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Uvavanyo olupheleleyo lwe-microwave lwe-LADP-17

Inkcazo emfutshane:

Esi sixhobo sovavanyo samkela ingcamango yoyilo efana ne-optical spectrometer ukuze senze uvavanyo lweempawu ze-microwave optical.


Iinkcukacha zeMveliso

Iithegi zeMveliso

Iimvavanyo

1. Ukuqonda nokufunda imigaqo esisiseko yokwenza ii-microwave kunye nokusasazwa kunye nokwamkelwa kwazo kunye nezinye iimpawu ezisisiseko;

2. I-microwaveukuphazamiseka, ukusasazeka, ukwahlukana kunye nezinye iimvavanyo;

3. Uvavanyo lokuphazamiseka kwe-microwave lukaMeckelsen;

4, Ukuqwalaselwa kwe-microwave Bragg diffraction phenomenon yeekristale ezilinganisiweyo.

Iimpawu zobugcisa eziphambili

1. I-oscillator ye-microwave esemgangathweni oqinileyo kunye ne-attenuator, i-isolator, uyilo oludibeneyo lokuhambisa uphondo, amandla e-microwave afanelekileyo, anokuncitshiswa kuluhlu olubanzi, angabi nabungozi ebantwini;

2. Isixhobo sokubona isikrini sedijithali sekristale yolwelo, uvakalelo oluphezulu, kulula ukusifunda, kunye ne-microwave receiving horn, ukuhlanganiswa kwesixhobo sokubona, ulwakhiwo oluncinci, ukusebenza okuzinzileyo;

3. Ulungelelwaniso olufanelekileyo lweziphumo zokulinganisa, akukho kuphambuka okucacileyo kwe-engile esisigxina;

4. Nika izixhobo ezahlukeneyo kunye neenkqubo zovavanyo, unokuba lubanzi, uyilo kunye nophando lwezilingo.

 

Iiparameter eziphambili zobugcisa

1. I-microwave frequency: 9.4GHz, i-bandwidth: malunga ne-200MHz;

2. Amandla e-microwave: malunga ne-20mW, ubukhulu bokunciphisa: 0 ~ 30dB;

3. Isixhobo sokubona isikrini sedijithali esineemitha ezintathu ezinesiqingatha, ukuphambuka kwe-engile yokulinganisa ≤ 3º;

4. Ukusetyenziswa kwamandla: kungabi ngaphezu kwe-25W xa umthwalo ugcwele;

5. Ixesha lokusebenza eliqhubekayo: ngaphezulu kweeyure ezi-6.


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