| Content Provider |
IEEE Xplore Digital Library |
| Author |
Blanchard, Jay Crew, Geoff Doeleman, Shep Greenberg, Joseph Hecht, Michael Honma, Mareki Inoue, Makato Jacques, Christophe Lacasse, Richard Matthews, Lynn Mora, Matias Nagar, Neil Pradel, Nicola Rotteman, Helge Rusczcyk, Chester Saez, Alejandro Treacy, Robert |
| Copyright Year |
2015 |
| Description |
Author affiliation: Institute of Astronomy and Astrophysics, Academia Sinica, P.O. Box 23-141, Taipei 10617, Taiwan (Inoue, Makato; Pradel, Nicola) || MIT Haystack Observatory, Westform, USA (Crew, Geoff; Doeleman, Shep; Hecht, Michael; Matthews, Lynn; Rusczcyk, Chester) || National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo, Japan (Greenberg, Joseph; Honma, Mareki) || Joint ALMA Office, Alonso de Cordova 3107, Vitacura, Santiago de Chile, Chile (Saez, Alejandro) || Universidad de Concepción, Chile (Blanchard, Jay; Nagar, Neil) || Max-Plank-Institut für Radioastronomie, Bonn, Germany (Rotteman, Helge) || National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903, USA (Jacques, Christophe; Lacasse, Richard; Mora, Matias; Treacy, Robert) |
| Abstract |
An international group of collaborators, led by Haystack Observatory, has designed and implemented a system to phase-up the ALMA array, making it appear as a large single dish whose output can be recorded. This system includes both hardware and software. Hardware consists of a new hydrogen maser time standard, a suite of MK6 VLBI recorders, enhancements to the 64-Antenna Correlator and an optical link between the correlator at the ALMA high site and the recorders at the low site. The hydrogen maser provides enhanced timing stability to ALMA, which previously used a Rubidium time standard, making it suitable for Very Long Baseline Interferometry (VLBI). MK6 data recorders are the latest generation VLBI data recorders, using assemblies of disk drives as a recording medium, with each recorder capable of recording 16 Gbps. Enhancements to the correlator consist primarily of new modules to format the data using the VLBI Data Interchange Format (VDIF) standard. They also incorporate a new sub-system to distribute and use the VLBI time standard of one-pulse-per-second. The optical link combines 9 (8 plus one spare) 10 GbE channels of data onto one ALMA optical fiber spanning the 33 km distance between the high and low sites. Software consists of enhancements to the TelCal program to provide real-time phase feedback to phase the antennas as well as enhancements to the ALMA control software. Both the hardware and software were designed to conform to the existing ALMA infrastructure, preserving the “look and feel” of the existing system. The system is capable of formatting and recording the entire ALMA bandwidth of 16 GHz or binary sub-multiples of this down to 62.5 MHz. The system was designed primarily with Very Long Baseline Interferometry (VLBI) in mind but is also well-suited to high frequency pulsar searches. Recently, system level tests have been successfully concluded, the system has provisionally been accepted by ALMA and commissioning has begun. This talk will describe the design of the phasing system and report its status. |
| Starting Page |
291 |
| Ending Page |
291 |
| File Size |
59588 |
| Page Count |
1 |
| File Format |
PDF |
| ISBN |
9781479978175 |
| DOI |
10.1109/USNC-URSI.2015.7303575 |
| Language |
English |
| Publisher |
Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
| Publisher Date |
2015-07-19 |
| Publisher Place |
Canada |
| Access Restriction |
Subscribed |
| Rights Holder |
Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
| Content Type |
Text |
| Resource Type |
Article |
