| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.31 | 223.33 | 17.04 | 129.80 | 28.23 | 42.27 | 19.65 | 325.44 | 0.5242 | -854.7 | -416.1 | |
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back to the solar disc SDO HMI 2011-11-14 13:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.86 | 208.90 | 0.50 | 121.51 | 28.62 | 42.88 | 20.26 | 325.11 | 0.5336 | -367.9 | -440.3 | |
| 0.00 | 1.46 | 0.00 | 0.84 | 26.18 | 42.39 | 19.76 | 322.62 | 0.5019 | -689.0 | -431.1 | |
| 7.39 | -1.00 | 4.31 | -1.00 | 28.36 | 42.58 | 19.96 | 325.18 | 0.5282 | -1187.3 | 999999 | |
| 15.73 | -1.00 | 9.13 | -1.00 | 28.03 | 42.48 | 19.86 | 324.90 | 0.5236 | -1351.5 | 999999 | |
| 0.86 | -1.00 | 0.50 | -1.00 | 28.43 | 42.13 | 19.51 | 325.85 | 0.5252 | -958.8 | 999999 | |
| 3.09 | -1.00 | 1.80 | -1.00 | 28.60 | 42.12 | 19.50 | 326.06 | 0.5271 | -853.2 | 999999 | |
| 1.38 | -1.00 | 0.80 | -1.00 | 28.63 | 41.85 | 19.22 | 326.46 | 0.5252 | -647.6 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.60 | 28.86 | 41.85 | 19.23 | 326.73 | 0.5279 | -609.0 | -470.5 | |
| 0.00 | 1.72 | 0.00 | 1.01 | 30.02 | 42.05 | 19.43 | 327.83 | 0.5429 | 517.0 | 347.0 | |
| 0.00 | 1.03 | 0.00 | 0.60 | 29.00 | 41.59 | 18.97 | 327.23 | 0.5274 | -722.0 | -625.8 | |
| 0.00 | 1.20 | 0.00 | 0.69 | 26.85 | 40.99 | 18.37 | 325.39 | 0.4971 | -687.0 | -630.5 | |
| 0.00 | 1.46 | 0.00 | 0.85 | 29.71 | 40.58 | 17.96 | 329.39 | 0.5280 | -727.0 | -572.4 | |
| 0.00 | 1.12 | 0.00 | 0.65 | 29.42 | 40.24 | 17.62 | 329.52 | 0.5218 | -830.0 | -671.0 | |
| 0.00 | 1.29 | 0.00 | 0.75 | 29.96 | 39.62 | 17.00 | 330.96 | 0.5239 | -817.0 | -618.7 | |
| 0.00 | 2.06 | 0.00 | 1.15 | 26.52 | 36.52 | 13.90 | 331.82 | 0.4571 | 925.0 | 766.0 | |
| 0.00 | 2.06 | 0.00 | 1.15 | 26.88 | 36.39 | 13.77 | 332.45 | 0.4609 | 805.0 | 591.7 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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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. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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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. |
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| 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. | |