Abstract
A complete dataset of sunspot drawings recorded at Sacramento Peak Observatory (SPO) from late 1947 till mid-2004 has been digitized. We present the history of the observations and describe the data included in the drawings. We compare the sunspot number index calculated from the SPO data and the International Sunspot Number (SNv2), and we find that both series exhibit a similar behavior. The ratio of two sunspot numbers is relatively constant at about 1.2 – 1.3 during 1955–1995, with larger variations present at the beginning of the time series. This work represents the first step for the publication of the SPO sunspot catalogue in digital format. More information, such as positions and areas of sunspots, will be included in the next versions in order to provide the space weather and climate community a more complete sunspot catalogue with good quality observations.
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Acknowledgements
The authors acknowledge the international team on Recalibration of the Sunspot Number Series supported by the International Space Science Institute (ISSI), Bern, Switzerland. This research was supported by the Economy and Infrastructure Counselling of the Junta of Extremadura through project IB16127 and grants GR18097 (cofinanced by the European Regional Development Fund) and by the Ministerio de Economía y Competitividad of the Spanish Government (CGL2017-87917-P). Sac Peak drawings were digitized by NOAA’s (former) National Geophysical Data Center (NGDC) and AAP. AAP acknowledges fruitful conversation with Kim Streander about his experience as a Sac Peak observer, and the help by Lou Gilliam and Douglas Gilliam with identifying the names of many observers (their initials on drawings are shown in parentheses): Bryan Armstrong (BDA), George Austin (GMA), Harley Baird (HB), Ed Bergstrom (ENB, EHB), Bill Breedlove (WOB), Todd Brown (DTB), Don Carson (DC), Roger Carson (RC), Eddy Coleman (JEC), Roy Colter (RLC), Rudolph Cook (RHC), John Cornett (JLC), Harry Crawford (HC), Bill Davis (B, BD), Lee Davis (LD), William Davis (W), Howard DeMastus (HD, D, HLD), Joe Elrod (JKE), Lou Gilliam (G, LBG, LG), Douglas Gilliam (DLG), Buzz Graves (BG, BEG), Frank Hegwer (H), Steve Hegwer (SLH), Tim Henry (TWH), Ellis Johansen (E, EEJ, EJ), Dick Mann (M), Frank Manigold (FEM), Patrick S. McIntosh (MC INTOSH), Gary Phyllis (GLP, GP), Harry Ramsey (HER), George Schnable (GSK, GS), Mike Smith (MTS), Arnold Starr (AUS), Rod Stover (S), Kim V. Streander (KVS), Steve Tullis (SET, TULLIS), Bob Wade (W), Jim Warwick (JPW, WARWICK), Phil Young (PCY, PYC), and Dr. Ching-Sung Yu (Y, YU). We thank all observers for their dedication to the program of daily sunspot drawings at Sacramento Peak observatory. Data were acquired by the white-light patrol instrument operated by NSO/AURA/NSF.
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Carrasco, V.M.S., Pevtsov, A.A., Nogales, J.M. et al. The Sunspot Drawing Collection of the National Solar Observatory at Sacramento Peak (1947–2004). Sol Phys 296, 3 (2021). https://doi.org/10.1007/s11207-020-01746-5
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DOI: https://doi.org/10.1007/s11207-020-01746-5