Pith. sign in

REVIEW 1 cited by

Solar cycle 25: another moderate cycle?

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1604.05405 v2 pith:SVAYJHWJ submitted 2016-04-19 astro-ph.SR

classification astro-ph.SR
keywords cycledipoleminimummomentactivityduringmoderatepredictions
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
abstract

Surface flux transport simulations for the descending phase of cycle 24 using random sources (emerging bipolar magnetic regions) with empirically determined scatter of their properties provide a prediction of the axial dipole moment during the upcoming activity minimum together with a realistic uncertainty range. The expectation value for the dipole moment around 2020 $(2.5\pm1.1\,$G) is comparable to that observed at the end of cycle 23 (about $2\,$G). The empirical correlation between the dipole moment during solar minimum and the strength of the subsequent cycle thus suggests that cycle 25 will be of moderate amplitude, not much higher than that of the current cycle. However, the intrinsic uncertainty of such predictions resulting from the random scatter of the source properties is considerable and fundamentally limits the reliability with which such predictions can be made before activity minimum is reached.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models

    astro-ph.SR 2026-07 conditional novelty 6.0 of 10

    A comparative analysis of 2D surface flux transport and 3D dynamo models yields a mode-dependent radial decay spectrum with effective timescales τ≈2 yr (l=8) for magnetogram assimilation and τ≈7 yr (dipole) for active...

Pith tools