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We present and analyse the sunspot observations performed by Franz I. C. Hallaschka in 1814 and 1816. These solar observations were carried out during the so-called Dalton minimum, around the maximum phase of the Solar Cycle 6. These…

太阳与恒星天体物理 · 物理学 2018-08-01 V. M. S. Carrasco , J. M. Vaquero , R. Arlt , M. C. Gallego

The sunspot groups have been observed since 1610 and their numbers have been used for evaluating the amplitude of solar activity. Daniel M\"ogling recorded his sunspot observations for more than 100 days in 1626 - 1629 and formed a…

太阳与恒星天体物理 · 物理学 2021-02-09 Hisashi Hayakawa , Tomoya Iju , Koji Murata , Bruno P. Besser

In addition to regular Schwabe cycles (~ 11 years), solar activity also shows longer periods of enhanced or reduced activity. Of these, reconstructions of the Dalton Minimum provide controversial sunspot group numbers and limited sunspot…

太阳与恒星天体物理 · 物理学 2021-05-13 Hisashi Hayakawa , Shoma Uneme , Bruno P. Besser , Tomoya Iju , Shinsuke Imada

A revision is presented of the sunspot observations made by Charles Malapert from 1618 to 1626, studying several documentary sources that include those observations. The revised accounting of the group numbers recorded by Malapert for that…

太阳与恒星天体物理 · 物理学 2021-03-18 V. M. S. Carrasco , M. C. Gallego , J. Villalba Álvarez , J. M. Vaquero

There is a low frequency of sunspot observations in some years of the 17th and 18th century. In particular, the interval 1777-1795 is one of the periods with scarce observations in the databases. In this note, we report a sunspot…

太阳与恒星天体物理 · 物理学 2017-07-13 F. Domínguez-Castro , J. M. Vaquero

The solar program of the Astronomical Observatory of Madrid started in 1876. For ten solar cycles, observations were made in this institution to determine sunspot numbers and areas. The program was completed in 1986. The resulting data have…

太阳与恒星天体物理 · 物理学 2015-06-22 A. J. P. Aparicio , J. M. Vaquero , V. M. S. Carrasco , M. C. Gallego

A long time-series of sunspot observations is preserved from Samuel Heinrich Schwabe who made notes and drawings of sunspots from 1825-1867. Schwabe's observing records are preserved in the manuscript archives of the Royal Astronomical…

物理学史与哲学 · 物理学 2015-05-30 R. Arlt

As we are heading towards the next solar cycle, presumably with a relatively small amplitude, it is of significant interest to reconstruct and describe the past grand minima on the basis of actual observations of the time. The Dalton…

太阳与恒星天体物理 · 物理学 2020-01-09 Hisashi Hayakawa , Bruno P. Besser , Tomoya Iju , Rainer Arlt , Shoma Uneme , Shinsuke Imada , Philippe-A. Bourdin , Amand Kraml

We revise the sunspot observations made by Galileo Galilei and Christoph Scheiner in the context of their controversy on the nature of sunspots. Their sunspot records not included in the current sunspot group database, used as a basis to…

太阳与恒星天体物理 · 物理学 2021-03-19 V. M. S. Carrasco , M. C. Gallego , J. M. Vaquero

We have recovered the sunspot observations made by David E. Hadden during 1890-1931 from Alta, Iowa. We have digitized the available data published by Hadden in different astronomical journals. This data series have been analyzed and…

太阳与恒星天体物理 · 物理学 2015-06-16 V. M. S. Carrasco , J. M. Vaquero , M. C. Gallego , R. M. Trigo

William Cranch Bond, director of the Harvard College Observatory in mid-19th century, carried out detailed sunspot observations during the period 1847-1849. We highlight Bond was the observer with the highest daily number of sunspot groups…

太阳与恒星天体物理 · 物理学 2021-03-19 V. M. S. Carrasco , M. C. Gallego , R. Arlt , J. M. Vaquero

In addition to the regular Schwabe cycles of approximately 11 y, "prolonged solar activity minima" have been identified through the direct observation of sunspots and aurorae, as well as proxy data of cosmogenic isotopes. Some of these…

太阳与恒星天体物理 · 物理学 2020-12-29 Sam M. Silverman , Hisashi Hayakawa

Extending the knowledge about the properties of solar cycles into the past is essential for understanding the solar dynamo. This paper aims at estimating areas of sunspots observed by Schwabe in 1825-1867 and at calculating the tilt angles…

太阳与恒星天体物理 · 物理学 2015-12-02 V. Senthamizh Pavai , R. Arlt , M. Dasi-Espuig , N. Krivova , S. Solanki

We have examined the more than 1100 drawings of the solar disk made by the German astronomy amateur Johann Caspar Staudach during 1749-1799 and counted the spots on each image. Using the modern perception of how to group spots into active…

太阳与恒星天体物理 · 物理学 2015-11-06 Leif Svalgaard

French astronomer Honor\'e Flaugergues compiled astronomical observations in a series of hand-written notebooks for 1782$\unicode{x2013}$1830, which are preserved at Paris Observatory. We reviewed these manuscripts and encoded the records…

太阳与恒星天体物理 · 物理学 2023-05-24 Egor Illarionov , Rainer Arlt

Early observations of sunspot were realised by the naked eye. Possible utilization of these records for studying the long-term change in the Sun is discussed here. Other historical sunspot observations with camera obscuras are also…

天体物理学 · 物理学 2008-11-26 J. M. Vaquero

Most of our knowledge about the Sun's activity cycle arises from sunspot observations over the last centuries since telescopes have been used for astronomy. The German astronomer Gustav Sp\"orer observed almost daily the Sun from 1861 until…

太阳与恒星天体物理 · 物理学 2015-11-11 Andrea Diercke , Rainer Arlt , Carsten Denker

The focus of this article is a re-count of Richard Carrington's original sunspot observations from his book drawings (Carrington,1863) by an observer from the World data Center-SILSO network, Thomas H. Teague(UK). This modern recount will…

太阳与恒星天体物理 · 物理学 2023-01-06 Shreya Bhattacharya , E. T. H Teague , S. Fay , Laure Lefèvre , M. Jansen , F. Clette

Naked-eye sunspot observations (NESO, hereafter) have been recorded for last two millennia, approximately. This kind of records were made around the world, mainly in Asian civilizations, and they are compiled in several catalogues. In this…

太阳与恒星天体物理 · 物理学 2020-12-02 V. M. S. Carrasco , M. C. Gallego , R. Arlt , J. M. Vaquero

We revisit the sunspot drawings made by the Japanese astronomer Kunitomo Toubei during 1835-1836 and recount the sunspot group number for each image. There are two series of drawings, preliminary (P, containing 17 days with observations)…

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