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REVIEW 3 major objections 7 minor 105 references

Unlocking the hidden potential of pulsar astronomy

T0 review · 3 major / 7 minor · reviewed 2026-08-07 · deepseek-v4-flash

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Pith's one-line read A roughly 4-meter radio dish with modest bandwidth near 700 MHz could detect many pulsars, localize itself to about 10 kilometers by pulsar navigation, and draw random sequences from scintillation and pulse jitter.

desk verdict Useful review with plausible compact-receiver numbers, but the printed radiometer equation is inverted and the randomness demo is not yet a demonstration. read the letter →

arxiv 2506.08056 v1 pith:N3MMYFD6 submitted 2025-06-09 astro-ph.IM astro-ph.HEastro-ph.SR

D. Kaur , G. Hobbs , A. Zic , J. R. Dawson , J. Morgan , W. Ling , S. Camtepe , J. Pieprzyk
show 1 more author
M. C. M. Cheung
This is my paper · ORCID
classification astro-ph.IMastro-ph.HEastro-ph.SR
keywords pulsarspulsartimingnavigationrandomnumbergenerationscintillationpulsejitterspaceweathercompactradioreceivers
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

The paper argues that pulsars have practical value well beyond fundamental physics, and that this value can be tapped with remarkably small radio hardware. Using the radiometer equation and catalog flux densities, it shows that a roughly four-meter dish with small bandwidth near 700 MHz can detect the Vela pulsar and many other pulsars, and that such a receiver could determine its position to around 10 kilometers by timing millisecond pulsars. It also demonstrates, on real data, that random bit sequences can be extracted from scintillation patterns and from single-pulse timing jitter. If these estimates hold, compact, GNSS-independent navigation and publicly verifiable randomness become engineering targets rather than science fiction.

What carries the argument

The load-bearing object is the radiometer equation, $$S_{\min} = \frac{2k_B T_{\rm sys}}{A_{\rm eff}} \sqrt{\frac{n_p \$\Delta$\nu\, \tau\, \delta}{1-\delta}}\,(S/N),$$ which converts dish diameter, system temperature, bandwidth, and integration time into a minimum detectable pulsed flux density. The paper evaluates this against 700 MHz flux densities drawn from the standard pulsar catalog, with a spectral-index extrapolation from 1400 MHz, and compares the resulting sensitivity with the positions of the Vela pulsar and the brightest millisecond pulsar. For randomness, the operative mechanisms are diffractive scintillation, which produces frequency-time intensity patterns correlated on the diffractive bandwidth scale, and pulse jitter, whose single-pulse timing residuals around a median yield bit sequences; both are demonstrated on archival timing-array data.

What would settle it

Build or simulate a 4 m dish with a 300 K receiver, 10 MHz of bandwidth near 700 MHz, and a 10-minute integration, and count how many catalog pulsars are actually detected at S/N > 8; alternatively, measure 700 MHz pulsed flux densities of the pulsars in the paper's navigation table with a calibrated telescope and compare them with the assumed values. If the detected number is much smaller than predicted, or the arrival-time scatter cannot reach the claimed sub-kilometre to 10 km accuracy, the central claim fails.

Watch

Extended reading notes

Core claim

The central claim is that the same pulsar signals used for gravity tests can serve as infrastructure for navigation, timing, synchronization, space-weather monitoring, and randomness, and that the hardware need not be large. In the paper's calculations, a roughly four-meter dish with about 10 MHz of bandwidth and a 300 K receiver around 700 MHz can detect the Vela pulsar, and a similar system detects many more pulsars when the operating band and system temperature are chosen sensibly; a 256-element array with 64 MHz of bandwidth at 700 MHz and a 60 K system temperature yields one-dimensional positional accuracies as good as a few hundred meters for the best millisecond pulsars. The paper revisits the old argument that radio pulsar navigation requires huge telescopes, countering that dispersion is handled by coherent dedispersion and that compact receivers now make radio navigation comparable to X-ray navigation at lower cost. It further shows, using archival observations, that random sequences can be generated from the diffractive scintillation pattern of one pulsar and from the jitter of another, with verification possible even when telescopes are not exactly time-synchronized.

Load-bearing premise

The counts of detectable pulsars and the 10 km navigation accuracy rely on 700 MHz flux densities obtained by extrapolating 1400 MHz catalog values with a spectral-index assumption that the paper does not state or propagate with uncertainties; if the true 700 MHz fluxes are lower for many pulsars, the compact-receiver performance will not materialize.

Editorial extensions

If this is right

  • A small, low-cost radio receiver could serve as a GNSS-independent navigation and timing source, useful in jamming or spoofing environments and on planets whose atmospheres block X-rays.
  • Radio pulsar navigation would reach accuracy comparable to X-ray systems, roughly 10 km with sub-kilometre potential, using hardware that can be tested end-to-end on Earth.
  • Pulsar-based time synchronization between widely separated sites could be triggered by the same naturally varying pulse train, reducing the need for communication links.
  • Pulsar dispersion and rotation measures measured near the Sun provide model-independent solar-wind and coronal-mass-ejection diagnostics, including simultaneous DM and RM from the same source.
  • Scintillation- and jitter-based random sequences can be publicly verified by independent telescopes, supporting applications from cryptographic beacons to treaty monitoring.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • If the assumed 700 MHz fluxes are confirmed, the same receiver class could be deployed as a distributed network on ships, aircraft, or lunar rovers; the main engineering gap would be real-time coherent dedispersion and scintillation mitigation in a low-power package.
  • The randomness methods differ in geographic reach: scintillation patterns are shared only by closely spaced telescopes, while jitter is broadband and shared over intercontinental baselines, so the choice of source effectively sets the distance scale of the verification network.
  • Archival high-time-resolution pulsar data sets could be reanalysed to measure 700 MHz flux densities directly, turning the paper's extrapolation-based predictions into a cheap empirical test before any hardware is built.
  • Longer integrations and multi-pulsar combinations could plausibly push the localization accuracy below one kilometer, the regime already indicated by one-pulsar timing estimates, but this requires real compact-antenna tests rather than catalog calculations.
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Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, and a circularity audit.

Referee Report

3 major / 7 minor

Summary. The paper is a broad review of non-astronomical applications of pulsars: compact-receiver detection, positioning and navigation, time/frequency transfer, space weather monitoring, random-number generation, large archival data sets for machine learning, calibration, and outreach. It combines a review of prior work with new quantitative estimates: a ~3.8 m dish at 700 MHz should detect Vela at S/N≈8, a ~4 m-class system could detect many pulsars, and a 256-element array could achieve ~10 km self-localization (Table 1). It also presents worked examples of bit sequences derived from scintillation and pulse jitter (Figure 7).

