Ukufaka isiteshi sesimo sezulu esizenzakalelayo kusiza abafundi ukuthi bathole amakhono ekusebenzeni kwezinsimbi, ukubuka isimo sezulu nokuhlaziya idatha

I-Community Weather Information Network (Co-WIN) iwuhlelo oluhlanganyelwe phakathi kweHong Kong Observatory (HKO), iNyuvesi yaseHong Kong kanye neNyuvesi yaseShayina yaseHong Kong. Ihlinzeka izikole ezibamba iqhaza nezinhlangano zomphakathi ngenkundla ye-inthanethi yokuhlinzeka ngosekelo lobuchwepheshe ukuze izisize zifake futhi zilawule iziteshi zesimo sezulu ezizenzakalelayo (AWS) futhi zinikeze umphakathi idatha yokuqaphela okuhlanganisa izinga lokushisa, umswakama ohlobene, imvula, isiqondiso somoya nesivinini, nezimo zomoya . umfutho, imisebe yelanga kanye nenkomba ye-UV. Ngale nqubo, abafundi ababambe iqhaza bathola amakhono afana nokusebenza kwezinsimbi, ukubhekwa kwesimo sezulu, nokuhlaziywa kwedatha. I-AWS Co-WIN ilula kodwa iguquguquka. Ake sibone ukuthi ihluke kanjani ekusetshenzisweni okujwayelekile kwe-HKKO ku-AWS.
I-Co-WIN AWS isebenzisa ama-thermometers okumelana nama-hygrometers amancane kakhulu futhi afakwe ngaphakathi kwesihlangu selanga. Isihlangu sisebenza ngenjongo efanayo nesihlangu sikaStevenson ku-AWS evamile, sivikela izinga lokushisa kanye nezinzwa zomswakama ekuchayekeni okuqondile elangeni nasemvuleni kuyilapho sivumela ukujikeleza komoya mahhala.
Ku-Observatory ye-AWS evamile, ama-thermometers okumelana ne-platinum afakwa ngaphakathi kwesihlangu sikaStevenson ukuze kulinganiswe izinga lokushisa le-bulb eyomile kanye ne-wet-bulb, okuvumela ukubalwa komswakama ohlobene. Abanye basebenzisa izinzwa zokuswakama kwe-capacitive ukuze balinganise umswakama ohlobene. Ngokwezincomo ze-World Meteorological Organization (WMO), izikrini ezijwayelekile zikaStevenson kufanele zifakwe phakathi kwamamitha angu-1.25 no-2 ngaphezu komhlaba. I-Co-WIN AWS ​​ivamise ukufakwa ophahleni lwesakhiwo sesikole, ihlinzeka ngokukhanya okungcono nomoya omncane, kodwa endaweni ephakeme kakhulu ukusuka phansi.
Kokubili i-Co-WIN AWS ne-Standard AWS zisebenzisa izikali zemvula zamabhakede ukuze zilinganise imvula. Igeji yemvula yebhakede le-Co-WIN itholakala phezu kwesivikelo semisebe yelanga. Ku-AWS evamile, igeji yemvula ivamise ukufakwa endaweni evuleke kahle phansi.
Njengoba amathonsi emvula engena esikalini semvula sebhakede, kancane kancane agcwalisa elinye lamabhakede amabili. Lapho amanzi emvula efinyelela izinga elithile, ibhakede litshekela kolunye uhlangothi ngaphansi kwesisindo salo, likhipha amanzi emvula. Lapho lokhu kwenzeka, elinye ibhakede liyaphakama futhi liqale ukugcwala. Phinda ugcwalise futhi uthele. Inani lemvula lingabalwa ngokubala ukuthi itsheke kangaki.
Kokubili i-Co-WIN AWS kanye ne-Standard AWS zisebenzisa ama-anemometer enkomishi nama-vanes omoya ukukala isivinini somoya nesiqondiso. Inzwa yomoya ejwayelekile ye-AWS ifakwe kunsika yomoya ephakeme yamamitha ayi-10, efakwe umqhubi wombani futhi ikala umoya ongamamitha ayi-10 ngaphezu komhlaba ngokuhambisana nezincomo ze-WMO. Akufanele kube khona izithiyo eziphezulu eduze kwesayithi. Ngakolunye uhlangothi, ngenxa yemikhawulo yendawo yokufaka, izinzwa zomoya ze-Co-WIN zivame ukufakwa kuma-mass amamitha ambalwa ukuphakama ophahleni lwezakhiwo zemfundo. Kungase futhi kube nezakhiwo ezinde eduze.
