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Uncertainty of sunspot parameters reconstructed from early telescopic sunspot observations. / Золотова, Надежда Валерьевна; Вохмянин, Михаил Владимирович.

Problems of Geocosmos–2020. 2022. p. 489-495 (Springer Proceedings in Earth and Environmental Sciences).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Research › peer-review

Harvard

Золотова, НВ & Вохмянин, МВ 2022, Uncertainty of sunspot parameters reconstructed from early telescopic sunspot observations. in Problems of Geocosmos–2020. Springer Proceedings in Earth and Environmental Sciences, pp. 489-495, XIII Школа-конференция "Проблемы Геокосмоса" , Санкт-Петербург, Russian Federation, 5/10/20. https://doi.org/10.1007/978-3-030-91467-7_37

APA

Золотова, Н. В., & Вохмянин, М. В. (2022). Uncertainty of sunspot parameters reconstructed from early telescopic sunspot observations. In Problems of Geocosmos–2020 (pp. 489-495). (Springer Proceedings in Earth and Environmental Sciences). https://doi.org/10.1007/978-3-030-91467-7_37

Vancouver

Золотова НВ, Вохмянин МВ. Uncertainty of sunspot parameters reconstructed from early telescopic sunspot observations. In Problems of Geocosmos–2020. 2022. p. 489-495. (Springer Proceedings in Earth and Environmental Sciences). https://doi.org/10.1007/978-3-030-91467-7_37

Author

Золотова, Надежда Валерьевна ; Вохмянин, Михаил Владимирович. / Uncertainty of sunspot parameters reconstructed from early telescopic sunspot observations. Problems of Geocosmos–2020. 2022. pp. 489-495 (Springer Proceedings in Earth and Environmental Sciences).

BibTeX

@inproceedings{39c45260b8614ccc89ceb6234479f3ba,
title = "Uncertainty of sunspot parameters reconstructed from early telescopic sunspot observations",
abstract = "We present the results of the reconstruction of the parameters of solar activity from astronomical observations in the seventeenth century. Drawings of the solar disk made by various observers differ in the observing methodology and accuracy. The distribution of the sunspot group areas from historical archives was compared with that of the modern epoch. A lack of small groups of sunspots was found in early observations. This, in turn, leads to an uncertainty in the number of sunspot groups in tens of percent. Additional uncertainty of group numbers is introduced by sorting the sunspots into groups. The latitude-time distribution of sunspots is also discussed.",
keywords = "Observations, Solar cycle, Sunspots",
author = "Золотова, {Надежда Валерьевна} and Вохмянин, {Михаил Владимирович}",
note = "Publisher Copyright: {\textcopyright} 2022, The Author(s), under exclusive license to Springer Nature Switzerland AG.; null ; Conference date: 05-10-2020 Through 09-10-2020",
year = "2022",
doi = "10.1007/978-3-030-91467-7_37",
language = "English",
series = "Springer Proceedings in Earth and Environmental Sciences",
pages = "489--495",
booktitle = "Problems of Geocosmos–2020",

}

RIS

TY - GEN

T1 - Uncertainty of sunspot parameters reconstructed from early telescopic sunspot observations

AU - Золотова, Надежда Валерьевна

AU - Вохмянин, Михаил Владимирович

N1 - Publisher Copyright: © 2022, The Author(s), under exclusive license to Springer Nature Switzerland AG.

PY - 2022

Y1 - 2022

N2 - We present the results of the reconstruction of the parameters of solar activity from astronomical observations in the seventeenth century. Drawings of the solar disk made by various observers differ in the observing methodology and accuracy. The distribution of the sunspot group areas from historical archives was compared with that of the modern epoch. A lack of small groups of sunspots was found in early observations. This, in turn, leads to an uncertainty in the number of sunspot groups in tens of percent. Additional uncertainty of group numbers is introduced by sorting the sunspots into groups. The latitude-time distribution of sunspots is also discussed.

AB - We present the results of the reconstruction of the parameters of solar activity from astronomical observations in the seventeenth century. Drawings of the solar disk made by various observers differ in the observing methodology and accuracy. The distribution of the sunspot group areas from historical archives was compared with that of the modern epoch. A lack of small groups of sunspots was found in early observations. This, in turn, leads to an uncertainty in the number of sunspot groups in tens of percent. Additional uncertainty of group numbers is introduced by sorting the sunspots into groups. The latitude-time distribution of sunspots is also discussed.

KW - Observations

KW - Solar cycle

KW - Sunspots

UR - http://www.scopus.com/inward/record.url?scp=85125252453&partnerID=8YFLogxK

UR - https://www.mendeley.com/catalogue/d02d8710-d54b-34dc-95e9-24ab61b4e585/

U2 - 10.1007/978-3-030-91467-7_37

DO - 10.1007/978-3-030-91467-7_37

M3 - Conference contribution

T3 - Springer Proceedings in Earth and Environmental Sciences

SP - 489

EP - 495

BT - Problems of Geocosmos–2020

Y2 - 5 October 2020 through 9 October 2020

ER -

ID: 100038735