Significance. If the quantitative estimates hold, the paper provides a useful, consolidated assessment of the feasibility of small-scale pulsar systems for practical applications, with concrete, falsifiable predictions (e.g., a 3.8 m dish with a 300 K receiver, 10 MHz bandwidth and 10 min integration should detect Vela at S/N≈8). The central sensitivity calculations use standard radiometer equations and public catalog data rather than fitted parameters, and the data behind the randomness examples are identified in the Data Availability section. The main limitations are that the printed sensitivity equation is inverted relative to the calculations actually used, and the 700 MHz flux densities and their uncertainties are not documented.

major comments (3)
  1. [Section 2, Eq. (1)] Eq. (1) prints sqrt(n_p Δν τ) in the numerator, but the example in the same paragraph (3.8 m dish, T_sys=300 K, Δν=10 MHz, τ=10 min, δ=0.01, S/N=8) yields S_min ≈ 6.4×10^9 Jy if Eq. (1) is used as printed, whereas the text states 540 mJy. The stated value is obtained only if sqrt(n_p Δν τ) is placed in the denominator. Since Figures 2–3 and Table 1 all rely on this equation, the central sensitivity calculation is internally inconsistent as published. Please correct Eq. (1), or explicitly define S_min differently, so that the printed equation reproduces the numerical example.
  2. [Section 3, Table 1; Figures 2–3] The S700 column in Table 1 and the detectability counts in Figure 3 depend on 700 MHz flux densities, but the paper does not state how these values were derived from the ATNF catalog. No spectral-index values, interpolation scheme, or uncertainty propagation are given. Because the detectability and localization claims scale directly with these flux densities, please document the conversion procedure and propagate catalog and spectral-index uncertainties into the quoted counts and Δx values.
  3. [Section 6 / Abstract] The abstract claims that random sequences 'can be produced using the scintillation properties of pulsars as well as from pulse jitter,' but Section 6 presents only a few illustrative bit sequences and explicitly states (footnote 8) that follow-up work is required to determine whether such sequences pass standardized randomness tests. No statistical tests are applied to the new examples. Please either add appropriate randomness tests or revise the 'demonstrate' language to 'illustrate' or 'propose' in both the abstract and the body.
minor comments (7)
  1. [Section 6] The statement that pulsar emissions 'originate millions of light-years away' is incorrect for Galactic pulsars, which are at distances of thousands to tens of thousands of light-years.
  2. [Section 5] The text refers to 'Table 5' when introducing the list of pulsars for space weather studies, but the table is numbered Table 2.
  3. [Figure 6 / Section 5] The Figure 6 caption describes millisecond pulsars as 'blue circles', while Section 5 says they are 'blue squares'; please make the descriptions consistent.
  4. [Tables 1 and 3] Tables 1 and 3 list inconsistent S1400 values for PSR J0437−4715 (364 mJy vs 150 mJy) and PSR J0835−4510 (3100 mJy vs 1050 mJy); please reconcile these values with the catalog.
  5. [Section 6, Figure 7] The description of the bit-extraction algorithm from the dynamic spectrum is not specific enough to reproduce the shown 12-bit sequences; please state exactly how the threshold comparison is applied.
  6. [Abstract] The final sentence of the abstract ends with 'as well as from pulse.' and appears truncated; it should presumably read 'pulse jitter'.
  7. [Section 2] The 'four brightest pulsars' used to set the 540 mJy limiting flux are not named; please identify them so the example is checkable.

Circularity Check

0 steps flagged · score 1.0 of 10

No significant circularity: central sensitivity and navigation estimates are standard radiometer-equation calculations with catalog fluxes, and the randomness demonstrations are data-driven extractions, not fitted predictions.

full rationale

I examined the paper's claimed derivation chain for reductions to its own inputs. The central detectability and localization calculations (Section 2, Figures 2–3, Table 1) use the radiometer equation together with flux densities from the ATNF pulsar catalog; no parameter is fitted to reproduce the claimed minimum dish size, detectable-pulsar counts, or 10 km localization accuracy. The navigation accuracy estimate (Section 3) follows arithmetically from σToA ≈ W50/(2·S/N) with stated assumptions (duty cycle, S/N=8) and catalog-derived 700 MHz fluxes; those fluxes are not tuned to force the 10 km result. The randomness section (Section 6) extracts bit sequences from actual dynamic-spectrum slices and jitter residuals using explicitly stated threshold rules, and the paper itself cautions that 'follow-up work is required to demonstrate whether such sequences would pass standardized randomness tests', so it does not overclaim a validated output. Self-citations appear (e.g., Dawson et al. 2022 for NIST-passing random sequences, Hobbs et al. 2020 for pulsar timescales), but these cite published, peer-reviewed results that are external to the present paper's fitted values; they are not load-bearing in a way that makes the present claims circular. A separate issue: Eq. 1 as printed has sqrt(np Δν τ) in the numerator, whereas the worked 3.8 m example giving 540 mJy requires that factor in the denominator; this is an internal inconsistency (likely a typographical inversion) that affects reproducibility, but it is not a circular reduction of the output to the input. Overall, the paper's predictions do not reduce by construction to fitted parameters or to self-citations, so the circularity score is low.

Assumptions & free parameters 4 free parameters · 5 assumptions · 0 invented entities

The paper's central feasibility estimates rest on standard radio astronomy formulas and catalog data; the main unstated assumption is the spectral index extrapolation to 700 MHz, plus assumed system noise, duty cycle, and detection threshold.

free parameters (4)
  • System temperature Tsys = 30, 60, 120, 300 K
    Assumed values in Figures 2-4 and Table 1; directly set the sensitivity limits and number of detectable pulsars.
  • Detection threshold (S/N) = 8
    Used in Eq. (1) and all sensitivity figures; higher thresholds would reduce the number of detectable pulsars.
  • Pulse duty cycle (delta) = 1% (Figures 2-3) and W50/P = 1/10 (Eq. 3)
    Assumed for detectability and ToA uncertainty estimates; affects S_min linearly.
  • Bandwidth and integration time = 10 MHz/10 min; 64 MHz/1 hr
    Two representative observing setups used in Figures 2-4 and Table 1.
assumptions (5)
  • domain assumption The radiometer equation (Eq. 1) is the correct sensitivity model for pulsed signals.
    Used in Section 2 for all detectability calculations; assumes a specific pulse shape and noise statistics.
  • domain assumption Pulsar flux densities at 700 MHz are obtainable from 1400 MHz catalog values via an assumed spectral index.
    The paper uses ATNF catalog flux densities to predict detectability at 700 MHz (Figure 3), but does not specify the spectral index values or their uncertainties.
  • domain assumption For timing accuracy, pulse profiles are Gaussian with width W50 = P/10.
    Equation (3) derives ToA uncertainty using this shape assumption; real profiles differ, affecting the 10 km localization estimate.
  • domain assumption The ATNF pulsar catalog provides accurate flux densities, periods, and positions.
    All source counts, detectability, and localization estimates rely on catalog values.
  • domain assumption Scintillation patterns are stable over minutes for a given telescope.
    The random sequence extraction from the dynamic spectrum (Fig. 7) assumes a verifying telescope observing a few minutes later sees an almost identical pattern.

