scholarly journals VLBI data, acquisition, environmental effects

1995 ◽  
Vol 33 ◽  
pp. 345 ◽  
Author(s):  
Thomas A. Herring
Keyword(s):  
Data Acquisition ◽  
Environmental Effects ◽  
Vlbi Data

scholarly journals The Mark IV VLBI Data-Acquisition and Correlation System

1993 ◽  
Vol 156 ◽  
pp. 151-157
Author(s):  
Alan R. Whitney
Keyword(s):  
Data Acquisition ◽  
Cost Effective ◽  
Data Acquisition System ◽  
Data Rate ◽  
Acquisition System ◽  
The Past ◽  
Vlbi Observations ◽  
Data Rates ◽  
Correlation System ◽  
Vlbi Data

Modern VLBI observations for both astronomy and geodesy continue to demand the utmost in sensitivity. Of the methods potentially available for increasing the sensitivity of continuum VLBI observations, increasing the recorded bandwidth is generally the most cost effective.Over the past two years a broadly-supported program has been underway at Haystack Observatory to increase the sensitivity of the Mark IIIA VLBI system by more than a factor of 2. The result is an upgrade to the existing Mark IIIA data-acquisition system, dubbed Mark IV, which increases the maximum data rate to 1024 Mbits/sec, more than quadrupling the maximum data-rate of the Mark IIIA.A new correlator, based on a new custom VLSI correlator chip is also being designed to support the 1 Gbit/sec data rates from the Mark IV data-acquisition-system. An international collaborative effort is being mounted to help defray the high costs of development.

scholarly journals Receiving And Data Acquisition Systems Of Rt-32 For Vlbi Observations / Rt-32 Uztveršanas Un Datu Reģistrācijas Sistēmas Vlbi Novērojumiem

2012 ◽  
Vol 49 (6-II) ◽  
pp. 30-42
Author(s):  
Vl. Bezrukovs ◽  
I. Shmeld ◽  
M. Nechaeva ◽  
J. Trokss ◽  
D. Bezrukovs ◽  
...  
Keyword(s):  
Data Acquisition ◽  
Radio Astronomy ◽  
Very Long Baseline Interferometry ◽  
Low Frequency ◽  
Current Status ◽  
Data Acquisition Systems ◽  
Long Baseline ◽  
Vlbi Observations ◽  
Parabolic Antenna ◽  
Vlbi Data

Abstract Radiotelescope RT-32 is a fully steerable 32-m parabolic antenna located at Irbene and belonging to Ventspils International Radio Astronomy Centre (VIRAC). Currently, the work on upgrading and repair of its receiving hardware and data acquisition systems is of high priority for the VIRAC. One of the main scientific objectives for the VIRAC Radioastronomical observatory is VLBI (very long baseline interferometry) observations in centimetre wavelengths in collaboration with world VLBI networks, such as European VLBI network (EVN), Low Frequency VLBI network (LFVN), and others. During the last years the room in the secondary focus of telescope was reconstructed, and several new receivers were installed. Currently, RT-32 observations are carried out in four different bands: 92 cm, 18 cm, 6 cm, and 2.5 cm. First three of them are already successfully employed in diversified VLBI experiments. The receiver on 2.5 cm band has only one linear polarized chain and is used mainly for the methanol maser single dish observations. The apparatus system of RT-32 is equipped with two independent VLBI data acquisition systems: TN-16, and DBBC in combination with MK5b. Both systems are employed in interferometric observations depending on the purpose of experiment and the enabled radiotelescopes. The current status of RT-32, the availability of its receiving and data acquisition units for VLBI observations and the previous VLBI sessions are discussed.

scholarly journals VLBI Observations of the Gravitational-Lens Images of Q0957+561

1984 ◽  
Vol 110 ◽  
pp. 243-246
Author(s):  
M. V. Gorenstein ◽  
I. I. Shapiro ◽  
N. L. Cohen ◽  
R. J. Bonometti ◽  
E. E. Falco ◽  
...  
Keyword(s):  
Time Delay ◽  
Data Acquisition ◽  
Mass Distribution ◽  
Data Acquisition System ◽  
Gravitational Lens ◽  
Acquisition System ◽  
Vlbi Observations ◽  
Vlbi Data ◽  
Cosmological Constants

We have conducted a series of VLBI observations of the gravitational-lens images of the quasar Q0957+561 (Walsh et al., 1979), utilizing the Mark III VLBI data acquisition system (Rogers et al., 1983). The goals of our observations are to (1) map the milliarcsecond structure of the A and B images, (2) detect the predicted third image of the quasar, and (3) determine the time delay between the images. We will use these results to constrain the mass distribution of the lens and, possibly, cosmological constants.

scholarly journals K-4 VLBI Data-Acquisition System

1997 ◽  
Vol 49 (6) ◽  
pp. 699-708 ◽  
Author(s):  
Hitoshi Kiuchi ◽  
Jun Amagai ◽  
Shin'ichi Hama ◽  
Michito Imae
Keyword(s):  
Data Acquisition ◽  
Data Acquisition System ◽  
Acquisition System ◽  
Vlbi Data

Imaging molecules adsorbed onto electrodes under potential control by scanning probe microscopy

1991 ◽  
Vol 49 ◽  
pp. 376-377 ◽  
Author(s):  
N.J. Tao ◽  
J.A. DeRose ◽  
P.I. Oden ◽  
S.M. Lindsay
Keyword(s):  
Surface Charge ◽  
Environmental Effects ◽  
Scanning Probe Microscopy ◽  
Statistical Significance ◽  
Electrochemical Methods ◽  
Surface Structures ◽  
Scanning Probe ◽  
Potential Control ◽  
Afm Imaging ◽  
Special Circumstances

Clemmer and Beebe have pointed out that surface structures on graphite substrates can be misinterpreted as biopolymer images in STM experiments. We have been using electrochemical methods to react DNA fragments onto gold electrodes for STM and AFM imaging. The adsorbates produced in this way are only homogeneous in special circumstances. Searching an inhomogeneous substrate for ‘desired’ images limits the value of the data. Here, we report on a reversible method for imaging adsorbates. The molecules can be lifted onto and off the substrate during imaging. This leaves no doubt about the validity or statistical significance of the images. Furthermore, environmental effects (such as changes in electrolyte or surface charge) can be investigated easily.

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