Skip to main content
Log in

Study of Sunspot Penumbra to Umbra Area Ratio Using Kodaikanal White-light Digitised Data

  • Published:
Solar Physics Aims and scope Submit manuscript

Abstract

We study the long-term behaviour of the sunspot penumbra to umbra area ratio by analysing recently digitised Kodaikanal white-light data (1923 – 2011). We implement an automatic umbra extraction method and compute the ratio over eight solar cycles (Cycles 16 – 23). Although the average ratio does not show any variation with spot latitudes, cycle phases and strengths, it increases from 5.5 to 6 as the sunspot size increases from 100 μhem to 2000 μhem. Interestingly, our analysis also reveals that this ratio for smaller sunspots (area \({<}\,100\) μhem) does not have any long-term systematic trend as was earlier reported from the photographic results of the Royal Observatory, Greenwich (RGO). To verify the same, we apply our automated extraction technique to Solar and Heliospheric Observatory (SOHO)/Michelson Doppler Imager (MDI) continuum images (1996 – 2010). Results from this data not only confirm our previous findings, but they also show the robustness of our analysis method.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Figure 1
Figure 2
Figure 3
Figure 4
Figure 5
Figure 6
Figure 7
Figure 8
Figure 9
Figure 10

Similar content being viewed by others

Notes

  1. This catalogue is available online at https://kso.iiap.res.in/new/white_light.

  2. Description is available at http://www.idlcoyote.com/idldoc/cg/cgotsu_threshold.html.

  3. For more details, visit https://www.harrisgeospatial.com/Software-Technology/IDL.

  4. This data is downloaded from http://fenyi.solarobs.csfk.mta.hu/ftp/pub/DPD/data/dailyDPD1974_2016.txt.

References

  • Antalová, A.: 1971, The ratio of penumbral and umbral areas of sun-spots in the 11-year solar activity cycle. Bull. Astron. Inst. Czechoslov. 22, 352. ADS .

    ADS  Google Scholar 

  • Baranyi, T., Győri, L., Ludmány, A.: 2016, On-line tools for solar data compiled at the Debrecen observatory and their extensions with the Greenwich sunspot data. Solar Phys. 291, 3081. DOI . ADS .

    Article  ADS  Google Scholar 

  • Beck, J.G., Chapman, G.A.: 1993, A study of the contrast of sunspots from photometric images. Solar Phys. 146, 49. DOI . ADS .

    Article  ADS  Google Scholar 

  • Brandt, P.N., Schmidt, W., Steinegger, M.: 1990, On the umbra–penumbra area ratio of sunspots. Solar Phys. 129, 191. DOI . ADS .

    Article  ADS  Google Scholar 

  • Carrasco, V.M.S., Vaquero, J.M., Trigo, R.M., Gallego, M.C.: 2018, A curious history of sunspot penumbrae: An update. Solar Phys. 293, 104. DOI . ADS .

    Article  ADS  Google Scholar 

  • Fröhlich, C.: 1977, Contemporary measures of the solar constant. In: White, O.R. (ed.) The Solar Output and Its Variation, 93. ADS .

    Google Scholar 

  • Győri, L., Ludmány, A., Baranyi, T.: 2017, Comparative analysis of Debrecen sunspot catalogues. Mon. Not. Roy. Astron. Soc. 465(2), 1259. DOI .

    Article  ADS  Google Scholar 

  • Hale, G.E.: 1908, On the probable existence of a magnetic field in sun-spots. Astrophys. J. 28, 315. DOI . ADS .

    Article  ADS  Google Scholar 

  • Hathaway, D.H.: 2013, A curious history of sunspot penumbrae. Solar Phys. 286, 347. DOI . ADS .

    Article  ADS  Google Scholar 

  • Hathaway, D.H.: 2015, The solar cycle. Living Rev. Solar Phys. 12(1), 4. DOI .

    Article  ADS  Google Scholar 

  • Hudson, H.S., Silva, S., Woodard, M., Willson, R.C.: 1982, The effects of sunspots on solar irradiance. Solar Phys. 76(2), 211. DOI .

    Article  ADS  Google Scholar 

  • Jensen, E., Nordø, J., Ringnes, T.S.: 1955, Variations in the structure of sunspots in relation to the sunspot cycle. Astrophys. Nor. 5, 167. ADS .

    ADS  Google Scholar 

  • Jensen, E., Nordø, J., Ringnes, T.S.: 1956, Variations in the relative size of penumbra and umbra of sunspots in the years 1878 – 1954. Ann. Astrophys. 19, 165. ADS .

    ADS  Google Scholar 

  • Jha, B.K., Mandal, S., Banerjee, D.: 2018, Long-term variation of sunspot penumbra to umbra area ratio: A study using Kodaikanal white-light digitized data. Proc. Int. Astron. Union 13(S340), 185. DOI .

    Article  Google Scholar 

  • Mandal, S., Banerjee, D.: 2016, Sunspot sizes and the solar cycle: Analysis using Kodaikanal white-light digitized data. Astrophys. J. Lett. 830, L33. DOI . ADS .

    Article  ADS  Google Scholar 

  • Mandal, S., Hegde, M., Samanta, T., Hazra, G., Banerjee, D., Ravindra, B.: 2017, Kodaikanal digitized white-light data archive (1921 – 2011): Analysis of various solar cycle features. Astron. Astrophys. 601, A106. DOI . ADS .

