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Akademický článek

Diabetes self-management education improves quality of care and clinical outcomes determined by a diabetes bundle measure

Autor: Brunisholz KD, Briot P, Hamilton S, Joy EA, Lomax M, Barton N, Cunningham R, Savitz LA, Cannon W

Publikováno v: Journal of Multidisciplinary Healthcare, Vol 2014, Iss default, Pp 533-542 (2014)

Kimberly D Brunisholz,1,2,* Pascal Briot,1,2,* Sharon Hamilton,1 Elizabeth A Joy,3 Michael Lomax,2 Nathan Barton,2 Ruthann Cunningham,3 Lucy A Savitz,2 Wayne Cannon1 1Primary Care Clinical Program, Intermountain Healthcare, Salt Lake City, UT, USA; 2

Externí odkaz: https://doaj.org/article/edb534dae9ec44c294d7eb20fff43509

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Radio Imaging of SN 1993J: The Story Continues

Autor: Bietenholz, M. F., Bartel, N., Rupen, M. P., Dwarkadas, V. V., Beasley, A. J., Graham, D. A., Venturi, T., Umana, G., Cannon, W., Conway, J.

We present the most recent VLBI images of SN 1993J, taken at 1.7 GHz on 2010 March 5-6, along with a discussion of its evolution with time. The new image is the latest in a sequence covering almost the entire lifetime of the supernova. For these late

Externí odkaz: http://arxiv.org/abs/1103.1783

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Probing cosmic plasma with giant radio pulses

Autor: Kondratiev, V. I., Popov, M. V., Soglasnov, V. A., Kovalev, Y. Y., Bartel, N., Cannon, W., Novikov, A. Yu.

VLBI observations of the Crab pulsar with the 64-m radio telescope at Kalyazin (Russia) and the 46-m radio telescope of the Algonquin Radio Observatory (Canada) at 2.2 GHz and single-dish observations of the millisecond pulsar B1937+21 with the GBT (

Externí odkaz: http://arxiv.org/abs/astro-ph/0703046

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Giant Pulses from PSR B1937+21 with widths <= 15 nanoseconds and T_b >= 5 x 10^39 K, the Highest Brightness Temperature Observed in the Universe

Autor: Soglasnov, V. A., Popov, M. V., Bartel, N., Cannon, W., Novikov, A. Yu., Kondratiev, V. I., Altunin, V. I.

Publikováno v: Astrophys.J. 616 (2004) 439-451

Giant radio pulses of the millisecond pulsar B1937+21 were recorded with the S2 VLBI system at 1.65 GHz with NASA/JPL's 70-m radio telescope at Tidbinbilla, Australia. These pulses have been observed as strong as 65000 Jy with widths <= 15 ns, corres

Externí odkaz: http://arxiv.org/abs/astro-ph/0408285

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Pulsar microstructure and its quasi-periodicities with the S2 VLBI system at a resolution of 62.5 nanoseconds

Autor: Popov, M. V., Bartel, N., Cannon, W. H., Novikov, A. Yu., Kondratiev, V. I., Altunin, V. I.

Publikováno v: Astron.Astrophys. 396 (2002) 171-187

We report on a study of microstructure and its quasi-periodicities of three pulsars at 1.65 GHz with the S2 VLBI system at a resolution of 62.5 ns, by far the highest for any such statistical study yet. For PSR B1929+10 we found in the average cross-

Externí odkaz: http://arxiv.org/abs/astro-ph/0107073

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The S2 VLBI Correlator: A Correlator for Space VLBI and Geodetic Signal Processing

Autor: Carlson, B. R., Dewdney, P. E., Burgess, T. A., Casorso, R. V., Petrachenko, W. T., Cannon, W. H.

We describe the design of a correlator system for ground and space-based VLBI. The correlator contains unique signal processing functions: flexible LO frequency switching for bandwidth synthesis; 1 ms dump intervals, multi-rate digital signal-process

Externí odkaz: http://arxiv.org/abs/astro-ph/9908314

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