| dc.contributor.author | Artal Latorre, Eduardo | |
| dc.contributor.author | Aja Abelán, Beatriz | |
| dc.contributor.author | Cano de Diego, Juan Luis | |
| dc.contributor.author | Fuente Rodríguez, Luisa María de la | |
| dc.contributor.author | Terán Collantes, José Vicente | |
| dc.contributor.author | Villa Benito, Enrique | |
| dc.contributor.other | Universidad de Cantabria | es_ES |
| dc.date.accessioned | 2015-11-11T16:22:17Z | |
| dc.date.available | 2015-11-11T16:22:17Z | |
| dc.date.issued | 2015-09 | |
| dc.identifier.uri | http://hdl.handle.net/10902/7638 | |
| dc.description.abstract | Cryogenic cooled very low noise amplifiers are critical components in radio astronomy receivers and other applications. A general description of these devices and their role in receivers is presented. Several examples of microwave and millimeter wave amplifiers covering bands from 4 GHz to 36 GHz are described. Noise temperatures of about 5 K in 4-12 GHz and 15 K in 25-34 GHz bands have been achieved in mHEMT technology based amplifiers. | es_ES |
| dc.format.extent | 4 p. | es_ES |
| dc.language.iso | spa | es_ES |
| dc.rights | © 2015 URSI España | es_ES |
| dc.source | URSI 2015, XXX Simposium Nacional de la Unión Científica Internacional de Radio, Pamplona | es_ES |
| dc.title | Amplificadores criogénicos de muy bajo ruido en microondas y ondas milimétricas | es_ES |
| dc.type | info:eu-repo/semantics/conferenceObject | es_ES |
| dc.rights.accessRights | openAccess | es_ES |
| dc.type.version | publishedVersion | es_ES |
