A cikin 'yan makonnin nan, takaddamar da ke bayan sabon hanci na Formula 1 ya kasance mai girma. Idan ga mutane da yawa, sababbin hanci sun fi kama da caricatures, ga wasu suna ɗaukar siffofi da ke nuna mu ga yanayi ko abubuwa a cikin siffar phallic.
Ba ma so mu dame ku da manyan tambayoyi na injiniya da kuma hadadden lissafi, don haka bari mu sanya batun a matsayin haske kamar yadda su kansu hanci, wanda kuma ba ma son yin magana game da batutuwan da ke kusa da su. .
Williams Mercedes FW36
Gaskiyar ita ce, akwai dalilai masu kyau da ya sa irin wannan nau'in zane ya kama a cikin 2014 kuma za mu iya godiya da hakan. biyu daga cikin manyan dalilai alaka da: da Dokokin FIA da kuma lafiyar mota.
Me ya sa ake samun irin waɗannan tsararren ƙira tsakanin hanci? Amsar ita ce mafi sauƙi kuma kawai aikin injiniya ne mai tsabta, "baƙar fata" wanda ya ɗauki shekaru don ƙwarewa, kamar yadda ba koyaushe zai yiwu a haɗa mafi kyawun sakamako ba.
Abin sha'awa shine, injiniyoyi iri ɗaya waɗanda suka kawo sabbin abubuwa a duniyar Formula 1 kamar su carbon fiber monocoque Tsarin, 6-wheel single-seaters, twin diffusers da tsarin rage ja da iska, suma suna shirye su yi komai don cin gajiyar duk fa'idodin da ƙa'idodin ba da izini, ta yadda motocin su ne suka fi gudu a gasar.
Tyrell Ford 019
Amma bari mu bayyana muku yadda muka isa ga wani zane mai banƙyama, yana sa mu yi tambaya game da hayyacin waɗanda ke bayan tsarin injiniya na Formula 1. Dukkanin ya koma shekaru 24, tare da Tyrell 019 mai zama ɗaya, a lokacin 1990 da kuma ƙungiyar fasaha, tare da darekta Harvey Postlethwaite da shugaban zane Jean-Claude Migeo, sun gane cewa yana yiwuwa a watsar da iska mai yawa a cikin ƙananan ɓangaren F1 idan sun canza ƙirar hanci ta hanyar duba kana da matsayi mafi girma idan aka kwatanta da reshe. .
Ta hanyar yin wannan, iskar da ke yawo a cikin ƙananan yanki na F1 zai kasance mafi girma, kuma ta hanyar daɗaɗɗen iska ta hanyar ƙananan yanki maimakon na sama, zai haifar da haɓakar iska mai girma a cikin Formula 1 aerodynamics umarni ne mai tsarki a cikin Littafi Mai-Tsarki na kowane injiniya . Daga nan ne, hanci ya fara tashi dangane da jirgin saman da ke kwance na reshe na gaba, sashin da aka haɗa su.
RedBull ToroRosso Renault STR9
Amma waɗannan canje-canjen hawan hanci sun haifar da matsaloli, daidai a cikin 2010 kakar a Valencia GP, lokacin da Mark Webber's Red Bull, bayan wani rami a kan cinya tara, ya sa Webber ya ɗauka a kan gama kai tsaye bayan fita daga ramuka, Lotus. da Kovalinen. Webber ya sanya kansa a bayan Kovaleinen kuma ya yi amfani da ingantaccen kwararar sa, wanda kuma aka sani da mazugi. Webber ya yanke shawarar yin ƙoƙari ya wuce kuma ya jira Kovaleinen ya fita daga hanya, amma maimakon haka, Kovaleinen ya buge da birki na Lotus kuma Webber's Red Bull hancin ya taɓa motar Lotus ta baya, ya aika da shi yana jujjuya digiri 180 kuma ya tashi. a kusan 270km/ h zuwa ga shingen taya.
