2004 September-October
J.Singh, K.Ichimoto

1. Raster scans in 6374 Angstrom, [Fe XIV] 5303 Angstrom, [Fe XIII]
10747 Angstrom, and [Fe XI] 7892 Angstrom coronal emission lines were
obtained with large exposure times in polar regions to study the effect
of waves in polar regions.

Paper:
Spectroscopic Studies of the Solar Corona VIII. Temperature and
Non-Thermal Variations in Steady Coronal Structures
Singh,J., Sakurai,T. Ichimoto,K., Muneer, S., and Raveendran, A.V.: 2006, Solar Phys., 236, 245

2. Raster scans in the green and red lines and NOGIS data.

Paper:
Spectroscopic Studies of the Solar Corona VII. Formation of a
Coronal Loop by Evaporation
Singh,J., Sakurai,T. Ichimoto,K., Suzuki,I., and Hagino, M.: 2005,
Solar Phys., 226, 201