| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57 | 438 | 35 | 272 | 2.94 | 270.24 | -36.88 | 90.97 | 0.6009 | -179.6 | -260.6 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-07-14 12:47:31 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14 | 69 | 8 | 40 | 2.43 | 276.86 | -30.26 | 92.65 | 0.5060 | 1347.1 | 814.4 | |
| 9 | -1 | 5 | -1 | 1.99 | 276.78 | -30.34 | 93.50 | 0.5078 | 1069.6 | 999999 | |
| 0 | 4 | 0 | 2 | 3.28 | 275.17 | -31.95 | 90.81 | 0.5305 | 747.0 | 584.8 | |
| 3 | 10 | 2 | 6 | 2.71 | 273.77 | -33.35 | 91.71 | 0.5515 | 715.7 | 530.5 | |
| 0 | 6 | 0 | 4 | 2.90 | 272.72 | -34.40 | 91.25 | 0.5666 | 777.0 | 470.2 | |
| 0 | 12 | 0 | 7 | 3.07 | 272.23 | -34.89 | 90.88 | 0.5735 | 579.0 | 501.9 | |
| 0 | 5 | 0 | 3 | 4.01 | 271.94 | -35.18 | 89.23 | 0.5769 | -518.0 | -547.5 | |
| 0 | 6 | 0 | 4 | 3.26 | 271.05 | -36.07 | 90.46 | 0.5901 | -383.0 | -532.7 | |
| 0 | 4 | 0 | 3 | 3.60 | 270.64 | -36.48 | 89.85 | 0.5956 | -640.0 | -607.1 | |
| 0 | 18 | 0 | 11 | 2.48 | 270.44 | -36.68 | 91.71 | 0.5993 | 339.0 | -133.1 | |
| 0 | 4 | 0 | 2 | 1.54 | 269.87 | -37.26 | 93.19 | 0.6083 | 258.0 | 331.7 | |
| 8 | 300 | 5 | 190 | 3.37 | 269.05 | -38.07 | 90.11 | 0.6178 | -1354.0 | -562.1 | |
| 5 | -12 | 3 | -12 | 2.76 | 268.72 | -38.40 | 91.07 | 0.6227 | -1479.6 | 999999 | |
| 11 | -12 | 7 | -12 | 2.78 | 268.27 | -38.85 | 91.00 | 0.6290 | -1201.5 | 999999 | |
| 7 | -12 | 5 | -12 | 3.44 | 268.19 | -38.93 | 89.92 | 0.6296 | -948.1 | 999999 | |
| 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. | |