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References: [ +subject:/^(?:^\s*(re|sv|fwd|fw)[\[\]\d]*[:>-]+\s*)*LF\:\s+Very\s+large\s+adaptive\s+rx\s+array\s*$/: 4 ]

Total 4 documents matching your query.

1. Re: LF: Very large adaptive rx array (score: 1)
Author: [email protected]
Date: Mon, 12 Feb 2001 09:02:27 EST
Hi Paul, Nick, thank you for your interesting and helpful comments. In VLBI a very high stability frequency standard (hydrogen masers etc.) is used as a phase reference on each receiving station and
/rsgb_lf_group-archives/html/rsgb_lf_group/2001-02/msg00347.html (11,643 bytes)

2. Re: LF: Very large adaptive rx array (score: 1)
Author: "Nick" <[email protected]>
Date: Mon, 12 Feb 2001 08:57:19 +0000
for something? It might be a good idea to check what the radio astronomers have done during the last decades and hopefully some good ideas could be found that could now be implemented using low cost
/rsgb_lf_group-archives/html/rsgb_lf_group/2001-02/msg00354.html (9,182 bytes)

3. Re: LF: Very large adaptive rx array (score: 1)
Author: "Paul Keinanen" <[email protected]>
Date: Mon, 12 Feb 2001 09:18:04 +0200
Hi group, is there more you can do with that CW carrier-component than simply detect the presence of a signal without being able to decode it? Well, we could use it to guide a large adaptive array t
/rsgb_lf_group-archives/html/rsgb_lf_group/2001-02/msg00357.html (12,474 bytes)

4. LF: Very large adaptive rx array (score: 1)
Author: [email protected]
Date: Sun, 11 Feb 2001 21:16:15 EST
Hi group, is there more you can do with that CW carrier-component than simply detect the presence of a signal without being able to decode it? Well, we could use it to guide a large adaptive array to
/rsgb_lf_group-archives/html/rsgb_lf_group/2001-02/msg00360.html (9,267 bytes)


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