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1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany

Existing solar physics facilities and data bases at the Astronomical I nstitute of the Slovak Academy of Sciences. (Topic 3. Existing facilities and data bases) A. Kučera, J. Rybák, P. Gömöry, V. Rušin Astronomical Institute, Slovak Academy of Sciences, SK-05690 Tatranská Lomnica, Slovakia

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1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany

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  1. Existing solar physics facilities and data bases at the Astronomical Institute of the Slovak Academy of Sciences. • (Topic 3. Existing facilities and data bases) • A. Kučera, J. Rybák, P. Gömöry, V. Rušin • Astronomical Institute, Slovak Academy of Sciences, • SK-05690 Tatranská Lomnica, Slovakia • ABSTRACT: • A brief summary of existing solar physics synoptic facilities and data bases • at the Astronomical Institute of the Slovak Academy of Sciences • Observations and data sets from the Double coronagraph at Lomnický štit observatory • "Homogeneous series of coronal green line intensities"(1939 - present) • „Catalogue of solar Hα prominences“ (1967-present) 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany

  2. Astronomical Institute of the Slovak Academy of Sciences

  3. Astronomical Institute of the Slovak Academy of Sciences

  4. Astronomical Institute of the Slovak Academy of Sciences

  5. CoMP (2012) spectrograph Solar Chromospheric Detector SCD (2014 - 2015) (similar to ChroMag) (P. Gömöry talk)

  6. Topic 3. Existing facilities and data bases Homogeneous series of coronal green line intensities(1939 - present) 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany

  7. Topic 3. Existing facilities and data bases Homogeneous series of coronal green line intensities(1939 - present) 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany

  8. Topic 3. Existing facilities and data bases Homogeneous series of coronal green line intensities(1939 - present) 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany

  9. Topic 3. Existing facilities and data bases Homogeneous series of coronal green line intensities(1939 - present) 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany

  10. Topic 3. Existing facilities and data bases Homogeneous series of coronal green line intensities(1939 - present) 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany

  11. Topic 3. Existing facilities and data bases Homogeneous series of coronal green line intensities(1939 - present) Intensity variation, rotational characteristics, separately for hemispheres.... 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany

  12. Topic 3. Existing facilities and data bases Homogeneous series of coronal green line intensities(1939 - present) green line intensities Blue and yellow mark magnetic field of opposite polarity 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany

  13. Long-term catalogue of positions, areas, brightness of the H alpha prominences derived from the coronagraphic observations: coronagraph ZEISS 200/3000, interference filter - ~0.6 nm, film,... Papers “Catalogue of solar prominences (1967 – 1986)”, Rušin, V.; Rybanský, M.; Dermendjiev, V.; Stavrev,. Ya., CAOSP, Vol. 17, p. 63 – 292, 1988 “Catalogue of solar prominences 1987 – 1993”, Rusin, V.; Rybansky, M.; Dermendjiev, V.; Stavrev, K. Ya., CAOSP Supplement, vol. 24, p. 135-136, 1994 Topic 3. Existing facilities and data bases Catalogue of solar Hα prominences (1967-present)

  14. photographic film, 36x24mm, several exposures along the limb development with a high contrast, projection for a large image drawing of shapes of prominences, measurement of the parameters: position angle, limb, latitude, longitude, area, height, subjective brightness (1-2-3) observations: coronagraph ZEISS 200/3000, interference filter - ~0.6 nm, film,... Topic 3. Existing facilities and data bases Catalogue of solar Hα prominences (1967-present)

  15. Because of: Free post-focal space needed for new instruments – CoMP-S, SECIS,... End of the coronagraphic photographic observations at the LSO – 20/09/2009 we asked for introduction of the full-disk H alpha observations with an extended exposure time for prominences at the Kaznelhőhe Solar Observatory KSO Starting from 8/2009 Topic 3. Existing facilities and data bases Catalogue of solar Hα prominences (1967-present)

  16. KSO LSO Topic 3. Existing facilities and data bases Catalogue of solar Hα prominences (1967-present)

  17. Topic 3. Existing facilities and data bases Catalogue of solar Hα prominences (1967-present) oo 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany

  18. Topic 3. Existing facilities and data bases Catalogue of solar Hα prominences (1967-present) 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany

  19. Topic 3. Existing facilities and data bases Catalogue of solar Hα prominences (1967-present) 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany

  20. Topic 3. Existing facilities and data bases Catalogue of solar Hα prominences (1967-present) Prominences distribution Blue and yellow mark magnetic field of opposite polarity 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany

  21. Thank you

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