There is a newer version of the record available.

Published September 14, 2021 | Version v1
Preprint Open

Magnetar-type bursting evolution of Jupiter global magnetoactivity since 1996

Authors/Creators

  • 1. Journal of Geophysics

Description

The decade-scale evolution profile of short-burst pulses, observed previously in 4U 0142+61, emerges from mean spectra of mission-integrated Galileo–Cassini–Juno 1996-2020 annual orbiting samplings of Jupiter ⪅8nT global magnetic field. The profile is obtained by temporally mapping hyperlow-frequency (<1μHz) dynamics of the magnetospheric signature of solar wind’s Rieger-resonance perturbations in ~0.2–2 zeV, here used as a proxy of magnetoactivity. The 1–6 month (385.8–64.3 nHz) mechanical resonance of solar wind is impressed onto the Jovian magnetosphere entirely and encompassed the Rieger period PRg = 154 days and first six harmonics: 5/6 PRg, 2/3 PRg, 1/2 PRg, 1/3 PRg, 1/4 PRg, 1/5 PRg.  Statistical fidelity of spectral peaks stayed well within a very high (Φ≫12) range, 107–105, reflecting the imprint’s completeness and incessantness. The magnetoactivity upsurge from the means that reach a high ~20% field variance began reformatting the signature around 1999, gradually transforming it into an anomalous state by 2002, also indicated from the anisotropic splitting of spectral peaks. In contrast, a comparison against 2005-2016 Cassini global samplings of Saturn revealed a calm Saturnian magnetoactivity, at a low ⪅1% field variance except for every ~7.3 yr when it is ⪅5% due to orbital-tidal forcing.  Because the change in annual magnetoactivity is becoming more sinusoidal with time, resembling a magnetar bursts evolution profile, the Jupiter upsurge is the greatest possible. This conclusive confirmation of the ongoing Jupiter upsurge and its pulsar-type supports my earlier proposal that an increasing Jovian magnetoactivity facilitates seismicity on magnetically exposed Mars via magnetic reconnecting.  A global pulsation profile of magnetar type in a planet demands beacon orbiter missions to monitor Jupiter magnetoactivity permanently for deciphering the disruption capacity of possible Jovian magnetodipole-discharge jets to electrical grids and communication systems.

Files

Article-repo.pdf

Files (2.9 MB)

Name Size Download all
md5:6be38762830c201705c8e919cd11ef78
1.0 MB Preview Download
md5:a4e05afed5f5e29db32c1bea9367197b
1.8 MB Preview Download

