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Low noise amplifier design for dense phased arrays
Radio Astronomers demand for highly sensitive astronomical facility. Their demand is a radio telescope that can detect the weakest and deepest radio signal. To fulfill the demand of high sensitive telescope, an entirely new way of realizing a radio telescope is required. One of the most important components in the RF front end that determines the sensitivity of a radio telescope is the Low Nois…
Contributors
- Woestenberg Bert
- Beckman Claes
- Högskolan i Gävle Institutionen för teknik och byggd miljö
Creator
- Mohammad Afzal 1981- , Högskolan i Gävle, Institutionen för teknik och byggd miljö
Type of item
- Student thesis
- book
- Book
Date
- 2008
- 2008-05-09
- 2008-05-09
- 2008
Contributors
- Woestenberg Bert
- Beckman Claes
- Högskolan i Gävle Institutionen för teknik och byggd miljö
Creator
- Mohammad Afzal 1981- , Högskolan i Gävle, Institutionen för teknik och byggd miljö
Type of item
- Student thesis
- book
- Book
Date
- 2008
- 2008-05-09
- 2008-05-09
- 2008
Providing institution
Aggregator
Rights statement for the media in this item (unless otherwise specified)
- http://rightsstatements.org/vocab/InC/1.0/
- http://rightsstatements.org/vocab/InC/1.0/
Identifier
- oai:DiVA.org:hig-518
Format
- electronic99
- electronic
- 99
Language
- en
Is part of
- http://data.theeuropeanlibrary.org/Collection/a1041
Year
- 2008
Providing country
- Sweden
Collection name
First time published on Europeana
- 2014-09-07T10:32:39.419Z
Last time updated from providing institution
- 2014-09-07T10:32:39.419Z