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Cite this review

Pith. "Pith review of Unlocking the hidden potential of pulsar astronomy." pith.science (2026). https://pith.science/paper/N3MMYFD6

@misc{pith2026250608056,
  author       = {Pith},
  title        = {Pith review of: Unlocking the hidden potential of pulsar astronomy},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/N3MMYFD6}},
  note         = {Machine review of arXiv:2506.08056}
}
read the original abstract

Pulsars have traditionally been used for research into fundamental physics and astronomy. In this paper, we investigate the expanding applications of radio pulsars in societal and industrial domains beyond their conventional scientific roles. We describe emerging applications in positioning, navigation, timing and synchronization, random number generation, space weather monitoring, public engagement, antenna calibration techniques, and leveraging extensive pulsar data sets generated by large-scale observatories. Such pulsar data sets have already been used to demonstrate quantum-computing algorithms. We evaluate the potential for compact radio receiver systems for pulsar detection by describing optimal observing bands. We show that relatively simple and compact receiver systems can detect the brightest pulsar, Vela. The equivalent of an ~4m-diameter dish with a small bandwidth operating around 700 MHz would be able to detect many more pulsars. Such a detector would be able to localise itself to around 10 km using pulsar navigation techniques. The space weather community requires direct measurements of the integrated electron density at a range of solar elongations. The only method to get model-independent values is through pulsar observations and we explore the possibility of measuring dispersion measures (DMs) and rotation measures with a range of telescopes (observing from low to mid-frequencies) as well as using a typical model to predict the variation of the DM as a function of solar radii. We review how pulsars can be used to produce random sequences and demonstrate that such sequences can be produced using the scintillation properties of pulsars as well as from pulse jitter.

Figures

Figures reproduced from arXiv: 2506.08056 by the authors.

Figure 1
Figure 1. A diagram illustrating an overview of pulsar applications as described [PITH_FULL_IMAGE:figures/full_fig_p002_1.png] view at source ↗
Figure 2
Figure 2. (left) The minimum detectable (i.e. S/N > 8) flux density as a function of antenna diameter for a system with system temperatures of 300 K (blue) 120 K (orange), 60 K (green), and 30 K (red), assuming 10 minutes of integration, a bandwidth of 10 MHz, a 1% duty cycle, and two polarizations. The horizontal lines correspond to the 700 MHz flux densities of PSR J0437−4715 (dash-dotted) and the Vela pulsar (PSR J0835−451… view at source ↗
Figure 3
Figure 3. (left) The number of detectable pulsars for a small parabolic antenna (left) and an aperture array system (right) at 700 MHz, for a range of system temperatures, under the same assumptions as for [PITH_FULL_IMAGE:figures/full_fig_p003_3.png] view at source ↗
Figures from the paper (4 more)
Figure 4
Figure 4. Figure 4: Best-case positional uncertainties achievable with a small-scale radio detector system as a function of detector size, for a range of system temperatures (colours are as in [PITH_FULL_IMAGE:figures/full_fig_p006_4.png]
Figure 5
Figure 5. Figure 5: A typical LDB model integrate along the line of sight to pro￾duce a delta DM as a function of elongation. The upper x-axis shows the solar elongation for a line of sight which reaches the corresponding ‘r’ at the point of closest approach (the pierce point). The delta …
Figure 6
Figure 6. Figure 6: All known pulsars to date are presented by grey dots. The dashed lines present the ± 15 degree from the ecliptic plane. Solid line presents the path followed by the Sun. Bright pulsars with mean flux density >100 mJy are highlighted in red. Blue circles represent milli…
Figure 7
Figure 7. Figure 7: (left) Dynamic spectrum of PSR J1603−7202 observed with the Parkes radio telescope on 2018-06-03 as part of the Parkes Pulsar Timing Array project. The vertical lines indicate slices through the dynamic spectrum used for extracting random number sequences. (right) Timi…

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Reference graph

Works this paper leans on

105 extracted references · 40 canonical work pages

  1. [1]

    G:)PYmPY;5) 2VY ї ?f - | 12 &

    + is cited as + ESG96 +. In connection with cross-referencing and possible future hyperlinking it is not a good idea to collect more that one literature item in one + +. The so-called Harvard or author-year style of referencing is enabled by the package natbib . With this package the literature can be cited as follows: enumerate [ ] Parenthetical: + WB96 ...

    1996

  2. [2]

    write newline

    " write newline "" before.all 'output.state := FUNCTION n.dashify 't := "" t empty not t #1 #1 substring "-" = t #1 #2 substring "--" = not "--" * t #2 global.max substring 't := t #1 #1 substring "-" = "-" * t #2 global.max substring 't := while if t #1 #1 substring * t #2 global.max substring 't := if while FUNCTION word.in bbl.in ":" * " " * FUNCTION f...

  3. [3]

    , author Anumarlapudi , A

    author Agazie , G. , author Anumarlapudi , A. , author Archibald , A.M. , author Arzoumanian , Z. , author Baker , P.T. , author B \'e csy , B. , author Blecha , L. , author Brazier , A. , author Brook , P.R. , author Burke-Spolaor , S. , author Burnette , R. , author Case , R. , author Charisi , M. , author Chatterjee , S. , author Chatziioannou , K. , a...

    arXiv 2023

  4. [4]

    , author Pizzo, V.J

    author Arge, C.N. , author Pizzo, V.J. , year 2000 . title Improvement in the prediction of solar wind conditions using near-real time solar magnetic field updates . journal Journal of Geophysical Research: Space Physics volume 105 , pages 10465--10479 . :https://doi.org/10.1029/1999JA000262

    doi:10.1029/1999ja000262 2000

  5. [5]

    , year 2007

    author Avramenko, A. , year 2007 . title Synchronization on the basis of pulsar time . journal Measurement Techniques volume 50 , pages 725

    2007

  6. [6]

    , author Lorimer , D.R

    author Bates , S.D. , author Lorimer , D.R. , author Verbiest , J.P.W. , year 2013 . title The pulsar spectral index distribution . journal MNRAS volume 431 , pages 1352--1358 . :10.1093/mnras/stt257, http://arxiv.org/abs/1302.2053 arXiv:1302.2053

    arXiv 2013

  7. [7]

    , author Swainston , N.A

    author Bhat , N.D.R. , author Swainston , N.A. , author McSweeney , S.J. , author Xue , M. , author Meyers , B.W. , author Kudale , S. , author Dai , S. , author Tremblay , S.E. , author van Straten , W. , author Shannon , R.M. , author Smith , K.R. , author Sokolowski , M. , author Ord , S.M. , author Sleap , G. , author Williams , A. , author Hancock , ...

    arXiv 2023

  8. [8]

    , author Wayth , R.B

    author Bhat , N.D.R. , author Wayth , R.B. , author Knight , H.S. , author Bowman , J.D. , author Oberoi , D. , author Barnes , D.G. , author Briggs , F.H. , author Cappallo , R.J. , author Herne , D. , author Kocz , J. , author Lonsdale , C.J. , author Lynch , M.J. , author Stansby , B. , author Stevens , J. , author Torr , G. , author Webster , R.L. , a...

    arXiv 2007

Show all 105 references
  1. [9]

    , year 1966

    author Billings , D.E. , year 1966 . title A guide to the solar corona

    1966

  2. [10]

    , author Flisek , P

    author B aszkiewicz , L.P. , author Flisek , P. , author Kotulak , K. , author Krankowski , A. , author Lewandowski , W. , author Kijak , J. , author Fro \'n , A. , year 2020 . title Finding the Ionospheric Fluctuations Reflection in the Pulsar Signals' Characteristics Observe...