Additional details

References

  • Bai T. and Cliver E. W. (1990) A 154 day periodicity in the occurrence rate of proton flares. Astrophys. J. 363:299-309. https://doi.org/10.1086/169342
  • Cane, H.V., Richardson, I.G., von Rosenvinge, T.T. (1998) Interplanetary magnetic field periodicity of ∼153 days. Geophys. Res. Lett. 25(24):4437-4440. https://doi.org/10.1029/1998GL900208
  • Chancia, R.O., Hedman, M.M., Cowley, S.W.H., Provan, G., Ye, S.-Y. (2019) Seasonal structures in Saturn's dusty Roche Division correspond to periodicities of the planet's magnetosphere. Icarus 330:230-255. https://doi.org/10.1016/j.icarus.2019.04.012
  • Cho, J.-H., Lee, D.-Y., Noh, S.-J., Kim, H., Choi, C.R., Lee, J., Hwang, J., (2017) Spatial dependence of electromagnetic ion cyclotron waves triggered by solar wind dynamic pressure enhancements. J. Geophys. Res. Space Phys. 122, 5502–5518. https://doi.org/10.1002/2016JA023827
  • Dessler, A.J. (1987) Magnetospheric power from planetary spin (p.71). IEEE international conference on plasma science, 1-3 June, Crystal City, VA USA
  • Dougherty, M.K., Kellock, S., Slootweg, A.P., Achilleos, N., Joy, S.P., Mafi, J.N. (2006) Cassini orbiter magnetometer calibrated 1 minute averaged archive v2.0 & v.1.0, CO-E/SW/J/S-MAG-4-SUMM-AVG1MIN-V2.0. NASA Planetary Data System. https://doi.org/10.17189/1519602
  • Dowden, R.L. (1968) A Jupiter Model of Pulsars. Publications of the Astronomical Society of Australia 1(4):159–159. https://doi.org/10.1017/s132335800001122x
  • Gombosi T.I., Armstrong, T.P., Arridge, C.S., Khurana, K.K., Krimigis, S.M., Krupp, N., Persoon, A.M., Thomsen, M.F. (2009) Saturn's Magnetospheric Configuration. In: Dougherty M.K., Esposito L.W., Krimigis S.M. (Eds.) Saturn from Cassini-Huygens. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-9217-6_9
  • Gonzalez, M.E., Dib, R., Kaspi, V.M., Woods, P.M., Tam, C.R., Gavriil, F.P. (2010) Long-term X-ray changes in the emission from the anomalous X-ray pulsar 4U 0142+61. Astrophys. J. 716:1345–1355. https://dx.doi.org/10.1088/0004-637X/716/2/1345
  • Kivelson, M.G., Khurana, K.K., Russell, C.T., Walker, R.J., Joy, S.P., Mafi, J.N. (1997) Galileo orbiter at Jupiter calibrated mag high res v1.0, GO-J-MAG-3-RDR-HIGHRES-V1.0, NASA Planetary Data System. https://doi.org/10.17189/1519667
  • Lou, Y.-Q., Wang, Y.-M., Fan, Z., Wang, S., Wang, J.X. (2003) Periodicities in solar coronal mass ejections. Mon. Not. R. Astron. Soc. 345(3):809–818. https://doi.org/10.1046/j.1365-8711.2003.06993.x
  • Masters, M. (2017) Revealing how the solar wind interacts with Jupiter's magnetosphere. Magnetospheres of the outer planets (MOP), Conference by the Swedish Institute for Space Physics and Royal Institute of Technology, Uppsala Sweden, 12–16 June.
  • Michel, F.C. (1982) Theory of pulsar magnetospheres. Rev. Mod. Phys. 54:1. https://doi.org/10.1103/RevModPhys.54.1
  • Moore, K.M., Yadav, R.K., Kulowski, L., Cao, H., Bloxham, J., Connerney, J.E.P., Kotsiaros, S., Jørgensen, J.L., Merayo, J.M.G., Stevenson, D.J., Bolton, S.J., Levin, S.M. (2018) A complex dynamo inferred from the hemispheric dichotomy of Jupiter's magnetic field. Nature 561:76–78. https://doi.org/10.1038/s41586-018-0468-5
  • Mousis, O., Fletcher, L.N., Lebreton, J.-P., Wurz, P. et al. (2014) Scientific rationale for Saturn׳s in situ exploration. Planet. Space Sci. 104(A):29-47. https://doi.org/10.1016/j.pss.2014.09.014
  • Murakami, G., Yoshioka, K., Kimura, T., Yamazaki, A., Tsuchiya, F., Tao, C., Kita, H., Kagitani, M., Kasaba, Y., Yoshikawa, I., Fujimoto, M. (2017) Response of Jupiter's inner magnetosphere to the solar wind derived from 3-years observation by Hisaki. Magnetospheres of the outer planets (MOP), Conference by the Swedish Institute for Space Physics and Royal Institute of Technology, Uppsala Sweden, 12–16 June.
  • Omerbashich, M. (2021c) External forcing of Moon and Earth seismicity at Rieger periods. In review. https://doi.org/10.5281/zenodo.5069075
  • Omerbashich, M. (2021b) Extramartian forcing of Mars seismicity at Rieger periods. In review. https://doi.org/10.5281/zenodo.4921735
  • Omerbashich, M. (2021a) Non-marine tetrapod extinctions solve extinction periodicity mystery. Hist. Biol. 34 (29 March). https://doi.org/10.1080/08912963.2021.1907367
  • Omerbashich, M. (2009) Method for Measuring Field Dynamics. US Patent #20090192741, US Patent & Trademark Office. https://worldwide.espacenet.com/publicationDetails/biblio?CC=US&NR=2009192741A1
  • Omerbashich, M. (2007) Magnification of mantle resonance as a cause of tectonics. Geodinamica Acta 20:6:369-383. https://doi.org/10.3166/ga.20.369-383
