Abstract
A new solar imaging system was installed at Hida Observatory to observe the dynamics of flares and filament eruptions. The system (Solar Dynamics Doppler Imager; SDDI) takes full-disk solar images with a field of view of \(2520~\mbox{arcsec} \times 2520~\mbox{arcsec}\) at multiple wavelengths around the \(\mathrm{H}\alpha\) line at 6562 Å. Regular operation was started in May 2016, in which images at 73 wavelength positions spanning from \(\mathrm{H}\alpha -9~\mathring{\mathrm{A}}\) to \(\mathrm{H}\alpha +9~\mathring{\mathrm{A}}\) are obtained every 15 seconds. The large dynamic range of the line-of-sight velocity measurements (\({\pm}\,400~\mbox{km}\,\mbox{s}^{-1}\)) allows us to determine the real motions of erupting filaments in 3D space. It is expected that SDDI provides unprecedented datasets to study the relation between the kinematics of filament eruptions and coronal mass ejections (CME), and to contribute to the real-time prediction of the occurrence of CMEs that cause a significant impact on the space environment of the Earth.
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Fang, C., Chen, P.-F., Li, Z., Ding, M.-D., Dai, Y., Zhang, X.-Y., Mao, W.-J., Zhang, J.-P., Li, T., Liang, Y.-J., Lu, H.-T.: 2013, A new multi-wavelength solar telescope: Optical and Near-infrared Solar Eruption Tracer (ONSET). Res. Astron. Astrophys. 13, 1509. DOI . ADS .
Filippov, B.: 2013, A filament eruption on 2010 October 21 from three viewpoints. Astrophys. J. 773, 10. DOI . ADS .
Gopalswamy, N.: 2015, The dynamics of eruptive prominences. In: Vial, J.-C., Engvold, O. (eds.) Solar Prominences, Astrophys. Space Sci. Lib. 415, 381. DOI . ADS .
Gopalswamy, N., Shimojo, M., Lu, W., Yashiro, S., Shibasaki, K., Howard, R.A.: 2003, Prominence eruptions and coronal mass ejection: a statistical study using microwave observations. Astrophys. J. 586, 562. DOI . ADS .
Hagino, M., Ichimoto, K., Kimura, G., Nakatani, Y., Kawate, T., Shinoda, K., Suematsu, Y., Hara, H., Shimizu, T.: 2014, Development of a universal tunable filter for future solar observations. In: Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation, Proc. SPIE 9151, 91515V. DOI . ADS .
Howard, T.A.: 2015, Measuring an eruptive prominence at large distances from the Sun. I. Ionization and early evolution. Astrophys. J. 806, 175. DOI . ADS .
Kuhn, J.R., Lin, H., Loranz, D.: 1991, Gain calibrating nonuniform image-array data using only the image data. Publ. Astron. Soc. Pac. 103, 1097. DOI . ADS .
Kurokawa, H., Ishiura, K., Kimura, G., Nakai, Y., Kitai, R., Funakoshi, Y., Shinkawa, T.: 1995, Observations of solar H alpha filament disappearances with a new solar flare-monitoring-telescope at Hida Observatory. J. Geomagn. Geoelectr. 47, 1043.
McCauley, P.I., Su, Y.N., Schanche, N., Evans, K.E., Su, C., McKillop, S., Reeves, K.K.: 2015, Prominence and filament eruptions observed by the solar dynamics observatory: statistical properties, kinematics, and online catalog. Solar Phys. 290, 1703. DOI . ADS .
Morimoto, T., Kurokawa, H.: 2003, A method for the determination of 3-D velocity fields of disappearing solar filaments. Publ. Astron. Soc. Japan 55, 503. DOI . ADS .
Munro, R.H., Gosling, J.T., Hildner, E., MacQueen, R.M., Poland, A.I., Ross, C.L.: 1979, The association of coronal mass ejection transients with other forms of solar activity. Solar Phys. 61, 201. DOI . ADS .
Penn, M.J.: 2000, An erupting active region filament: three-dimensional trajectory and hydrogen column density. Solar Phys. 197, 313. DOI . ADS .
Shimojo, M.: 2014, Unusual migration of the prominence activities in recent solar cycles. In: Schmieder, B., Malherbe, J.-M., Wu, S.T. (eds.) Nature of Prominences and Their Role in Space Weather, IAU Symp. 300, 161. DOI . ADS .
UeNo, S., Nagata, S.-i., Kitai, R., Kurokawa, H., Ichimoto, K.: 2004, The development of filter vector magnetographs for the Solar Magnetic Activity Research Telescope (SMART). In: Moorwood, A.F.M., Iye, M. (eds.) Ground-Based Instrumentation for Astronomy, Proc. SPIE 5492, 958. DOI . ADS .
Acknowledgements
The authors are grateful to the staff of Hida Observatory for supporting the instrument development and daily observations. This work was supported by MEXT/JSPS KAKENHI Grant Number JP15H05814, Project for Solar-Terrestrial Environment Prediction (PSTEP).
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Earth-affecting Solar Transients
Guest Editors: Jie Zhang, Xochitl Blanco-Cano, Nariaki Nitta, and Nandita Srivastava
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Ichimoto, K., Ishii, T.T., Otsuji, K. et al. A New Solar Imaging System for Observing High-Speed Eruptions: Solar Dynamics Doppler Imager (SDDI). Sol Phys 292, 63 (2017). https://doi.org/10.1007/s11207-017-1082-7
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DOI: https://doi.org/10.1007/s11207-017-1082-7