2024MNRAS.529.1082Z


Query : 2024MNRAS.529.1082Z

2024MNRAS.529.1082Z - Mon. Not. R. Astron. Soc., 529, 1082-1090 (2024/April-1)

Research on establishing a joint time-scale of pulsar time and atomic time based on a wavelet analysis method.

ZHU X., ZHANG Z., ZHAO C., LI B., TONG M., GAO Y. and YANG T.

Abstract (from CDS):

Pulsar time has different physical mechanisms from atomic time, and these two time-scales are complementary in terms of stability performance. The joint timekeeping of pulsar and atomic time is currently an important application direction. Our research utilizes a wavelet analysis method to perform multiscale analysis of time signals in both the time and frequency domains, and assigns corresponding weights to different frequency bands for synthesis, which solves the problem of balancing long- and short-term stability in unified weighted synthesis. In this paper, a joint time-scale APT (atomic pulsar time) is obtained by a fusion of pulsar ensemble time (EPT) and atomic time TA(NTSC) (AT) based on wavelet analysis. The results show that APT effectively integrates the stability advantages of both EPT and AT, and the short-term stability of APT at 0.4 yr is consistent with that of AT, reaching 5.6 × 10–15 as evaluated by σz variance. The stability of APT remains consistent with EPT after 3.2 yr, and the long-term stability at 13.1 yr is close to 1.3 × 10–16, perfectly retaining the excellent long-term stability characteristics of pulsar time. The root mean square of APT's clock difference relative to TT(BIPM) is much lower than that of TA(NTSC). Moreover, we propose ways to improve the stability of APT through experimental comparisons. The results indicate that APT has the potential to serve as a reference for steering UTC(NTSC) in the future, improving the long-term timekeeping capability of local atomic time in China, thereby comprehensively improving the stability and reliability of China's time reference.

Abstract Copyright: © 2024 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.

Journal keyword(s): time - (stars:) pulsars: general - methods: data analysis

Simbad objects: 16

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Number of rows : 16
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 PSR J0437-47 Psr 04 37 15.7994581776 -47 15 08.544351636           DC 1032 0
2 PSR J0712-68 Psr 07 11 54.153093 -68 30 47.23387           ~ 120 1
3 PSR J0751+1807 Psr 07 51 09.1539 +18 07 38.335           ~ 316 1
4 PSR J1012+5307 Psr 10 12 33.4345449600 +53 07 02.548542576     19.5     DA 419 1
5 PSR J1022+10 Psr 10 22 57.990 +10 01 52.92           ~ 279 2
6 PSR J1045-45 Psr 10 45 50.179671 -45 09 54.05686           ~ 154 1
7 PSR J1604-72 Psr 16 03 35.670781 -72 02 32.82328           ~ 142 0
8 PSR J1640+2224 Psr 16 40 16.744850 +22 24 08.84119           ~ 210 0
9 PSR J1643-1224 Psr 16 43 38.16612 -12 24 58.6334           ~ 260 2
10 PSR J1713+0747 Psr 17 13 49.5367813 +07 47 37.450240           ~ 530 1
11 PSR J1730-2304 Psr 17 30 21.68471 -23 04 31.2590           ~ 194 1
12 PSR J1744-1134 Psr 17 44 29.4220844 -11 34 54.801320           ~ 323 1
13 PSR B1855+09 Psr 18 57 36.390620 +09 43 17.20712           DA 569 1
14 PSR J2124-3358 Psr 21 24 43.834930 -33 58 45.49195           ~ 337 1
15 PSR J2129-5718 Psr 21 29 22.781548 -57 21 14.33356           ~ 122 1
16 PSR B2145-07.8 Psr 21 45 50.45590 -07 50 18.5900           ~ 336 0

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