubekayo legumbi le-spectroscopic | 35OC±0.1OC |
I-Falling Line Dispersion Ratio | Isistimu yokutholwa enesivinini esiphezulu evumelanisiwe esekelwe kubuchwepheshe be-FPGA benzwa ye-CMOS esebenza kahle | Izimo zemvelo | Ukushisa kwegumbi 15 OC ~ 30 OC Umswakama ohlobene <80% |