Hostname: page-component-cd9895bd7-gxg78 Total loading time: 0 Render date: 2024-12-26T06:04:00.407Z Has data issue: false hasContentIssue false
  • English
  • Français

31. Time : (Heure)

Published online by Cambridge University Press:  25 April 2016

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The work of IAU Commission 31 is contained in the following sections contributed by the Members.

The two Working Groups installed during the period 1984-1987 :

“The Use of Millisecond Pulsars and Timing of Pulsars”

and

“Time Transfer with Modern Techniques”,

chaired by D. ALLAN and H. FLIEGEL respectively, maintained their activities and will report at the General Assembly. Time transfer with GPS has been and is still of concern with the introduction of the Selective Availability (SA), but the adaptation of the common view method seems to overcome part of this difficulty (Fliegel et al., 1990).

Type
Research Article
Information
Transactions of the International Astronomical Union , Volume 21 , Issue 1 , 1991 , pp. 327 - 337
Copyright
Copyright © Kluwer 1991

References

Bauch, A. : 1990, Proc. of the 2nd EFTF, Neuchâtel, 1988, 425–436.Google Scholar
Bauch, A., Heindorff, T. : 1989, Proc. of the 4th Symposium on Frequency Standards and Metrology, Ancona 1988, 370–373.Google Scholar
de Boer, H. : 1990, Proc. of the 4th EFTF, Neuchâtel 1990.Google Scholar
De Marchi, A. : 1986, Proc. 40th Ann. Syrap. Frequ. Contr., 441–444.Google Scholar
Fliegel, H., Beard, R.L., Landis, G.P., Stebbins, S.B.: 1990, An Alternative Common View Method for Time Transfer with GPS. Journal of Navigation, 1990 (in press).Google Scholar
Goto, T., Hanada, H., Sasaki, H., Goto, Y.: 1989, Estimation of excess path delay by using the Japan spectral model of Japan Meteorological Agency, Proc. Japanese Syrap. GPS (1989), 174–180.Google Scholar
Guinot, B.: 1988, Astron. Astrophys., 192, 370–373.Google Scholar
Guinot, B., Lewandowski, W.: 1989, Bull. Geod., 61, 371–386.Google Scholar
Guinot, B., Lewandowski, W., Thomas, C.: 1990, Proc. 4th EFTP, Neuchâtel 1990.Google Scholar
Guinot, B., Petit, G. : 1990, Berkely Workshop on impact of pulsar timing on Relativity and Cosmology.Google Scholar
Guinot, B., Thomas, C. : 1989, Proc. 21st PTTI meeting, 95–106.Google Scholar
Hanada, H., Goto, Y. and Goto, T.: 1989, Excess path delay estimated with the numerical prediction data in Japan spectral model of Japan Meteorological Agency. Proc. Japanese Symp. Earth Rotation, Astrometry, and Geodesy (1988), 298–303. (AAA 49A, 1990, 036.156).Google Scholar
Hara, T., Horiai, K., Sato, K.-H., Fujishita, M., Sakai, S., Iwadate, K. and Asari, K. : 1989, Measurements of the propagation time of Loran-C signals, Proc. 20th Annual PTTI Meeting, 145–150.Google Scholar
Hara, T. and Sato, K.-H.: 1989, Total electron content observation by Doppler method, Proc. Japanese Symp. GPS (1988), 55–59.Google Scholar
Hetzel, P.: 1988, Proc. of the 2nd EFTF, Neuchâtel, 1988, 351–364.Google Scholar
Horiai, K., Tamura, Y., Sato, K.-H. and Hara, T.: 1989, Time Comparison with a Trimble 4000SX GPS Receiver, Proc. Japanese Symp. GPS (1988), 74–79.Google Scholar
Ichikawa, R., Kasahara, M. and Naito, I.: 1989, An estimation of excess path delay based on JMA Global Analysis Data, Proc. Japanese Symp. GPS.Google Scholar
Sato, K.-H.: 1989, Ionospheric excess path delay correction using GPS dual channel receiver, Proc. Japanese Symp. GPS (1988), 60–65.Google Scholar
Tavella, P., Thomas, C.: 1990a, Metrologia (Submitted).Google Scholar
Tavella, P., Thomas, C.: 1990b, Proc. 4th Europ. Freq. and Time Forum.Google Scholar
Weiss, M., Thomas, C.: 1990, Ann. Rep. BIPM Time Section, 2, D-3 to D-22.Google Scholar
Weiss, M., Weissert, T., Thomas, C., Imae, M., Davies, K.: 1990, Proc. 4th EFTP, Neuchâtel 1990.Google Scholar