X- To Ka- Band cryogenic LNA module for very long baseline interferometry | Kütüphane.osmanlica.com

X- To Ka- Band cryogenic LNA module for very long baseline interferometry

İsim X- To Ka- Band cryogenic LNA module for very long baseline interferometry
Yazar Fung, A., Samoska, L., Bowen, J., Montanez, S., Kooi, J., Soriano, M., Jacobs, C., Manthena, R., Hoppe, D., Akgiray, Ahmed Halid, Lai, R., Mei, X., Barsky, M.
Basım Tarihi: 2020
Basım Yeri - IEEE
Konu Indium phosphide, HEMT, Low noise, Amplifier, Coaxial module, Cryogenic
Tür Belge
Dil İngilizce
Dijital Evet
Yazma Hayır
Kütüphane: Özyeğin Üniversitesi
Demirbaş Numarası 978-1-7281-6815-9
Kayıt Numarası 708d6b7e-1258-4e6e-b24d-eb780fd12467
Lokasyon Electrical & Electronics Engineering
Tarih 2020
Örnek Metin We report a new result of a packaged low noise amplifier (LNA) module with wide bandwidth of 5 to 35 GHz and low noise temperature performance of 10 -18 K, while operated at 10 K ambient. The LNA used 3-stages of sub-50 nm gate length, 100% indium channel content indium phosphide (InP) high electron mobility transistors (HEMTs). Wideband cryogenic LNAs are important for future radio astronomy observatories. To our knowledge these results represent the lowest noise achieved in a wideband amplifier from 5-35 GHz.
DOI 10.1109/IMS30576.2020.9224106
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X- To Ka- Band cryogenic LNA module for very long baseline interferometry

Yazar Fung, A., Samoska, L., Bowen, J., Montanez, S., Kooi, J., Soriano, M., Jacobs, C., Manthena, R., Hoppe, D., Akgiray, Ahmed Halid, Lai, R., Mei, X., Barsky, M.
Basım Tarihi 2020
Basım Yeri - IEEE
Konu Indium phosphide, HEMT, Low noise, Amplifier, Coaxial module, Cryogenic
Tür Belge
Dil İngilizce
Dijital Evet
Yazma Hayır
Kütüphane Özyeğin Üniversitesi
Demirbaş Numarası 978-1-7281-6815-9
Kayıt Numarası 708d6b7e-1258-4e6e-b24d-eb780fd12467
Lokasyon Electrical & Electronics Engineering
Tarih 2020
Örnek Metin We report a new result of a packaged low noise amplifier (LNA) module with wide bandwidth of 5 to 35 GHz and low noise temperature performance of 10 -18 K, while operated at 10 K ambient. The LNA used 3-stages of sub-50 nm gate length, 100% indium channel content indium phosphide (InP) high electron mobility transistors (HEMTs). Wideband cryogenic LNAs are important for future radio astronomy observatories. To our knowledge these results represent the lowest noise achieved in a wideband amplifier from 5-35 GHz.
DOI 10.1109/IMS30576.2020.9224106
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