A Revised Collection of Sunspot Group Numbers

被引：135

作者：

Vaquero, J. M. ^{[1
,2
]}

Svalgaard, L. ^{[3
]}

Carrasco, V. M. S. ^{[2
,4
]}

Clette, F. ^{[5
]}

LefSvre, L. ^{[5
]}

Gallego, M. C. ^{[2
,4
]}

Arlt, R. ^{[6
]}

Aparicio, A. J. P. ^{[2
,4
]}

Richard, J. -G. ^{[7
]}

Howe, R. ^{[8
]}

机构：

[1] Univ Extremadura, Dept Fis, Merida 06800, Spain

[2] Univ Extremadura, Inst Univ Invest Agua Cambio Climat & Sostenibili, Badajoz 06006, Spain

[3] Stanford Univ, WW Hansen Expt Phys Lab, Stanford, CA 94305 USA

[4] Univ Extremadura, Dept Fis, E-06071 Badajoz, Spain

[5] Royal Observ Belgium, World Data Ctr SILSO, 3 Ave Circulaire, B-1180 Brussels, Belgium

[6] Leibniz Inst Astrophys Potsdam AIP, Sternwarte 16, D-14482 Potsdam, Germany

[7] 6 Rue Guesnault, F-41100 Vendome, France

[8] AAVSO, Solar Sect, 49 Bay State Rd, Cambridge, MA 02138 USA

来源：

SOLAR PHYSICS | 2016年 / 291卷 / 9-10期

关键词：

Sunspots; statistics; Solar cycle; observations; SOLAR-ACTIVITY; MAUNDER MINIMUM; CYCLE; RELIABILITY; ROTATION; LIMIT; LOST;

D O I：

10.1007/s11207-016-0982-2

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We describe a revised collection of the number of sunspot groups from 1610 to the present. This new collection is based on the work of Hoyt and Schatten (Solar Phys. 179, 189, 1998). The main changes are the elimination of a considerable number of observations during the Maunder Minimum (hereafter, MM) and the inclusion of several long series of observations. Numerous minor changes are also described. Moreover, we have calculated the active-day percentage during the MM from this new collection as a reliable index of the solar activity. Thus, the level of solar activity obtained in this work is greater than the level obtained using the original Hoyt and Schatten data, although it remains compatible with a grand minimum of solar activity. The new collection is available in digital format.

引用

页码：3061 / 3074

页数：14

共 50 条

[41] Reconstruction of the Heliospheric Current Sheet Tilts Using Sunspot Numbers
Mykola I. Pishkalo
Solar Physics, 2006, 233 : 277 - 290
[42] Identification of Gleissberg Cycles and a Rising Trend in a 315-Year-Long Series of Sunspot Numbers
Le Mouel, Jean-Louis
Lopes, Fernand
Courtillot, Vincent
SOLAR PHYSICS, 2017, 292 (03)
[43] Periodicities in the coronal rotation and sunspot numbers
Chandra, Satish
Vats, Hari Om
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2011, 414 (04) : 3158 - 3165
[44] The effect of telescope aperture, scattered light and human vision on early measurements of sunspot and group numbers
Karachik, Nina V.
Pevtsov, Alexei A.
Nagovitsyn, Yury A.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2019, 488 (03) : 3804 - 3809
[45] The Discontinuity Circa 1885 in the Group Sunspot Number
Cliver, E. W.
Ling, A. G.
SOLAR PHYSICS, 2016, 291 (9-10) : 2763 - 2784
[46] Sunspot Group Development in High Temporal Resolution
J. Muraközy
T. Baranyi
A. Ludmány
Solar Physics, 2014, 289 : 563 - 577
[47] Hysteresis of Cosmic Rays with Respect to Sunspot Numbers During the Recent Sunspot Minimum
Kane, R. P.
SOLAR PHYSICS, 2011, 269 (02) : 451 - 454
[48] Comparison of solar activity proxies: eigenvectors versus averaged sunspot numbers
Zharkova, V. V.
Vasilieva, I
Popova, E.
Shepherd, S. J.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023, 521 (04) : 6247 - 6265
[49] Sunspot Numbers from ISOON: A Ten-Year Data Analysis
K. S. Balasubramaniam
T. W. Henry
Solar Physics, 2016, 291 : 3123 - 3138
[50] Sunspot Numbers from ISOON: A Ten-Year Data Analysis
Balasubramaniam, K. S.
Henry, T. W.
SOLAR PHYSICS, 2016, 291 (9-10) : 3123 - 3138

← 1 2 3 4 5 →