    2020 doi

  3. [11]

    , author Tolley , E

    author Brunet , T. , author Tolley , E. , author Corda , S. , author Ilic , R. , author Broekema , P.C. , author Kneib , J.P. , year 2023 . title Quantum Radio Astronomy: Data Encodings and Quantum Image Processing . journal arXiv e-prints , pages arXiv:2310.12084 :10.48550/ar...

    2023 doi arXiv

  4. [12]

    , author Hesselink, H

    author Buist, P. , author Hesselink, H. , author Gibbs, A. , author Keuning, M. , author Gaubitch, N. , author Noroozi, A. , author Bentum, M. , author Verhoeven, C. , author Heusdens, R. , author Fernandes, J. , author Kabakchiev, H. , author Kestil \"a , A. , year 2014 . tit...

    2014

  5. [13]

    , author Popov, M.V

    author Burgin, M.S. , author Popov, M.V. , year 2024 . title Probing the Ionosphere with Pulses from the Pulsar B2016+28 at a Frequency of 324 MHz . journal Astronomy Reports volume 68 , pages 257--267 . https://doi.org/10.1134/S1063772924700276 https://doi.org/10.1134/S106377...

    2024 doi

  6. [14]

    , author Guo , Y.J

    author Caballero , R.N. , author Guo , Y.J. , author Lee , K.J. , author Lazarus , P. , author Champion , D.J. , author Desvignes , G. , author Kramer , M. , author Plant , K. , author Arzoumanian , Z. , author Bailes , M. , author Bassa , C.G. , author Bhat , N.D.R. , author ...

    2018 arXiv

  7. [15]

    , author Flynn , C

    author Campbell-Wilson , D. , author Flynn , C. , author Bateman , T. , year 2024 . title Confirmation of glitch event observed in PSR J0835-4510 (Vela pulsar) . journal The Astronomer's Telegram volume 16610 , pages 1

    2024

  8. [16]

    , author Pass, R

    author Canetti, R. , author Pass, R. , author Shelat, A. , year 2007 . title Cryptography from sunspots: How to use an imperfect reference string , in: booktitle Proceedings of the 48th Annual IEEE Symposium on Foundations of Computer Science , publisher IEEE Computer Society ...

    2007 doi

  9. [17]

    , author Vilmer , N

    author Carley , E.P. , author Vilmer , N. , author Sim \ o es , P.J.A. , author \'O Fearraigh , B. , year 2017 . title Estimation of a coronal mass ejection magnetic field strength using radio observations of gyrosynchrotron radiation . journal AAP volume 608 , pages A137 . :1...

    2017 arXiv

  10. [18]

    , author Hobbs , G.B

    author Champion , D.J. , author Hobbs , G.B. , author Manchester , R.N. , author Edwards , R.T. , author Backer , D.C. , author Bailes , M. , author Bhat , N.D.R. , author Burke-Spolaor , S. , author Coles , W. , author Demorest , P.B. , author Ferdman , R.D. , author Folkner ...

    2010 arXiv

  11. [19]

    , year 2016

    author Chapman E., Grewar J., N.T. , year 2016 . title Celestial sources for random number generation . journal The Proceedings of 14th Australian Information Security Management Conference :10.4225/75/58a6975133e06

    2016 doi

  12. [20]

    , author Zhan, X

    author Chen, M. , author Zhan, X. , author Liu, B. , author Yuan, W. , year 2018 . title Gnss vulnerability network risk assessment and alleviation strategies considering efficiency cost . journal Journal of Aeronautics, Astronautics and Aviation, Series A volume 52 . :10.6125...

    2018 doi

  13. [21]

    , year 2018

    author Chen , P.T. , year 2018 . title Pulsar-Based Navigation and Timing: Analysis and Estimation . Ph.D. thesis. University of California, Los Angeles

    2018

  14. [22]

    , year 1970

    author Craft , Harold Dumont, J. , year 1970 . title Radio Observations of the Pulse Profiles and Dispersion Measures of Twelve Pulsars. Ph.D. thesis. Cornell University, New York

    1970

  15. [23]

    , author Hobbs , G

    author Dawson , J.R. , author Hobbs , G. , author Gao , Y. , author Camtepe , S. , author Pieprzyk , J. , author Feng , Y. , author Tranfa , L. , author Bradbury , S. , author Zhu , W. , author Li , D. , year 2022 . title Physical publicly verifiable randomness from pulsars . ...

    2022

  16. [24]

    , author Hobbs , G

    author Deng , X.P. , author Hobbs , G. , author You , X.P. , author Li , M.T. , author Keith , M.J. , author Shannon , R.M. , author Coles , W. , author Manchester , R.N. , author Zheng , J.H. , author Yu , X.Z. , author Gao , D. , author Wu , X. , author Chen , D. , year 2013...

    2013 arXiv

  17. [25]

    , author Caballero , R.N

    author Desvignes , G. , author Caballero , R.N. , author Lentati , L. , author Verbiest , J.P.W. , author Champion , D.J. , author Stappers , B.W. , author Janssen , G.H. , author Lazarus , P. , author Os owski , S. , author Babak , S. , author Bassa , C.G. , author Brem , P. ...

    2016 arXiv

  18. [26]

    , author Arumugam , P

    author EPTA Collaboration , author InPTA Collaboration , author Antoniadis , J. , author Arumugam , P. , author Arumugam , S. , author Babak , S. , author Bagchi , M. , author Bak Nielsen , A.S. , author Bassa , C.G. , author Bathula , A. , author Berthereau , A. , author Bone...

    2023 arXiv

  19. [27]

    , author Hollow , R

    author Fitzgerald , M.T. , author Hollow , R. , author Rebull , L.M. , author Danaia , L. , author McKinnon , D.H. , year 2014 . title A Review of High School Level Astronomy Student Research Projects Over the Last Two Decades . journal PASA volume 31 , pages e037 . :10.1017/p...

    2014 arXiv

  20. [28]

    , author Melatos , A

    author Fulgenzi , W. , author Melatos , A. , author Hughes , B.D. , year 2017 . title Radio pulsar glitches as a state-dependent Poisson process . journal MNRAS volume 470 , pages 4307--4329 . :10.1093/mnras/stx1353

    2017 doi

  21. [29]

    , author Serylak , M

    author Geyer , M. , author Serylak , M. , author Abbate , F. , author Bailes , M. , author Buchner , S. , author Chilufya , J. , author Johnston , S. , author Karastergiou , A. , author Main , R. , author van Straten , W. , author Shamohammadi , M. , year 2021 . title The Thou...