I-Co-WIN AWS ​​barometer i-piezoresistive futhi yakhelwe kukhonsoli, kuyilapho i-AWS evamile isebenzisa ithuluzi elihlukile (njenge-capacitance barometer) ukukala umfutho womoya.
I-Co-WIN AWS izinzwa zelanga neze-UV zifakwe eduze kwegeji yemvula yamabhakede. Inkomba yeleveli inamathiselwe kunzwa ngayinye ukuze kuqinisekiswe ukuthi inzwa isendaweni evundlile. Ngakho-ke, inzwa ngayinye inomfanekiso ocacile we-hemispherical wesibhakabhaka ukukala imisebe yelanga yomhlaba wonke kanye namandla e-UV. Ngakolunye uhlangothi, iHong Kong Observatory isebenzisa amapyranometer athuthuke kakhulu nama-radiometer e-ultraviolet. Afakwe ku-AWS eqokwe ngokukhethekile, lapho kunendawo evulekile yokubuka imisebe yelanga kanye namandla emisebe ye-UV.
Kungakhathaliseki ukuthi i-Win-win AWS noma i-AWS evamile, kunezidingo ezithile zokukhetha isayithi. I-AWS kufanele ibekwe kude nama-air conditioner, phansi kukakhonkolo, izindawo ezikhanyayo nezindonga eziphakeme. Kufanele futhi ibe lapho umoya ungahamba khona ngokukhululeka. Uma kungenjalo, izilinganiso zezinga lokushisa zingathinteka. Ngaphezu kwalokho, igeji yemvula akufanele ifakwe ezindaweni ezinomoya ukuze amanzi emvula angapheshulwa umoya onamandla futhi afinyelele esikalini semvula. Ama-anemometers kanye nama-vane sezulu kufanele afakwe phezulu ngokwanele ukuze kuncishiswe ukuvinjwa kwezakhiwo ezizungezile.
Ukwanelisa izimfuneko zokukhetha isayithi ezingenhla ze-AWS, i-Observatory yenza yonke imizamo yokufaka i-AWS endaweni evulekile, ngaphandle kwezithiyo ezivela ezakhiweni eziseduze. Ngenxa yezinkinga zemvelo zesakhiwo sesikole, amalungu e-Co-WIN ngokuvamile kufanele afake i-AWS ophahleni lwesakhiwo sesikole.
I-Co-WIN AWS ​​ifana ne- "Lite AWS". Ngokusekelwe kokuhlangenwe nakho kwangaphambilini, i-Co-WIN AWS ​​"iyabiza kakhulu kodwa inzima kakhulu" - ithwebula izimo zezulu kahle uma iqhathaniswa ne-AWS evamile.

Eminyakeni yamuva nje, i-Observatory yethule inethiwekhi yolwazi lomphakathi yesizukulwane esisha, i-Co-WIN 2.0, esebenzisa ama-microsensors ukukala umoya, izinga lokushisa, umswakama ohlobene, njll. Inzwa ifakwe endlini emise okwesibani. Ezinye izingxenye, njengezihlangu zelanga, zikhiqizwa kusetshenziswa ubuchwepheshe bokuphrinta be-3D. Ukwengeza, i-Co-WIN 2.0 isebenzisa ezinye izindlela zomthombo ovulekile kukho kokubili ama-microcontrollers nesofthiwe, yehlisa kakhulu izindleko zesofthiwe ne-hardware. Umqondo ongemuva kwe-Co-WIN 2.0 ukuthi abafundi bangafunda ukwenza eyabo i-“DIY AWS” futhi bathuthukise isoftware. Ukuze kufezeke lokhu, i-Observatory iphinde ihlele amakilasi ochwepheshe abafundi. I-Hong Kong Observatory ithuthukise i-AWS yekholomu esekelwe ku-Co-WIN 2.0 AWS futhi yayisebenzisa ukuze isebenze ukuqapha isimo sezulu sesikhathi sangempela sasendaweni.