This observation was hold in order to support the XUV-Dopper-Telescope
on boarded the rocket made by High-energy-solarphysics-team of National Astronomical Observatory.
The XDT can observe filtering images around a coronal emission line (FeXIV 211A)
of the solar full disk.
Thus, they can obtain the coronal velocity field along the line of sight
of the full disk.
Besides our Kwasan Observatory, this observation was co-operated by many ground-based observatories, such as Hida Obs., Norikura Corona Obs., Mitaka Obs., Nobeyama Radio Obs., Hiraiso Obs., Nishi-harima Public Obs. etc.
1) Target region (NOAA 8144, 8145, 8146)
[30-Jan; Ha line center], [30-Jan; Ha + 0.5A],[30-Jan; Ha - 0.5A]
[31-Jan; Before Rocket Launch; Ha line center]->[ ]
[31-Jan; After Rocket Launch; Ha line center]
2) Another Active Region (NOAA 8143)
[30-Jan; Ha line center]
[31-Jan; Ha line center]->[ ]
3) Other Regions in the Ha Absorption Line
[North Pole; 31-Jan], [North-East Limb; 31-Jan]
[South-East Quiet Region; 31-Jan]
Observation by using 18cm Refracting Telescope
made in German;Zartorius, 1910
and H alpha Lyot-filter by Halley
at Kwasan Obs.