Isivunguvungu se-Schumann esisizungezile

Imvamisa ye-Schumann iyisici samagagasi kagesi esiphila kuwo, ngoba Zihamba kusukela ebusweni bomhlaba kuya kwi-ionosphere. Ukubukeka kwabo kubangelwa ukuthi iplanethi yethu iyi-resonator enkulu futhi igcwele igesi eliqhuba kahle kagesi. Umgogodla womhlaba ibhola lensimbi ngobubanzi obuyizingalo eziyizigidi eziyizinkulungwane ezingu-6.96, kanti igobolondo lalo limanzi futhi liyashisa (2.26,000 km), futhi isikhungo - siqinile. Ngenxa yesimo sokudluliselwa komzimba, izingxenye zixubene, zakha amasimu kagesi.

Isimo samagagasi angenhla satholakala ngososayensi waseJalimane u-Otto Schumann waseNyuvesi yaseMunich. Kancane kancane, ngesikhathi sokuhlolwa okuhlukahlukene, kwatholakala ukuthi imvamisa ye-Schumann ingu-7.8 Hz. Nokho, leli xabiso alonawo kuphela. Lesi sici sinamanye "amaphuzu" emafenjini aphindaphindiwe angama-6, isb. Ngo-8, 14 - 20 - 24 - 32 Hz. Imvamisa eyinhloko iyafana - 7.8 Hz, kodwa ingahluka phakathi kuka-0,15 -0,2 Hz futhi ihluke ngaphakathi kwebanga kusuka ku-7 ukuya ku-10-11 Hz.

Ngaphansi kwethonya lensiza ye-Schumann? Ososayensi bakholelwa ukuthi kungathonywa yi: izigaba zenyanga, isimo seSanga (isigaba somsebenzi), isimo samanzi emanzini olwandle, isikhathi sosuku (ebusuku) inkontileka ye-wave amplitudes), isikhundla esisehlabathini (amagagasi akhulunywa kakhulu ebhanini le-equatorial).

Ukuvama kwensimu yamagnetic yomhlaba kuyinto engaqondakaliyo, ngoba isayensi yanamuhla ayinakukwazi ukuchaza ukuzinza kwayo okungajwayelekile. Kodwa wonke umuntu uyaqaphela ukuthi ngaphandle kokuvikeleka kwalokhu kuphila kwenkambu kwakungeke kube khona ngenxa ye-irradiation ye-cosmic. Lesi sici somhlaba sinamandla amakhulu ezindaweni ezahlukene. EYurophu, inani layo elilinganiselwe liyashintsha elizungeze 0.5 Gauss, kodwa kunamaphuzu lapho imingcele ingadlula isizinda esivamile ngesigamu. Kucatshangwa ukuthi izingxenye "zamandla" zigxila kulezi zindawo, futhi abantu beza lapho ukuvuselela noma ukwenza amasiko athile.

Njengamanje, insimu ye-electromagnetic yeplanethi ibuthakathaka futhi, njengoba abacwaningi basikisela, "kungavimbela" isikhathi esithile, okuzoholela ekuguqulweni kwezigxobo zamagnetic, izinhlekelele kanye nezinguquko eziphilayo eziphilayo ezingeni lezakhi zofuzo. Kukholelwa ukuthi ukungabi khona kwensimu kungasinda kuphela kunamandla kakhulu futhi okushintshiwe. Njengoba isikhala sezindiza sibonisiwe, umuntu angeke abe khona ngaphandle kwalesi sivikelo isikhathi eside, ngoba Ukunciphisa umzimba kwakhe kunciphise kakhulu.

Namuhla amahemuhemu asakazela ukuthi imvamisa ye-Schumann Emhlabeni iyanda kusuka ku-standard 7.83 kuya ku-15 Hz. Futhi lokhu kungathinta kakhulu abantu, ngoba Ama-frequencies e-Schumann asondelene kakhulu nama-alpha-isigqi sobuchopho (8-13 Hz), isici somuntu ngamunye ngokuvuka okuthulile. Ososayensi bakholelwa ukuthi ukwanda kwakuyobe kwenzeka, uma isivinini sokukhanya noma ububanzi beplanethi sashintshile, noma i-ionosphere yayiyophakama ibe ngu-300-400 km. Kulezi zici, yilabo kuphela abagcina banelungelo lokuba khona, kusukela Ebusuku, imingcele ye-ionosphere iphakama phezulu.

Umthelela oqondile walolu shintsho olwenzekayo kwizinto eziphilayo azange zenziwe, kodwa ukwahlulela ngenani elikhulayo lokubulala, ukuzibulala, nokuhlaselwa kwamaphekula, umvuthwandaba womhlaba ungaphazamisa ukuziphatha kwabantu ngendlela ethile. Okungenani ngoba ukuvama okwandayo kwe-15 Hz ngaphezulu kufana nesigaba se-beta, isici se-state esebenzayo yomuntu.