Bošković’s Method for Determining the Axis and Rate of Solar Rotation by Observing Sunspots in 1777-Reference-Cited by-同舟云学术

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Bošković’s Method for Determining the Axis and Rate of Solar Rotation by Observing Sunspots in 1777

Published:2023-10 Issue:10 Volume:298 Page:
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Husak Mirko^ORCID,Brajša Roman,Špoljarić Dragan^ORCID,Krajnović Davor^ORCID,Ruždjak Domagoj^ORCID,Skokić Ivica^ORCID,Roša Dragan,Hržina Damir

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://link.springer.com/content/pdf/10.1007/s11207-023-02214-6.pdf

Reference41 articles.

1. Arlt, R., Fröhlich, H.-E.: 2012, The solar differential rotation in the 18th century. Astron. Astrophys. 543, A7. DOI. ADS.

2. Arlt, R., Vaquero, J.M.: 2020, Historical sunspot records. Living Rev. Solar Phys. 17, 1. DOI. ADS.

3. Arlt, R., Senthamizh Pavai, V., Schmiel, C., Spada, F.: 2016, Sunspot positions, areas, and group tilt angles for 1611 – 1631 from observations by Christoph Scheiner. Astron. Astrophys. 595, A104. DOI. ADS.

4. Balthasar, H., Woehl, H., Stark, D.: 1987, The solar rotation elements $i$ and $\Omega $ derived from recurrent single sunspots. Astron. Astrophys. 174, 359. ADS.

5. Balthasar, H., Lustig, G., Woehl, H., Stark, D.: 1986, The solar rotation elements $i$ and $\Omega $ derived from sunspot groups. Astron. Astrophys. 160, 277. ADS.

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