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Barry Clark

dblp:10/5575 · DBLP profile ↗
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3ranked-venue papers
0as first author
0since 2021 · last 2009
—ORCID · none

Domains — the database's venue-derived domains; a paper can count in several

Applied, interdisciplinary, general and emerging computing · 2Systems, architecture and hardware · 1

Expertise — from the expertise taxonomy: the topics of the expert's papers under the CCF categories. A weight counts papers with recency: 1 for a paper about the topic, 0.3 when the topic is its context, halved every five years.

Computer architecture, parallel and distributed computing, and storage systems
1 paper
Integrated circuit design · 56% Electronic design automation · 44%
Computer networks
1 paper
Physical-layer communications · 100%

Topics — the 6 heaviest of 6, each with the papers that count most for it

TopicWeightPapersLastEvidence papers
Electronic design automation › system-level design
IP reuse		 0.012001
SoC Integration of Reusable Baseband Bluetooth IP · DAC 2001
Integrated circuit design › system-on-chip
system-on-chip integration		 0.012001
SoC Integration of Reusable Baseband Bluetooth IP · DAC 2001
Physical-layer communications
radio astronomy instrumentation		 0.011994
The Very Long Baseline Array · Proc. IEEE 1994
Physical-layer communications
very long baseline interferometry		 0.011994
The Very Long Baseline Array · Proc. IEEE 1994
Integrated circuit design › analog and mixed-signal circuits
mixed-signal circuit design		 0.012001
SoC Integration of Reusable Baseband Bluetooth IP · DAC 2001
Physical-layer communications
antenna arrays		 0.011994
The Very Long Baseline Array · Proc. IEEE 1994

Methods — techniques the papers use, named apart from their topics

wideband recording · 0.0correlation processing · 0.0
YearPublicationVenuePosition
2009 The Expanded Very Large Array
abstract
In almost 30 years of operation, the Very Large Array (VLA) has proved to be a remarkably flexible and productive radio telescope. However, the basic capabilities of the VLA have changed little since it was designed. A major expansion utilizing modern technology is currently under way to improve the capabilities of the VLA by at least an order of magnitude in both sensitivity and in frequency coverage. The primary elements of the Expanded Very Large Array (EVLA) project include new or upgraded receivers for continuous frequency coverage from 1 to 50 GHz, new local oscillator, intermediate frequency, and wide bandwidth data transmission systems to carry signals with 16 GHz total bandwidth from each antenna, and a new digital correlator with the capability to process this bandwidth with an unprecedented number of frequency channels for an imaging array. Also included are a new monitor and control system and new software that will provide telescope ease of use. Scheduled for completion in 2012, the EVLA will provide the world research community with a flexible, powerful, general-purpose telescope to address current and future astronomical issues.
Richard Perley, Peter Napier, Jim Jackson, Bryan Butler, Brent Carlson, David Fort, Peter Dewdney, Barry Clark, Robert Hayward, Steven Durand, Mike Revnell, Mark McKinnon
 Proc. IEEE8
2001 SoC Integration of Reusable Baseband Bluetooth IP
abstract
This presentation will give a list of design criteria an ASIC Design house need to look in the process of deciding to take the complex Bluetooth specification and implement everything from scratch or to integrate reusable Intellectual Property for integration into their SoC.
Torbjörn Grahm, Barry Clark
 DAC2
1994 The Very Long Baseline Array
abstract
The Very Long Baseline Array (VLBA) consists of ten high performance antennas and a 20-station correlator. The 25-m-diameter reflector antennas are located geographically to optimize spatial frequency coverage for high-duality imaging using VLBI techniques. The antennas are equipped with receivers for nine frequency bands over the range 300 MHz to 45 GHz. A wideband, high-density, recording system allows unattended operation at a sustained data rate of 125 Mb/s for a day, and peak rates of up to 512 Mb/s. The antennas operate unattended most of the time, and are controlled by a single operator in the Array Operations Center (AOC) at Socorro, NM. The correlator, located in the AOC, supports processing of all observations with the array.>
Peter Napier, Durgadas S. Bagri, Barry Clark, Alan E. E. Rogers, Jonathan D. Romney, A. Richard Thompson, R. Craig Walker
 Proc. IEEE3