SOHO MDI 2000-11-05 17:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30 | 215 | 42 | 306 | -23.21 | 304.85 | 66.06 | 243.52 | 0.9389 | -139.8 | -97.0 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-05 17:35:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 5 | 0 | 7 | -20.60 | 306.92 | 68.13 | 246.70 | 0.9473 | -166.0 | 7.2 | |
| 2 | 15 | 3 | 25 | -22.72 | 307.83 | 69.04 | 244.70 | 0.9541 | -279.4 | -169.4 | |
| 2 | 9 | 3 | 12 | -20.53 | 304.52 | 65.73 | 246.26 | 0.9342 | -314.5 | -217.5 | |
| 0 | 6 | 0 | 8 | -20.63 | 303.41 | 64.63 | 245.91 | 0.9279 | -473.0 | -427.7 | |
| 7 | 122 | 10 | 186 | -24.18 | 306.67 | 67.89 | 242.96 | 0.9503 | 73.9 | -106.9 | |
| 0 | 1 | 0 | 1 | -20.09 | 302.80 | 64.02 | 246.33 | 0.9234 | -392.0 | -411.5 | |
| 10 | -5 | 15 | -5 | -24.02 | 305.62 | 66.83 | 242.88 | 0.9449 | -519.9 | 999999 | |
| 0 | 5 | 0 | 7 | -20.91 | 302.59 | 63.80 | 245.42 | 0.9234 | -319.0 | -429.6 | |
| 0 | 9 | 0 | 11 | -21.39 | 302.78 | 63.99 | 244.96 | 0.9253 | -582.0 | -463.2 | |
| 1 | 5 | 1 | 6 | -20.22 | 300.19 | 61.40 | 245.55 | 0.9069 | 134.5 | 134.6 | |
| 3 | 14 | 4 | 16 | -21.66 | 300.34 | 61.55 | 244.06 | 0.9105 | 201.1 | 46.8 | |
| 0 | 3 | 0 | 3 | -22.66 | 299.44 | 60.65 | 242.75 | 0.9066 | 391.0 | 274.8 | |
| 5 | 13 | 6 | 15 | -23.39 | 299.57 | 60.78 | 242.01 | 0.9090 | 328.4 | 258.1 | |
| 0 | 3 | 0 | 3 | -22.85 | 299.07 | 60.28 | 242.44 | 0.9046 | 360.0 | 345.1 | |
| 0 | 5 | 0 | 6 | -23.81 | 298.02 | 59.24 | 241.11 | 0.8998 | 373.0 | 276.4 | |
| 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. | |