SDO HMI 2011-10-24 14:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63.00 | 310.19 | 42.45 | 207.18 | -21.57 | 332.10 | 33.13 | 229.33 | 0.6725 | -353.1 | -235.9 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.78 | 0.00 | 0.56 | -19.44 | 338.31 | 39.34 | 236.45 | 0.7197 | 543.0 | 439.0 | |
| 4.87 | 5.65 | 3.47 | 4.03 | -19.70 | 338.35 | 39.38 | 236.15 | 0.7216 | 538.6 | 416.9 | |
| 1.48 | 2.35 | 1.05 | 1.66 | -19.49 | 338.08 | 39.11 | 236.24 | 0.7177 | 601.4 | 476.3 | |
| 0.87 | 3.04 | 0.61 | 2.14 | -19.43 | 337.66 | 38.69 | 236.04 | 0.7130 | 521.9 | 550.8 | |
| 0.00 | 0.70 | 0.00 | 0.49 | -18.92 | 337.35 | 38.38 | 236.47 | 0.7069 | 687.0 | 555.1 | |
| 0.00 | 0.70 | 0.00 | 0.49 | -19.29 | 337.45 | 38.48 | 236.08 | 0.7101 | 289.0 | 408.0 | |
| 3.39 | 32.67 | 2.34 | 22.61 | -18.50 | 336.80 | 37.83 | 236.64 | 0.6987 | 890.4 | 676.8 | |
| 9.12 | -7.00 | 6.33 | -7.00 | -18.99 | 336.89 | 37.92 | 236.08 | 0.7026 | 898.4 | 999999 | |
| 0.00 | 1.65 | 0.00 | 1.15 | -19.64 | 336.79 | 37.82 | 235.21 | 0.7055 | 415.0 | 361.7 | |
| 0.00 | 2.78 | 0.00 | 1.90 | -19.22 | 335.76 | 36.79 | 235.04 | 0.6923 | 809.0 | 709.9 | |
| 4.08 | 259.87 | 2.71 | 172.15 | -21.66 | 331.54 | 32.57 | 228.83 | 0.6670 | -963.6 | -363.3 | |
| 0.35 | -11.00 | 0.23 | -11.00 | -21.99 | 331.47 | 32.50 | 228.37 | 0.6689 | -662.5 | 999999 | |
| 2.87 | -11.00 | 1.90 | -11.00 | -21.85 | 331.32 | 32.35 | 228.42 | 0.6663 | -835.7 | 999999 | |
| 1.39 | -11.00 | 0.92 | -11.00 | -21.58 | 331.25 | 32.28 | 228.69 | 0.6635 | -951.9 | 999999 | |
| 34.58 | -11.00 | 22.89 | -11.00 | -22.17 | 330.98 | 32.01 | 227.75 | 0.6655 | -1072.6 | 999999 | |
| 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. | |