| Issue |
J. Space Weather Space Clim.
Volume 10, 2020
Topical Issue - Space climate: The past and future of solar activity
|
|
|---|---|---|
| Article Number | 40 | |
| Number of page(s) | 10 | |
| DOI | https://doi.org/10.1051/swsc/2020041 | |
| Published online | 27 August 2020 | |
- Babcock HW. 1961. The topology of the Sun’s magnetic field and the 22-year cycle. Astrophys J 133: 572. https://doi.org/10.1086/147060. [NASA ADS] [CrossRef] [Google Scholar]
- Charbonneau P. 2010. Dynamo models of the solar cycle. Living Rev Sol Phys 7(1): 3. https://doi.org/10.12942/lrsp-2010-3. [NASA ADS] [CrossRef] [Google Scholar]
- Choudhuri AR, Chatterjee P, Jiang J. 2007. Predicting solar cycle 24 with a solar dynamo model. Phys Rev Lett 98(13): 131103. https://doi.org/10.1103/PhysRevLett.98.131103. [NASA ADS] [CrossRef] [PubMed] [Google Scholar]
- Dasi-Espuig M, Solanki SK, Krivova NA, Cameron R, Peñuela T. 2010. Sunspot group tilt angles and the strength of the solar cycle. A&A 518: A7. https://doi.org/10.1051/0004-6361/201014301. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- DeRosa ML, Brun AS, Hoeksema JT. 2012. Solar magnetic field reversals and the role of dynamo families. Astrophys J 757(1): 96. https://doi.org/10.1088/0004-637X/757/1/96. [NASA ADS] [CrossRef] [Google Scholar]
- Durney BR. 1995. On a Babcock-Leighton dynamo model with a deep-seated generating layer for the toroidal magnetic field. Sol Phys 160(2): 213–235. https://doi.org/10.1007/BF00732805. [NASA ADS] [CrossRef] [Google Scholar]
- Erdős G, Balogh A. 2010. North-south asymmetry of the location of the heliospheric current sheet revisited. J Geophys Res 115(A1): A01105. https://doi.org/10.1029/2009JA014620. [Google Scholar]
- Goel A, Choudhuri AR. 2009. The hemispheric asymmetry of solar activity during the last century and the solar dynamo. Res A&A 9(1): 115–126. https://doi.org/10.1088/1674-4527/9/1/010. [Google Scholar]
- Hale GE. 1924. Sun-spots as magnets and the periodic reversal of their polarity. Nature 113(2829): 105–112. https://doi.org/10.1038/113105a0. [CrossRef] [Google Scholar]
- Hale GE, Ellerman F, Nicholson SB, Joy AH. 1919. The magnetic polarity of sun-spots. Astrophys J 49: 153. https://doi.org/10.1086/142452. [CrossRef] [Google Scholar]
- Hathaway DH, Rightmire L. 2010. Variations in the Sun’s meridional flow over a solar cycle. Science 327(5971): 1350. https://doi.org/10.1126/science.1181990. [NASA ADS] [CrossRef] [Google Scholar]
- Hathaway DH, Upton LA. 2016. Predicting the amplitude and hemispheric asymmetry of solar cycle 25 with surface flux transport. J Geophys Res 121(11): 10744–10753. https://doi.org/10.1002/2016JA023190. [Google Scholar]
- Howard RF. 1991. Axial tilt angles of sunspot groups. Sol Phys 136(2): 251–262. https://doi.org/10.1007/BF00146534. [NASA ADS] [CrossRef] [Google Scholar]
- Hurwitz L. 1960. Eccentric dipoles and spherical harmonic analysis. J Geophys Res 65: 2555. https://doi.org/10.1029/JZ065i008p02555. [CrossRef] [Google Scholar]
- Koskela JS, Virtanen II, Mursula K. 2018. Southward shift of the coronal neutral line and the heliospheric current sheet: Evidence for radial evolution of hemispheric asymmetry. A&A 618: A105. https://doi.org/10.1051/0004-6361/201832609. [CrossRef] [EDP Sciences] [Google Scholar]
- Leighton RB. 1964. Transport of magnetic fields on the Sun. Astrophys J 140: 1547. https://doi.org/10.1086/148058. [NASA ADS] [CrossRef] [Google Scholar]
- Leighton RB. 1969. A magneto-kinematic model of the solar cycle. Astrophys J 156: 1. https://doi.org/10.1086/149943. [NASA ADS] [CrossRef] [Google Scholar]
- Mursula K, Hiltula T. 2003. Bashful ballerina: Southward shifted heliospheric current sheet. Geophys Res Lett 30(22): 2135. https://doi.org/10.1029/2003GL018201. [NASA ADS] [CrossRef] [Google Scholar]