    2021 arXiv

  22. [30]

    , author Li , G.Y

    author Guo , Y.J. , author Li , G.Y. , author Lee , K.J. , author Caballero , R.N. , year 2019 . title Studying the Solar system dynamics using pulsar timing arrays and the LINIMOSS dynamical model . journal MNRAS volume 489 , pages 5573--5581 . :10.1093/mnras/stz2515, http://...

    2019 arXiv

  23. [31]

    , author Wang , J

    author Han , W. , author Wang , J. , author Wang , N. , author Sun , G. , author He , D. , year 2020 . title A method of ground target positioning by observing radio pulsars . journal Experimental Astronomy volume 49 , pages 43--60 . :10.1007/s10686-020-09651-2

    2020 doi

  24. [32]

    , author Dennison , P.A

    author Hewish , A. , author Dennison , P.A. , year 1967 . title Measurements of the Solar Wind and the Small-Scale Structure of the Interplanetary Medium . journal Journal of Geophysical Research volume 72 , pages 1977 . :10.1029/JZ072i007p01977

    1967 doi

  25. [34]

    , author Guo , L

    author Hobbs , G. , author Guo , L. , author Caballero , R.N. , author Coles , W. , author Lee , K.J. , author Manchester , R.N. , author Reardon , D.J. , author Matsakis , D. , author Tong , M.L. , author Arzoumanian , Z. , author Bailes , M. , author Bassa , C.G. , author Bh...

    2020 arXiv

  26. [35]

    , author Hollow , R

    author Hobbs , G. , author Hollow , R. , author Champion , D. , author Khoo , J. , author Yardley , D. , author Carr , M. , author Keith , M. , author Jenet , F. , author Amy , S. , author Burgay , M. , author Burke-Spolaor , S. , author Chapman , J. , author Danaia , L. , aut...

    2009 arXiv

  27. [36]

    , author Manchester, R.N

    author Hobbs, G. , author Manchester, R.N. , author Dunning, A. , author Jameson, A. , author Roberts, P. , author George, D. , author Green, J.A. , author Tuthill, J. , author Toomey, L. , author Kaczmarek, J.F. , author Mader, S. , author Marquarding, M. , author Ahmed, A. ,...

    2020

  28. [37]

    , author Miller , D

    author Hobbs , G. , author Miller , D. , author Manchester , R.N. , author Dempsey , J. , author Chapman , J.M. , author Khoo , J. , author Applegate , J. , author Bailes , M. , author Bhat , N.D.R. , author Bridle , R. , author Borg , A. , author Brown , A. , author Burnett ,...

    2011 arXiv

  29. [38]

    , author Edwards , R.T

    author Hobbs , G.B. , author Edwards , R.T. , author Manchester , R.N. , year 2006 . title TEMPO2, a new pulsar-timing package - I. An overview . journal MNRAS volume 369 , pages 655--672 . :10.1111/j.1365-2966.2006.10302.x, http://arxiv.org/abs/astro-ph/0603381 arXiv:astro-ph/0603381

    2006

  30. [39]

    , author Park , W

    author Hong , J.H. , author Park , W. , author Ryoo , C. , year 2021 . title An Autonomous Space Navigation System Using Image Sensors. journal Int. J. Control Autom. Syst. volume 19 , pages 2122–2133

    2021

  31. [40]

    , author Stovall , K

    author Howard , T.A. , author Stovall , K. , author Dowell , J. , author Taylor , G.B. , author White , S.M. , year 2016 . title Measuring the Magnetic Field of Coronal Mass Ejections Near the Sun Using Pulsars . journal APJ volume 831 , pages 208 . :10.3847/0004-637X/831/2/208

    2016 doi

  32. [41]

    , year 1974

    author Hurd , W.J. , year 1974 . title An Analysis and Demonstration of Clock Synchronization by VLBI . journal IEEE Transactions on Instrumentation Measurement volume 23 , pages 80--89 . :10.1109/TIM.1974.4314222

    1974

  33. [42]

    , author Basalaeva , M.Y

    author Kazantsev , A.N. , author Basalaeva , M.Y. , year 2022 . title Low-frequency observations of giant pulses from ordinary pulsars . journal MNRAS volume 513 , pages 4332--4340 . :10.1093/mnras/stac473

    2022 doi

  34. [43]

    , author Ascione , M.L

    author Kooi , J.E. , author Ascione , M.L. , author Reyes-Rosa , L.V. , author Rier , S.K. , author Ashas , M. , year 2021 . title VLA Measurements of Faraday Rotation Through a Coronal Mass Ejection Using Multiple Lines of Sight . journal Solar Physics volume 296 , pages 11 ....

    2021 doi

  35. [44]

    , author Wexler , D.B

    author Kooi , J.E. , author Wexler , D.B. , author Jensen , E.A. , author Kenny , M.N. , author Nieves-Chinchilla , T. , author Wilson , Lynn B., I. , author Wood , B.E. , author Jian , L.K. , author Fung , S.F. , author Pevtsov , A. , author Gopalswamy , N. , author Mancheste...

    2022

  36. [45]

    , author Utting , A

    author Kordzanganeh , M. , author Utting , A. , author Scaife , A. , year 2021 . title Quantum Machine Learning for Radio Astronomy . journal arXiv e-prints , pages arXiv:2112.02655 :10.48550/arXiv.2112.02655, http://arxiv.org/abs/2112.02655 arXiv:2112.02655

    2021 doi arXiv

  37. [46]

    , author Stairs , I.H

    author Kramer , M. , author Stairs , I.H. , author Manchester , R.N. , author Wex , N. , author Deller , A.T. , author Coles , W.A. , author Ali , M. , author Burgay , M. , author Camilo , F. , author Cognard , I. , author Damour , T. , author Desvignes , G. , author Ferdman ,...

    2021

  38. [47]

    , author Andrew , S

    author Lanman , A.E. , author Andrew , S. , author Lazda , M. , author Shah , V. , author Amiri , M. , author Balasubramanian , A. , author Bandura , K. , author Boyle , P.J. , author Brar , C. , author Carlson , M. , author Cliche , J.F. , author Gusinskaia , N. , author Hend...

    2024 doi arXiv

  39. [48]

    , author Dulk , G.A

    author Leblanc , Y. , author Dulk , G.A. , author Bougeret , J.L. , year 1998 . title Tracing the Electron Density from the Corona to 1 au . journal Solar Physics volume 183 , pages 165--180 . :10.1023/A:1005049730506

    1998 doi

  40. [49]

    , author Cleaver , G.B

    author Lee , J.S. , author Cleaver , G.B. , year 2015 . title The Cosmic Microwave Background Radiation Power Spectrum as a Random Bit Generator for Symmetric and Asymmetric-Key Cryptography . journal arXiv e-prints , pages arXiv:1511.02511 :10.48550/arXiv.1511.02511, http://a...