    Article  ADS  Google Scholar 

  • Mathew, S.K., Lagg, A., Solanki, S.K., Collados, M., Borrero, J.M., Berdyugina, S., Krupp, N., Woch, J., Frutiger, C.: 2003, Three dimensional structure of a regular sunspot from the inversion of IR Stokes profiles. Astron. Astrophys. 410, 695. DOI . ADS .

    Article  ADS  Google Scholar 

  • Nicholson, S.B.: 1933, The area of a sun-spot and the intensity of its magnetic field. Publ. Astron. Soc. Pac. 45, 51. DOI . ADS .

    Article  ADS  Google Scholar 

  • Otsu, N.: 1979, A threshold selection method from gray-level histograms. IEEE Trans. Syst. Man Cybern. 9(1), 62. DOI .

    Article  Google Scholar 

  • Pettauer, T., Brandt, P.N.: 1997, On novel methods to determine areas of sunspots from photoheliograms. Solar Phys. 175, 197. DOI . ADS .

    Article  ADS  Google Scholar 

  • Pucha, R., Hiremath, K.M., Gurumath, S.R.: 2016, Development of a code to analyze the solar white-light images from the Kodaikanal observatory: Detection of sunspots, computation of heliographic coordinates and area. J. Astrophys. Astron. 37, 3. DOI . ADS .

    Article  ADS  Google Scholar 

  • Ravindra, B., Priya, T.G., Amareswari, K., Priyal, M., Nazia, A.A., Banerjee, D.: 2013, Digitized archive of the Kodaikanal images: Representative results of solar cycle variation from sunspot area determination. Astron. Astrophys. 550, A19. DOI . ADS .

    Article  ADS  Google Scholar 

  • Scherrer, P.H., Bogart, R.S., Bush, R.I., Hoeksema, J.T., Kosovichev, A.G., Schou, J., Rosenberg, W., Springer, L., Tarbell, T.D., Title, A., Wolfson, C.J., Zayer, I. (MDI Engineering Team): 1995, The solar oscillations investigation – Michelson Doppler imager. Solar Phys. 162, 129. DOI . ADS .

    Article  ADS  Google Scholar 

  • Schou, J., Scherrer, P.H., Bush, R.I., Wachter, R., Couvidat, S., Rabello-Soares, M.C., Bogart, R.S., Hoeksema, J.T., Liu, Y., Duvall, T.L., Akin, D.J., Allard, B.A., Miles, J.W., Rairden, R., Shine, R.A., Tarbell, T.D., Title, A.M., Wolfson, C.J., Elmore, D.F., Norton, A.A., Tomczyk, S.: 2012, Design and ground calibration of the Helioseismic and Magnetic Imager (HMI) instrument on the Solar Dynamics Observatory (SDO). Solar Phys. 275, 229. DOI . ADS .

    Article  ADS  Google Scholar 

  • Solanki, S.K.: 2003, Sunspots: An overview. Astron. Astrophys. Rev. 11(2), 153. DOI .

    Article  ADS  Google Scholar 

  • Steinegger, M., Bonet, J.A., Vázquez, M.: 1997a, A new method for the photometric determination of umbral and total sunspot areas. In: JOSO Annu. Rep., 1996, 89. ADS .

    Google Scholar 

  • Steinegger, M., Bonet, J.A., Vázquez, M.: 1997b, Simulation of seeing influences on the photometric determination of sunspot areas. Solar Phys. 171(2), 303. DOI .

    Article  ADS  Google Scholar 

  • Tandberg-Hanssen, E.: 1956, A study of the penumbra–umbra ratio of sunspot pairs. Astrophys. Nor. 5, 207. ADS .

    ADS  Google Scholar 

  • Waldmeier, M.: 1939, Über die Struktur der Sonnenflecken. Astron. Mitt. Eidgenöss. Sternwarte Zür. 14, 439. ADS .

    ADS  Google Scholar 

  • Watson, F.T., Fletcher, L., Marshall, S.: 2011, Evolution of sunspot properties during solar cycle 23. Astron. Astrophys. 533, A14. DOI . ADS .

    Article  ADS  Google Scholar 

  • Watson, F., Fletcher, L., Dalla, S., Marshall, S.: 2009, Modelling the longitudinal asymmetry in sunspot emergence: The role of the Wilson depression. Solar Phys. 260(1), 5. DOI .

    Article  ADS  Google Scholar 

Download references

Acknowledgements

Kodaikanal solar observatory is a facility of the Indian Institute of Astrophysics, Bangalore, India. The data utilised in this article is now available for public use at http://kso.iiap.res.in. We would like to thank Ravindra B. and Manjunath Hegde for their tireless support during the digitisation, calibration and sunspot detection processes. The authors also acknowledge Subhamoy Chatterjee for his useful suggestions during the entire process.

Author information

Authors and Affiliations

Authors

Corresponding authors

Correspondence to Bibhuti Kumar Jha, Sudip Mandal or Dipankar Banerjee.

Ethics declarations

Disclosure of Potential Conflicts of Interest

The authors declare that they have no conflicts of interest.

Additional information

Publisher’s Note

Springer Nature remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.

Rights and permissions

Reprints and permissions

About this article

Check for updates. Verify currency and authenticity via CrossMark

Cite this article

Jha, B.K., Mandal, S. & Banerjee, D. Study of Sunspot Penumbra to Umbra Area Ratio Using Kodaikanal White-light Digitised Data. Sol Phys 294, 72 (2019). https://doi.org/10.1007/s11207-019-1462-2

Download citation

  • Received:

  • Accepted:

  • Published:

  • DOI: https://doi.org/10.1007/s11207-019-1462-2

Keywords

Navigation