- Mursula K, Hiltula T. 2004. Systematically asymmetric heliospheric magnetic field: Evidence for a quadrupole mode and non-axisymmetry with polarity flip-flops. Sol Phys 224(1–2): 133–143. https://doi.org/10.1007/s11207-005-4977-7. [NASA ADS] [CrossRef] [Google Scholar]
- Nandy D, Choudhuri AR. 2001. Toward a mean field formulation of the Babcock-Leighton type solar dynamo. I. α-coefficient versus Durney’s double-ring approach. Astrophys J 551(1): 576–585. https://doi.org/10.1086/320057. [Google Scholar]
- Petrie GJD. 2013. Solar magnetic activity cycles, coronal potential field models and eruption rates. Astrophys J 768(2): 162. https://doi.org/10.1088/0004-637X/768/2/162. [NASA ADS] [CrossRef] [Google Scholar]
- Petrie GJD. 2015. Solar magnetism in the polar regions. Living Rev Sol Phys 12(1): 5. https://doi.org/10.1007/lrsp-2015-5. [Google Scholar]
- Pulkkinen PJ, Brooke J, Pelt J, Tuominen I. 1999. Long-term variation of sunspot latitudes. A&A 341: L43–L46. [Google Scholar]
- Sivaraman KR, Gupta SS, Howard RF. 1999. Measurement of Kodaikanal white-light images – IV. Axial tilt angles of sunspot groups. Sol Phys 189(1): 69–83. https://doi.org/10.1023/A:1005277515551. [NASA ADS] [CrossRef] [Google Scholar]
- Smith EJ, Balogh A. 2008. Decrease in heliospheric magnetic flux in this solar minimum: Recent Ulysses magnetic field observations. Geophys Res Lett 35(22): L22103. https://doi.org/10.1029/2008GL035345. [CrossRef] [Google Scholar]
- Virtanen I, Mursula K. 2016. Photospheric and coronal magnetic fields in six magnetographs. I. Consistent evolution of the bashful ballerina. A&A 591: A78. https://doi.org/10.1051/0004-6361/201628096. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Virtanen II, Mursula K. 2010. Asymmetry of solar polar fields and the southward shift of HCS observed by Ulysses. J Geophys Res 115(A9): A09110. https://doi.org/10.1029/2010JA015275. [NASA ADS] [CrossRef] [Google Scholar]
- Virtanen II, Mursula K. 2014. North-south asymmetric solar cycle evolution: Signatures in the photosphere and consequences in the corona. Astrophys J 781(2): 99. https://doi.org/10.1088/0004-637X/781/2/99. [NASA ADS] [CrossRef] [Google Scholar]
- Wang YM. 1996. Nonradial coronal streamers. Astrophys J Lett 456: L119. https://doi.org/10.1086/309871. [Google Scholar]
- Wang YM, Nash AG, Sheeley NR. 1989. Magnetic flux transport on the Sun. Science 245(4919): 712–718. https://doi.org/10.1126/science.245.4919.712. [NASA ADS] [CrossRef] [PubMed] [Google Scholar]
- Wang YM, Sheeley NR. 1991. Magnetic flux transport and the Sun’s dipole moment: New twists to the Babcock-Leighton model. Astrophys J 375: 761. https://doi.org/10.1086/170240. [CrossRef] [Google Scholar]
- Wang YM, Sheeley NR. 1992. On potential field models of the solar corona. Astrophys J 392: 310. https://doi.org/10.1086/171430. [Google Scholar]
- Winch DE. 1968. Eccentric geomagnetic dipole potential. Planet Space Sci 16(11): 1341–1347. https://doi.org/10.1016/0032-0633(68)90137-2. [CrossRef] [Google Scholar]
- Zhao XP, Hoeksema JT, Scherrer PH. 2005. Prediction and understanding of the north-south displacement of the heliospheric current sheet. J Geophys Res 110(A10): A10101. https://doi.org/10.1029/2004JA010723. [NASA ADS] [CrossRef] [Google Scholar]
- Zhou X, Smith EJ. 2009. Solar cycle variations of heliospheric magnetic flux. J Geophys Res 114(A3): A03106. https://doi.org/10.1029/2008JA013421. [Google Scholar]
- Zieger B, Virtanen I, Mursula K. 2019. Spatial power spectrum of the photospheric magnetic field during solar minimum. A&A 623: A51. https://doi.org/10.1051/0004-6361/201834216. [CrossRef] [EDP Sciences] [Google Scholar]
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.