Ƙayyadaddun bayanai
| RM-DCPFA2640-8 | ||
| Siga | Na al'ada | Raka'a |
| Yawan Mitar | 26.5-40 | GHz |
| Riba | 8 typ. | dBi |
| VSWR | <2.2 |
|
| Polarization | Dual-Da'ira |
|
| AR | <2 | dB |
| 3dB-nisa | 57.12°-73.63° | dB |
| XPD | 25 typ. | dB |
| mai haɗawa | 2.92-Mace |
|
| Girman (L*W*H) | 32.5*39.2*12.4±5) | mm |
| Nauyi | 0.053 | kg |
| abu | Al |
|
| Gudanar da wutar lantarki, CW | 20 | W |
| Gudanar da Wutar Lantarki, Peak | 40 | W |
Eriyar ciyarwa, wacce aka fi sani da kawai a matsayin “ciyarwa,” ita ce ainihin abin da ke cikin tsarin eriya mai haskakawa wanda ke haskaka makamashin lantarki zuwa ga mai tunani na farko ko tattara kuzari daga gare ta. Ita kanta cikakkiyar eriya ce (misali, eriyar ƙaho), amma aikinta kai tsaye yana ƙayyade ingancin tsarin eriya gabaɗaya.
Babban aikinsa shi ne don "haske" babban abin haskakawa yadda ya kamata. Mahimmanci, tsarin hasken ciyarwar ya kamata ya rufe gaba dayan saman mai nuni ba tare da zubewa ba don cimma matsakaicin riba da mafi ƙarancin lobes na gefe. Dole ne a daidaita tsakiyar lokaci na ciyarwar daidai a wurin mai nuni.
Babban fa'idar wannan bangaren shine matsayinsa a matsayin "kofar" don musayar makamashi; Ƙirar sa kai tsaye yana tasiri tasirin hasken tsarin, matakan giciye-tsalle-tsalle, da madaidaicin impedance. Babban koma bayansa shine hadadden ƙirar sa, yana buƙatar daidaitaccen daidaitawa tare da mai haskakawa. Ana amfani dashi ko'ina a cikin tsarin eriya mai haskakawa kamar sadarwar tauraron dan adam, telescopes na rediyo, radar, da hanyoyin ba da sandar microwave.
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