  • Omerbashich, M. (2006) Gauss–Vaníček Spectral Analysis of the Sepkoski Compendium: No New Life Cycles. Comp. Sci. Eng. 8(4):26–30. https://doi.org/10.1109/MCSE.2006.68 (Erratum due to journal error. Comp. Sci. Eng. 9(4):5–6. https://doi.org/10.1109/MCSE.2007.79; full text: https://arxiv.org/abs/math-ph/0608014)
  • Omerbashich, M. (2003) Earth-model Discrimination Method. Ph.D. Dissertation, pp.129. ProQuest, USA. https://doi.org/10.6084/m9.figshare.12847304
  • Pagiatakis, S. (1999) Stochastic significance of peaks in the least-squares spectrum. J. Geod. 73:67-78. https://doi.org/10.1007/s001900050220
  • Pap, J., Tobiska, W.K., Bouwer, S.D. (1990) Periodicities of solar irradiance and solar activity indices, I. Sol. Phys. 129:165–189. https://doi.org/10.1007/BF00154372
  • Pizzocaro, D., Tiengo, A., Mereghetti, S., Turolla, R., Esposito, P., Stella, L., Zane, S., Rea, N., Coti Zelati, F., Israel, G. (2019) Detailed X-ray spectroscopy of the magnetar 1E 2259+586. Astron. Astrophys. 626:A39. https://doi.org/10.1051/0004-6361/201834784
  • Rieger, E., Share, G.H., Forrest, D.J., Kanbach, G., Reppin, C., Chupp, E.L. (1984) A 154-day periodicity in the occurrence of hard solar flares? Nature 312:623–625. https://doi.org/10.1038/312623a0
  • Roussos, E., Krupp, N., Paranicas, C., Kollmann, P., Mitchell, D.G., Krimigis, S.M., Palmaerts, B., Dialynas, K., Jackman, C.M. (2018) Heliospheric conditions at Saturn during Cassini's ring-grazing and proximal orbits. Geophys. Res. Lett. 45:10812–10818. https://doi.org/10.1029/2018GL078093
  • Saur, J., Schreiner, A., Mauk, B.H., Clark, G.B., Kollmann, P. (2017) Wave particle interactions in Jupiter's magnetosphere and associated particle acceleration. Magnetospheres of the outer planets (MOP), Conference by the Swedish Institute for Space Physics and Royal Institute of Technology, Uppsala Sweden, 12–16 June.
  • Simpson, J.F. (1968) Solar activity as a triggering mechanism for earthquakes. Earth Planet. Sci. Lett. 3:417-425. https://doi.org/10.1016/0012-821X(67)90071-4
  • Stallard, T.S., Baines, K.H., Melin, H., Bradley, T.J., Moore, L., O'Donoghue, J., Miller, S., Chowdhury, M.N., Badman, S.V., Allison, H.J., Roussos, E. (2019) Local-time averaged maps of H3+ emission, temperature and ion winds. Phil. Trans. R. Soc. A. 3772018040520180405. https://doi.org/10.1098/rsta.2018.0405
  • Taylor, J., Hamilton, S. (1972) Some tests of the Vaníček Method of spectral analysis. Astrophys. Space Sci. 17:357–367. https://doi.org/10.1007/BF00642907
  • Vaníček, P. (1969) Approximate Spectral Analysis by Least-Squares Fit. Astrophys. Space Sci. 4(4):387–391. https://doi.org/10.1007/BF00651344
  • Vaníček, P. (1971) Further Development and Properties of the Spectral Analysis by Least-Squares Fit. Astrophys. Space Sci. 12(1):10–33. https://doi.org/10.1007/BF00656134
  • Vogt, M.F., Gyalay, S., Kronberg, E.A., Bunce, E.J., Kurth, W.S., Zieger, B., Tao, C. (2019) Solar Wind Interaction With Jupiter's Magnetosphere: A Statistical Study of Galileo In Situ Data and Modeled Upstream Solar Wind Conditions. J. Geophys. Res. Space Phys. 124(12):10170–10199. https://doi.org/10.1029/2019JA026950
  • Wells, D.E., Vaníček, P., Pagiatakis, S. (1985) Least squares spectral analysis revisited. Department of Geodesy & Geomatics Engineering Technical Report 84, University of New Brunswick, Canada. http://www2.unb.ca/gge/Pubs/TR84.pdf
  • Yao, Z., Dunn, W.R., Woodfield, E.E., Clark, G., Mauk, B.H. et al. (2021) Revealing the source of Jupiter's x-ray auroral flares. Sci. Adv. 7:eabf0851. https://doi.org/10.1126/sciadv.abf0851
  • Ye, S.-Y., Fischer, G., Kurth, W.S., Menietti, J.D., Gurnett, D.A. (2017) Rotational modulation of Saturn kilometric radiation, narrowband emission and auroral hiss. In: Fischer, G., Mann, G., Panchenko, M., Zarka, P. (Eds.) Proceedings of the 8th International Workshop on Planetary, Solar and Heliospheric Radio Emissions, Graz Austria, 25–27 Oct 2016. Austrian Academy of Sciences Press, Vienna. https://doi.org/10.1553/PRE8s191

Subjects

Planetary magnetospheres
http://astrothesaurus.org/uat/997
Magnetars
http://astrothesaurus.org/uat/992
High energy astrophysics
http://astrothesaurus.org/uat/739
Jupiter
http://astrothesaurus.org/uat/873
Saturn
http://astrothesaurus.org/uat/1426
Time series analysis
http://astrothesaurus.org/uat/1916
Period search
http://astrothesaurus.org/uat/1955
Gauss-Vaniček spectral analysis
http://astrothesaurus.org/uat/1959
Mars
http://astrothesaurus.org/uat/1007
Interplanetary magnetic fields
http://astrothesaurus.org/uat/824
Planetary dynamics
http://astrothesaurus.org/uat/2173
Planetary science
http://astrothesaurus.org/uat/1255
Astrophysical processes
http://astrothesaurus.org/uat/104
Active sun
http://astrothesaurus.org/uat/18
Pulsars
http://astrothesaurus.org/uat/1306
Solar storm
http://astrothesaurus.org/uat/1526