Bayan faruwar wannan lamari dai, hukumar ta FIA ta bayyana cewa hancin ya yi tashin gwauron zabi, wanda hakan na iya haifar da hadari ga matukan jirgin, saboda suna iya buga kan matukin jirgin idan wani hatsari ya faru. Tun daga nan, FIA ta kafa sababbin dokoki kuma an tsara matsakaicin tsayin daka na gaba na F1 a 62.5cm, tare da matsakaicin tsayin da aka ba da izini ga hanci na 55cm dangane da jirgin saman kujera daya, wanda aka wakilta. ta hanyar ƙananan motar mota da kuma cewa ba tare da la'akari da tsarin dakatarwa ba, ba zai iya zama sama da 7.5cm daga ƙasa ba.
A wannan shekara, an hana manyan hancin da aka gani zuwa yanzu, bisa sabbin ka'idojin aminci. Amma abin da ke tafiyar da zane mai ban dariya shine canje-canjen tsari: ya bayyana cewa hanci ba zai iya zama fiye da 18.5 cm tsayi ba dangane da jirgin motar, wanda idan aka kwatanta da shekara ta 2013 yana wakiltar raguwar 36.5 cm da sauran gyara ga dokoki, a cikin aya 15.3.4 na ka'idar. , ya bayyana cewa F1 dole ne ya sami sashin giciye guda ɗaya a gaban tsinkayar kwance, tare da matsakaicin 9000mm² (50mm a bayan ƙarshen mafi ci gaba watau tip na hanci).
Kamar yadda yawancin ƙungiyoyi ba sa son sake fasalin dakatarwar gaba da gaba na F1 ɗin su, sun zaɓi sauke jirgin daga saman hannun dakatarwar. Amma a lokaci guda suna so su ci gaba da haɓaka hanci kamar yadda zai yiwu. Sakamakon haka shine wannan zane tare da irin waɗannan fitattun cavities na hanci.
Farashin F14T
Domin 2015, dokokin za su kasance ma fi tsayi kuma kawai motar da ta riga ta bi su ita ce Lotus F1. A cikin Lotus F1 hanci ya riga ya sami kusurwar saukar da linzamin kwamfuta zuwa ƙarshen ƙarshe, don haka ana sa ran ƙarin rhinoplasty a cikin sauran F1. Yayin da aminci shine babban fifiko a cikin Formula 1, aerodynamics ya kasance babban fifiko ga duk injiniyoyinsa.
Tare da waɗannan canje-canjen yanzu yana yiwuwa a kafa nau'ikan kujerun mota guda biyu na F1 don wannan kakar. A daya hannun muna da pointy-nosed F1 , wanda lalle ne zai zama mafi sauri mota a kan straights saboda da karami gaban surface da ƙananan aerodynamic juriya, gyara ga saman gudun, A daya bangaren kuma muna da motocin F1 wadanda za su rika lankwasa cikin sauri sosai , tare da manyan kogon hancinsa a shirye don samar da babban ƙarfin iska, saboda girman gaban gaba. Tabbas, koyaushe muna magana game da ƙarancin bambance-bambance tsakanin motoci, amma a cikin Formula 1 komai yana ƙidaya.
Idan gaskiya ne cewa F1 cavities na hanci za su karkata da sauri sosai, saboda girman ƙarfinsu don samar da ƙarfin iska, sakamakon mafi yawan iska mai vortexed ta cikin ƙananan yanki, kuma gaskiya ne cewa za su kasance a hankali a kan ƙasa. madaidaiciya, wanda aka azabtar ta hanyar ja aerodynamics da za su samar. Waɗannan za su buƙaci amfani da ƙarin ƙarfin dawakai 160 na tsarin (ERS-K) don ramawa, yayin da sauran za su buƙaci ƙarin ikon tsarin (ERS-K) daga sasanninta don samun saurin sauri saboda ƙananan ƙarfin iska a cikin sasanninta.
Tilastawa Indiya Mercedes VJM07