    2015 doi arXiv

  41. [50]

    , author Young , A

    author Liu , K. , author Young , A. , author Wharton , R. , author Blackburn , L. , author Cappallo , R. , author Chatterjee , S. , author Cordes , J.M. , author Crew , G.B. , author Desvignes , G. , author Doeleman , S.S. , author Eatough , R.P. , author Falcke , H. , author ...

    2019 arXiv

  42. [51]

    , author Zhu , Z

    author Liu , N. , author Zhu , Z. , author Antoniadis , J. , author Liu , J.C. , author Zhang , H. , author Jiang , N. , year 2022 a. title Comparison of dynamical and kinematic reference frames via pulsar positions from timing, Gaia, and interferometric astrometry . journal a...

    2022 doi arXiv

  43. [52]

    , author Verbiest , J.P.W

    author Liu , Y. , author Verbiest , J.P.W. , author Main , R.A. , author Wu , Z. , author Ambalappat , K.M. , author Champion , D.J. , author Cognard , I. , author Guillemot , L. , author Gaikwad , M. , author Janssen , G.H. , author Kramer , M. , author Keith , M.J. , author ...

    2022 arXiv

  44. [53]

    , author Kramer , M

    author Lorimer , D.R. , author Kramer , M. , year 2012 . title Handbook of Pulsar Astronomy

    2012

  45. [54]

    , author Chatterjee , S

    author Madison , D.R. , author Chatterjee , S. , author Cordes , J.M. , year 2013 . title The Benefits of VLBI Astrometry to Pulsar Timing Array Searches for Gravitational Radiation . journal APJ volume 777 , pages 104 . :10.1088/0004-637X/777/2/104, http://arxiv.org/abs/1210....

    2013 arXiv

  46. [55]

    , author Cordes , J.M

    author Madison , D.R. , author Cordes , J.M. , author Arzoumanian , Z. , author Chatterjee , S. , author Crowter , K. , author DeCesar , M.E. , author Demorest , P.B. , author Dolch , T. , author Ellis , J.A. , author Ferdman , R.D. , author Ferrara , E.C. , author Fonseca , E...

    2019 arXiv

  47. [56]

    , author Alielden , K

    author Mahrous , A. , author Alielden , K. , author Vr s nak , B. , author Youssef , M. , year 2018 . title Type II solar radio burst band-splitting: Measure of coronal magnetic field strength . journal Journal of Atmospheric and Solar-Terrestrial Physics volume 172 , pages 75...

    2018 doi

  48. [57]

    , year 2017

    author Manchester , R.N. , year 2017 . title Millisecond Pulsars, their Evolution and Applications . journal Journal of Astrophysics and Astronomy volume 38 , pages 42 . :10.1007/s12036-017-9469-2, http://arxiv.org/abs/1709.09434 arXiv:1709.09434

    2017 arXiv

  49. [58]

    , author Hobbs , G.B

    author Manchester , R.N. , author Hobbs , G.B. , author Teoh , A. , author Hobbs , M. , year 2005 . title The Australia Telescope National Facility Pulsar Catalogue . journal AJ volume 129 , pages 1993--2006 . :10.1086/428488, http://arxiv.org/abs/astro-ph/0412641 arXiv:astro-...

    2005 arXiv

  50. [59]

    , year 2012

    author Manoharan, P.K. , year 2012 . title Three-dimensional evolution of solar wind during solar cycles 22–24 . journal The Astrophysical Journal volume 751 , pages 128 . https://dx.doi.org/10.1088/0004-637X/751/2/128, :10.1088/0004-637X/751/2/128

    2012 doi

  51. [60]

    , author Shannon , R.M

    author Miles , M.T. , author Shannon , R.M. , author Bailes , M. , author Reardon , D.J. , author Keith , M.J. , author Cameron , A.D. , author Parthasarathy , A. , author Shamohammadi , M. , author Spiewak , R. , author van Straten , W. , author Buchner , S. , author Camilo ,...

    2023 arXiv

  52. [61]

    , author Jenet , F.A

    author Miller , A.F. , author Jenet , F.A. , author Zermeno , A. , author Stovall , K. , year 2009 . title The Arecibo Remote Command Center: Creating an Inspiring Environment for Astrophysics , in: booktitle American Astronomical Society Meeting Abstracts \#213 , p. pages 431.04

    2009

  53. [62]

    , author Chhetri , R

    author Morgan , J.S. , author Chhetri , R. , author Ekers , R. , year 2022 . title A census of compact sources at 162 MHz: First data release from the MWA Phase II IPS Survey . journal PASA volume 39 , pages e063 . :10.1017/pasa.2022.56, http://arxiv.org/abs/2210.05400 arXiv:2...

    2022 arXiv

  54. [63]

    , year 1992

    author Narayan , R. , year 1992 . title The Physics of Pulsar Scintillation . journal Philosophical Transactions of the Royal Society of London Series A volume 341 , pages 151--165 . :10.1098/rsta.1992.0090

    1992

  55. [64]

    , author Lonsdale , C.J

    author Oberoi , D. , author Lonsdale , C.J. , year 2012 . title Media responsible for Faraday rotation: A review . journal Radio Science volume 47 , pages RS0K08 . :10.1029/2012RS004992

    2012 doi

  56. [65]

    , author Vourlidas, A

    author Ontiveros, V. , author Vourlidas, A. , year 2009 . title Quantitative measurements of coronal mass ejection-driven shocks from lasco observations . journal The Astrophysical Journal volume 693 , pages 267 . https://dx.doi.org/10.1088/0004-637X/693/1/267, :10.1088/0004-6...

    2009 doi

  57. [66]

    , author Chang, T.C

    author Paciga, G. , author Chang, T.C. , author Gupta, Y. , author Nityanada, R. , author Odegova, J. , author Pen, U.L. , author Peterson, J.B. , author Roy, J. , author Sigurdson, K. , year 2011 . title The GMRT Epoch of Reionization experiment: a new upper limit on the neut...

    2011

  58. [67]

    , author Holmes , R.M

    author Palmer , D.M. , author Holmes , R.M. , year 2018 . title ELROI: A License Plate For Your Satellite . journal arXiv e-prints , pages arXiv:1802.04820 :10.48550/arXiv.1802.04820, http://arxiv.org/abs/1802.04820 arXiv:1802.04820

    2018 doi arXiv

  59. [68]

    , author Bailes , M

    author Parthasarathy , A. , author Bailes , M. , author Shannon , R.M. , author van Straten , W. , author Os owski , S. , author Johnston , S. , author Spiewak , R. , author Reardon , D.J. , author Kramer , M. , author Venkatraman Krishnan , V. , author Pennucci , T.T. , autho...

