J/A+A/698/A182          1000-year sunspot series                (Usoskin+, 2025)

Sunspot cycles for the first millennium BC reconstructed from radiocarbon. Usoskin I., Chatzistergos T., Solanki S.K., Krivova N., Kovaltsov G., Brehm N., Christl M., Wacker L. <Astron. Astrophys. 698, A182 (2025)> =2025A&A...698A.182U 2025A&A...698A.182U (SIMBAD/NED BibCode)
ADC_Keywords: Sun ; Magnetic fields Keywords: Sun: activity - Sun: magnetic fields - sunspots Abstract: The relative sunspot number (SN) is the primary index of solar activity back to 1610. For earlier periods, SN can be reconstructed from the concentrations of cosmogenic isotopes, particularly 14C and 10Be in natural archives. However, due to the limitations of measurement techniques, these reconstructions typically provide SN with only decadal resolution. We aim to reconstruct the first annually resolved sunspot numbers for the first millennium BC, providing a detailed view of solar cycles over a period when this was not possible before. Methods. We reconstruct sunspot numbers from high-precision annual measurements of relative decay-corrected 14C concentrations, Δ14C, covering 1000-BC (Brehm et al. 2025). The process is based on the physics-based approach developed by Usoskin et al. (2021A&A...649A.141U 2021A&A...649A.141U, Cat. J/A+A/649/A141) and has the following four steps: (1) inverting the carbon-cycle model to reconstruct the production rate of 14C, Q; (2) accounting for the effect of the varying geomagnetic field on Q; (3) computing the open solar magnetic flux; and (4) converting it into sunspot numbers. A Monte-Carlo approach is used to account for the uncertainty of the reconstruction. We reconstructed annually resolved SN covering the first millennium BC. Over that period, we identified 93 complete solar cycles with a mean length of 10.5 years. Among those cycles, 23 are well- defined, 21 are reasonably defined, while the rest are poorly defined. We found strong agreement between our reconstructed SN and previous decadal reconstructions, though with higher SN around 1000-920 BC. We did not find any significant long-term periodicities beyond the 11-year solar cycle. Conclusions. This reconstruction offers unique insights into cyclic solar activity for this period of time, which will be valuable for solar dynamo studies and irradiance modelling Description: Five tabular files are presented. * File q1000bc.dat contains annual reconstructions of the 14C production rate [Q] along with its 1-sigma uncertainties [sQ] and the smoothed (22-yr SSA -- see text) values []. This table corresponds to Figure 2a in the text. * File qa1000bc.dat contains annual reconstructions of the 14C production rate reduced to the present-day conditions [Q*] along with its 1-sigma uncertainties [sQ*] and the smoothed (22-yr SSA) values [<Q*>]. This table corresponds to Figure 2b in the text. * File fo1000bc.dat contains annual reconstructions of the open solar flux (OSF) [Fo] along with its 1-sigma uncertainties [sF] and the smoothed (22-yr SSA) values [<Fo>]. This table corresponds to Figure 2c in the text. * File sn1000bc.dat contains annual reconstructions of the sunspot number (SN) [SN] along with its 1-sigma uncertainties [sSN] and the smoothed (22-yr SSA) values []. This table corresponds to Figure 2d in the text. * File cycles.dat presents a textual tabular version of Table 1 in the text and contains the internal cycle number [n], years of minimum [Ymin] and maximum [Ymax] of each cycle, cycle-averaged sunspot number [], its 1-sigma uncertainty [sS], cycle length (min-to-min) [T], and quality flag [q]. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file q1000bc.dat 22 993 Annual reconstructions of the 14C production rate qa1000bc.dat 22 993 Annual reconstructions of the 14C production rate reduced to the present-day conditions (Q*) fo1000bc.dat 22 993 Annual reconstructions of the open solar flux sn1000bc.dat 22 991 Annual reconstructions of the sunspot number (SN) cycles.dat 24 93 Cycles (table 1) -------------------------------------------------------------------------------- Byte-by-byte Description of file: q1000bc.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 yr Year Year (BC) 6- 10 F5.3 1/cm2/s Q Annual value of the 14C production rate (Q) 12- 16 F5.3 1/cm2/s e_Q 1-sigma uncertainty of Q 18- 22 F5.3 1/cm2/s Smoothed Q value -------------------------------------------------------------------------------- Byte-by-byte Description of file: qa1000bc.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 yr Year Year (BC) 6- 10 F5.3 1/cm2/s Q* Annual value of the 14C production rate reduced to the present-day conditions (Q*) 12- 16 F5.3 1/cm2/s e_Q* 1-sigma uncertainty of Q* 18- 22 F5.3 1/cm2/s <Q*> Smoothed Q* value -------------------------------------------------------------------------------- Byte-by-byte Description of file: fo1000bc.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 yr Year Year (BC) 6- 10 F5.2 10+14Wb Fo Annual value of the reconstructed of the open solar flux (OSF) 12- 16 F5.2 10+14Wb e_Fo 1-sigma uncertainty of Fo 18- 22 F5.2 10+14Wb <Fo> Smoothed Fo value -------------------------------------------------------------------------------- Byte-by-byte Description of file: sn1000bc.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 yr Year Year (BC) 6- 10 F5.1 --- SN Annual value of the reconstructed of the sunspot number (SN) 12- 16 F5.1 --- e_SN 1-sigma uncertainty of SN 18- 22 F5.1 --- Smoothed SN value -------------------------------------------------------------------------------- Byte-by-byte Description of file: cycles.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- N Internal cycle number 4- 7 I4 yr Ymin Year of solar cycle minimum 9- 12 I4 yr Ymax Year of solar cycle maximum 14- 16 I3 --- Cycle-averaged SN 18- 19 I2 --- e_ 1-sigma uncertainty of 21- 22 I2 yr T Solar cycle length 24 I1 -- q [0/5] Quality flag -------------------------------------------------------------------------------- Acknowledgements: Ilya Usoskin, ilya.usoskin(at)oulu.fi
(End) Patricia Vannier [CDS] 07-May-2025
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line