Date | Photosph. | N | Fe II | N | DIB | N |
km s-1 | km s-1 | km s-1 | ||||
2000/07/19 | ![]() |
9 | ||||
2000/07/21 | ![]() |
12 | ![]() |
4 | ![]() |
3 |
2002/03/03 | ![]() |
37 | ![]() |
9 | ![]() |
5 |
2002/05/23 | ![]() |
13 | ![]() |
4 | ![]() |
3 |
2002/05/24 | ![]() |
24 | ![]() |
3 | ![]() |
3 |
2002/06/23 | ![]() |
23 | ![]() |
2 | ![]() |
3 |
2002/06/24 | ![]() |
45 | ![]() |
5 | ![]() |
5 |
2002/06/25 | ![]() |
48 | ![]() |
7 | ![]() |
4 |
2002/09/25 | ![]() |
14 | ![]() |
3 | ![]() |
7 |
The mean HRV of the photospheric lines are listed in Col. 2,
those of the emission peaks of the Fe II lines in Col. 4, and
those of the DIBs in Col. 6. The number of lines used for the averaging are listed in Cols. 3, 5, and 7, respectively. The DIBs HRV measurements show the wavelength scale stability. |