    2021 arXiv

  60. [69]

    , author Majid , W.A

    author Pearlman , A.B. , author Majid , W.A. , author Prince , T.A. , year 2019 . title Observations of Radio Magnetars with the Deep Space Network . journal Advances in Astronomy volume 2019 , pages 6325183 . :10.1155/2019/6325183, http://arxiv.org/abs/1902.10712 arXiv:1902.10712

    2019 arXiv

  61. [70]

    , author Bulmer , M

    author Pimbblet , K.A. , author Bulmer , M. , year 2005 . title Random Numbers from Astronomical Imaging . journal PASA volume 22 , pages 1--5 . :10.1071/AS04043, http://arxiv.org/abs/astro-ph/0408281 arXiv:astro-ph/0408281

    2005 arXiv

  62. [71]

    , author Yin, H

    author Qiu, W. , author Yin, H. , author Zhang, L. , author Luo, X. , author Wang, W. , author Liu, Y. , author Yao, W. , author Zhan, L. , author Fuhr, P.L. , author King, T.J. , year 2021 . title Pulsar based timing for grid synchronization . journal IEEE Transactions on Ind...

    2021

  63. [72]

    , author Wood , K.S

    author Ray , P.S. , author Wood , K.S. , author Wolff , M.T. , year 2017 . title Characterization of Pulsar Sources for X-ray Navigation . journal arXiv e-prints , pages arXiv:1711.08507 http://arxiv.org/abs/1711.08507 arXiv:1711.08507

    2017 arXiv

  64. [73]

    , author Zic , A

    author Reardon , D.J. , author Zic , A. , author Shannon , R.M. , author Di Marco , V. , author Hobbs , G.B. , author Kapur , A. , author Lower , M.E. , author Mandow , R. , author Middleton , H. , author Miles , M.T. , author Rogers , A.F. , author Askew , J. , author Bailes ...

    2023 arXiv

  65. [74]

    , author Rankin , J.M

    author Redman , S.L. , author Rankin , J.M. , year 2009 . title On the randomness of pulsar nulls . journal MNRAS volume 395 , pages 1529--1532 . :10.1111/j.1365-2966.2009.14632.x

    2009

  66. [75]

    , author Mendonca, F.A

    author Rocha, B.S. , author Mendonca, F.A. , author Ramos, R.V. , year 2022 . title An algorithm to decrease the key distribution error rate using pulsars , in: booktitle 2022 Workshop on Communication Networks and Power Systems (WCNPS) , pp. pages 1--5 . :10.1109/WCNPS56355.2...

    2022

  67. [76]

    , author Swiggum , J

    author Rosen , R. , author Swiggum , J. , author McLaughlin , M.A. , author Lorimer , D.R. , author Yun , M. , author Heatherly , S.A. , author Boyles , J. , author Lynch , R. , author Kondratiev , V.I. , author Scoles , S. , author Ransom , S.M. , author Moniot , M.L. , autho...

    2013 arXiv

  68. [77]

    , author Salzman Sagan , L

    author Sagan , C. , author Salzman Sagan , L. , author Drake , F. , year 1972 . title A Message from Earth . journal Science volume 175 , pages 881--884 . :10.1126/science.175.4024.881

    1972 doi

  69. [78]

    , author Reynolds , J.E

    author Sarkissian , J.M. , author Reynolds , J.E. , author Hobbs , G. , author Harvey-Smith , L. , year 2017 . title One Year of Monitoring the Vela Pulsar Using a Phased Array Feed . journal PASA volume 34 , pages e027 . :10.1017/pasa.2017.19, http://arxiv.org/abs/1705.08355 ...

    2017 arXiv

  70. [79]

    , author Radke, K

    author Schmidt, D. , author Radke, K. , author Camtepe, S. , author Foo, E. , author Ren, M. , year 2016 . title A survey and analysis of the gnss spoofing threat and countermeasures . journal ACM Comput. Surv. volume 48 . https://doi.org/10.1145/2897166, :10.1145/2897166

    2016 doi

  71. [80]

    , author Kauristie , K

    author Schrijver , C.J. , author Kauristie , K. , author Aylward , A.D. , author Denardini , C.M. , author Gibson , S.E. , author Glover , A. , author Gopalswamy , N. , author Grande , M. , author Hapgood , M. , author Heynderickx , D. , author Jakowski , N. , author Kalegaev ...

    2015 arXiv

  72. [81]

    , author Pant, V

    author Sheoran, J. , author Pant, V. , author Patel, R. , author Banerjee, D. , year 2023 . title Evolution of the thermodynamic properties of a coronal mass ejection in the inner corona . journal Frontiers in Astronomy and Space Sciences volume 10 . https://www.frontiersin.or...

    2023

  73. [82]

    , author Singh, J

    author Singh, S. , author Singh, J. , author Singh, S. , author Goyal, S.B. , author Raboaca, M.S. , author Verma, C. , author Suciu, G. , year 2022 . title Detection and mitigation of gnss spoofing attacks in maritime environments using a genetic algorithm . journal Mathemati...

    2022 doi

  74. [83]

    , author Lourens , M

    author Slabbert , D. , author Lourens , M. , author Petruccione , F. , year 2023 . title Pulsar Classification: Comparing Quantum Convolutional Neural Networks and Quantum Support Vector Machines . journal arXiv e-prints , pages arXiv:2309.15592 :10.48550/arXiv.2309.15592, htt...

    2023 doi arXiv

  75. [84]

    , author Flynn , C

    author Spiewak , R. , author Flynn , C. , author Johnston , S. , author Keane , E.F. , author Bailes , M. , author Barr , E.D. , author Bhandari , S. , author Burgay , M. , author Jankowski , F. , author Kramer , M. , author Morello , V. , author Possenti , A. , author Venkatr...

    2020 arXiv

  76. [85]

    , year 2016

    author Sreeja , V. , year 2016 . title Impact and mitigation of space weather effects on GNSS receiver performance . journal Geoscience Letters volume 3 , pages 24 . :10.1186/s40562-016-0057-0

    2016 doi

  77. [86]

    , year 1969

    author Staelin , D.H. , year 1969 . title Fast folding algorithm for detection of periodic pulse trains. journal IEEE Proceedings volume 57 , pages 724--725 . :10.1109/PROC.1969.7051

    1969

  78. [87]

    , author Azou , S

    author Stanciu , M.I. , author Azou , S. , author Serbanescu , A. , year 2011 . title On the Blind Estimation of Chip Time of Time-Hopping Signals Through Minimization of a Multimodal Cost Function . journal IEEE Transactions on Signal Processing volume 59 , pages 842--847 . :...

    2011

  79. [88]

    u nsem \

    author Tiburzi , C. , author Shaifullah , G.M. , author Bassa , C.G. , author Zucca , P. , author Verbiest , J.P.W. , author Porayko , N.K. , author van der Wateren , E. , author Fallows , R.A. , author Main , R.A. , author Janssen , G.H. , author Anderson , J.M. , author Bak ...

