Christian Horrebow's Sunspot Observations -- I. Life and Published Writings
arXiv:1906.10884 · doi:10.1007/s11207-019-1465-z
Abstract
Between 1761 and 1776, Christian Horrebow made regular observations of sunspots from Rundetaarn in Copenhagen. Based on these observations he writes in 1775 that "it appears that after the course of a certain number of years, the appearance of the Sun repeats itself with respect to the number and size of the spots". Thus, Horrebow hypothesized the idea of a cyclic Sun several decades before Heinrich Schwabe discovered the solar cycle and estimated its period. This proves the ability of Horrebow as a sunspot observer. In this article, we present a general overview of the work of Christian Horrebow, including a brief biography and a complete bibliography. We also present a translation from Danish to English of his writings on sunspots in the Dansk Historisk Almanak. These writings include tables of daily sunspot measurements of which we discuss the completeness.
arXiv commentPublished in Solar Physics. If you like to have acces to the Supplementary material, please send me an email: [email protected]
References in corpus (6)
- Revisiting the Sunspot Number
- Reconstruction of the Sunspot Group Number: the Backbone Method
- A Revised Collection of Sunspot Group Numbers
- A New Calibrated Sunspot Group Series Since 1749: Statistics of Active Day Fractions
- Visualization of the challenges and limitations of the long-term sunspot number record
- Christian Horrebow's Sunspot Observations -- II. Construction of a Record of Sunspot Positions
Cited by in corpus (4)
- Re-calibration of the Sunspot Number: Status Report
- Thaddäus Derfflinger's sunspot observations during 1802-1824: A primary reference to understand the Dalton Minimum
- A comparative study of two X2.2 and X9.3 solar flares observed with HARPS-N: Reconciling Sun-as-a-star spectroscopy and high-spatial resolution solar observations in the context of the solar-stellar connection
- Christian Horrebow's Sunspot Observations -- II. Construction of a Record of Sunspot Positions