Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-23T10:56:14.255Z Has data issue: false hasContentIssue false
  • English
  • Français

Oscillatory phenomena in a solar network region

Published online by Cambridge University Press:  01 September 2008

Georgia Tsiropoula ,
Kostas Tziotziou ,
Pavol Schwartz  and
Petr Heinzel
Georgia Tsiropoula
Affiliation:
Institute for Space Applications and Remote Sensing, National Observatory of Athens, Lofos Koufos, 15236 P. Penteli, Greece email: [email protected]; [email protected]
Kostas Tziotziou
Affiliation:
Institute for Space Applications and Remote Sensing, National Observatory of Athens, Lofos Koufos, 15236 P. Penteli, Greece email: [email protected]; [email protected]
Pavol Schwartz
Affiliation:
Academy of Sciences of the Czech Republic, Astronomical Institut, CZ-25165 Ondřejov, Czech Republic email: [email protected]; [email protected]
Petr Heinzel
Affiliation:
Academy of Sciences of the Czech Republic, Astronomical Institut, CZ-25165 Ondřejov, Czech Republic email: [email protected]; [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We examine oscillatory phenomena in a solar network region from multi-wavelength, observations obtained by the ground-based Dutch Open Telescope (DOT), and by instruments on the spacecraft Solar and Heliospheric Observatory (SoHO). The observations were obtained during a coordinated observing campaign on October 14, 2005. The temporal variations of the intensities and velocities in two distinct regions of the quiet Sun were investigated: one containing several dark mottles and the other several bright points defining the network boundaries (NB). The aim is to find similarities and/or differences in the oscillatory phenomena observed in these two regions and in different spectral lines formed from the chromosphere to the transition region, as well as propagation characteristics of waves.

Keywords

Sun: chromospheretransition regionoscillations
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S257: Universal Heliophysical Processes , September 2008 , pp. 181 - 184
Copyright
Copyright © International Astronomical Union 2009

References

Cauzzi, G., Falchi, A., & Falciani, R. 2000, A&A, 357, 1093Google Scholar
Curdt, W. & Heinzel, P. 1998, ApJ(Letters), 503, L95Google Scholar
Lites, B. W., Rutten, R. J., & Kalkofen, W. 1993, ApJ, 414, 345CrossRefGoogle Scholar
Tziotziou, K., Tsiropoula, G., & Mein, P. 2004, A&A, 423, 1133Google Scholar
Tsiropoula, G., Tziotziou, K., Schwartz, P., & Heinzel, P. 2009, A&A, 493, 217Google Scholar