    2021 arXiv

  80. [89]

    u nsem \

    author Tiburzi , C. , author Verbiest , J.P.W. , author Shaifullah , G.M. , author Janssen , G.H. , author Anderson , J.M. , author Horneffer , A. , author K \"u nsem \"o ller , J. , author Os owski , S. , author Donner , J.Y. , author Kramer , M. , author Kumari , A. , author...

    2019 arXiv

  81. [90]

    , author Goeke , R

    author Tingay , S.J. , author Goeke , R. , author Bowman , J.D. , author Emrich , D. , author Ord , S.M. , author Mitchell , D.A. , author Morales , M.F. , author Booler , T. , author Crosse , B. , author Wayth , R.B. , author Lonsdale , C.J. , author Tremblay , S. , author Pa...

    2013 arXiv

  82. [91]

    , author Tawara , K

    author Tokumaru , M. , author Tawara , K. , author Takefuji , K. , author Sekido , M. , author Terasawa , T. , year 2020 . title Radio Sounding Measurements of the Solar Corona Using Giant Pulses of the Crab Pulsar in 2018 . journal Solar Physics volume 295 , pages 80 . :10.10...

    2020 doi

  83. [92]

    , author Desvignes , G

    author Torne , P. , author Desvignes , G. , author Eatough , R.P. , author Karuppusamy , R. , author Paubert , G. , author Kramer , M. , author Cognard , I. , author Champion , D.J. , author Spitler , L.G. , year 2017 . title Detection of the magnetar SGR J1745-2900 up to 291 ...

    2017 arXiv

  84. [93]

    , author Brenkle, J.P

    author Tyler, G.L. , author Brenkle, J.P. , author Komarek, T.A. , author Zygielbaum, A.I. , year 1977 . title The viking solar corona experiment . journal Journal of Geophysical Research (1896-1977) volume 82 , pages 4335--4340 . :https://doi.org/10.1029/JS082i028p04335

    1977 doi

  85. [94]

    o randel , J. , author Koopmans , L.V.E. , author Mann , G. , author Miley , G. , author R \

    author van Haarlem , M.P. , author Wise , M.W. , author Gunst , A.W. , author Heald , G. , author McKean , J.P. , author Hessels , J.W.T. , author de Bruyn , A.G. , author Nijboer , R. , author Swinbank , J. , author Fallows , R. , author Brentjens , M. , author Nelles , A. , ...

    2013 arXiv

  86. [95]

    , year 2013

    author van Straten , W. , year 2013 . title High-fidelity Radio Astronomical Polarimetry Using a Millisecond Pulsar as a Polarized Reference Source . journal APJs volume 204 , pages 13 . :10.1088/0067-0049/204/1/13, http://arxiv.org/abs/1212.3446 arXiv:1212.3446

    2013 arXiv

  87. [96]

    , author Demorest , P.B

    author Walker , M.A. , author Demorest , P.B. , author van Straten , W. , year 2013 . title Cyclic Spectroscopy of The Millisecond Pulsar, B1937+21 . journal APJ volume 779 , pages 99 . :10.1088/0004-637X/779/2/99, http://arxiv.org/abs/1310.3535 arXiv:1310.3535

    2013 arXiv

  88. [97]

    , author Shaifullah , G.M

    author Wang , J. , author Shaifullah , G.M. , author Verbiest , J.P.W. , author Tiburzi , C. , author Champion , D.J. , author Cognard , I. , author Gaikwad , M. , author Graikou , E. , author Guillemot , L. , author Hu , H. , author Karuppusamy , R. , author Keith , M.J. , au...

    2022 arXiv

  89. [98]

    , author Coles , W.A

    author Wang , J.B. , author Coles , W.A. , author Hobbs , G. , author Shannon , R.M. , author Manchester , R.N. , author Kerr , M. , author Yuan , J.P. , author Wang , N. , author Bailes , M. , author Bhat , N.D.R. , author Dai , S. , author Dempsey , J. , author Keith , M.J. ...

    2017 arXiv

  90. [99]

    title Comparison of vlbi and gnss common view for time transfer

    author Wang, Pingli , author Wang, Guangli , author Gao, Yuping , author Cai, Hongbing , author Liu, Na , year 2019 . title Comparison of vlbi and gnss common view for time transfer . journal Int. J. Metrol. Qual. Eng. volume 10 , pages 15 . https://doi.org/10.1051/ijmqe/20190...

    2019

  91. [100]

    , author Tingay , S.J

    author Wayth , R.B. , author Tingay , S.J. , author Trott , C.M. , author Emrich , D. , author Johnston-Hollitt , M. , author McKinley , B. , author Gaensler , B.M. , author Beardsley , A.P. , author Booler , T. , author Crosse , B. , author Franzen , T.M.O. , author Horsley ,...

    2018 arXiv

  92. [101]

    , author Chen, S

    author Xu, H. , author Chen, S. , author Guo, Y. , author Jiang, J. , author Wang, B. , author Xu, J. , author Xue, Z. , author Caballero, R.N. , author Yuan, J. , author Xu, Y. , author Wang, J. , author Hao, L. , author Luo, J. , author Lee, K. , author Han, J. , author Jian...

    2023

  93. [102]

    , author Shi , Y

    author Xue , M. , author Shi , Y. , author Guo , Y. , author Huang , N. , author Peng , D. , author Luo , J. , author Shentu , H. , author Chen , Z. , year 2019 . title X-Ray Pulsar-Based Navigation Considering Spacecraft Orbital Motion and Systematic Biases . journal Sensors ...

    2019 doi

  94. [103]

    , author Coles , W.A

    author You , X.P. , author Coles , W.A. , author Hobbs , G.B. , author Manchester , R.N. , year 2012 . title Measurement of the electron density and magnetic field of the solar wind using millisecond pulsars . journal MNRAS volume 422 , pages 1160--1165 . :10.1111/j.1365-2966....

    2012

  95. [104]

    , author Hobbs, G.B

    author You, X.P. , author Hobbs, G.B. , author Coles, W.A. , author Manchester, R.N. , author Han, J.L. , year 2007 . title An improved solar wind electron density model for pulsar timing . journal The Astrophysical Journal volume 671 , pages 907 . https://dx.doi.org/10.1086/5...

    2007 doi

  96. [105]

    , author Zhang , S.N

    author Zheng , S.J. , author Zhang , S.N. , author Lu , F.J. , author Wang , W.B. , author Gao , Y. , author Li , T.P. , author Song , L.M. , author Ge , M.Y. , author Han , D.W. , author Chen , Y. , author Xu , Y.P. , author Cao , X.L. , author Liu , C.Z. , author Zhang , S. ...

    2019

  97. [106]

    , author Yermolaev , Y.I

    author Zhuravlev , V.I. , author Yermolaev , Y.I. , author Andrianov , A.S. , year 2020 . title Probing the ionosphere by the pulsar B0950+08 with help of RadioAstron ground-space baselines . journal MNRAS volume 491 , pages 5843--5851 . :10.1093/mnras/stz3370, http://arxiv.or...

    2020 arXiv

Pith tools

Reviewed August 7, 2026 · model on record in the stance chip above.