SOHO MDI 2000-07-14 06:17:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50 | 217 | 27 | 111 | -10.22 | 307.17 | -3.54 | 166.62 | 0.2616 | -267.0 | -244.2 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-07-14 06:17:31 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6 | 19 | 3 | 10 | -10.25 | 311.58 | 0.88 | 183.42 | 0.2534 | -1240.2 | -977.1 | |
| 0 | 6 | 0 | 3 | -10.04 | 311.10 | 0.39 | 181.56 | 0.2496 | -992.0 | -922.0 | |
| 0 | 2 | 0 | 1 | -11.44 | 310.17 | -0.53 | 178.08 | 0.2732 | -498.0 | -520.3 | |
| 7 | 21 | 4 | 11 | -9.88 | 308.73 | -1.97 | 172.13 | 0.2490 | 1025.2 | 859.0 | |
| 0 | 5 | 0 | 3 | -9.60 | 307.41 | -3.30 | 166.75 | 0.2485 | 782.0 | 606.9 | |
| 15 | 112 | 8 | 57 | -10.38 | 307.12 | -3.59 | 166.37 | 0.2624 | -1391.3 | -298.5 | |
| 15 | -6 | 8 | -6 | -9.81 | 306.56 | -4.14 | 163.75 | 0.2555 | 956.6 | 999999 | |
| 0 | 6 | 0 | 3 | -10.39 | 305.95 | -4.76 | 162.19 | 0.2678 | -535.0 | -451.3 | |
| 0 | 4 | 0 | 2 | -10.31 | 305.63 | -5.08 | 160.97 | 0.2683 | -921.0 | -823.0 | |
| 0 | 6 | 0 | 3 | -10.92 | 305.46 | -5.25 | 161.13 | 0.2790 | -107.0 | -191.5 | |
| 7 | 17 | 4 | 9 | -10.43 | 305.18 | -5.52 | 159.60 | 0.2728 | -1062.4 | -813.7 | |
| 0 | 8 | 0 | 4 | -11.50 | 304.80 | -5.91 | 159.69 | 0.2919 | 781.0 | 630.8 | |
| 0 | 5 | 0 | 2 | -10.44 | 304.13 | -6.58 | 156.14 | 0.2796 | -744.0 | -601.7 | |
| 0 | 6 | 0 | 3 | -10.58 | 302.79 | -7.92 | 152.19 | 0.2915 | 520.0 | 426.2 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
||
| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |