SDO HMI 2011-10-05 12:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.56 | 219.64 | 22.18 | 117.09 | -11.73 | 178.82 | -11.88 | 147.09 | 0.3719 | 528.8 | 309.8 | |
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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 |
| 0.88 | 187.83 | 0.47 | 99.83 | -11.86 | 179.50 | -11.21 | 148.71 | 0.3677 | 835.9 | 426.3 | |
| 1.23 | -1.00 | 0.66 | -1.00 | -11.83 | 179.31 | -11.39 | 148.25 | 0.3689 | 781.5 | 999999 | |
| 33.03 | -1.00 | 17.56 | -1.00 | -11.52 | 179.26 | -11.44 | 147.67 | 0.3650 | 1191.9 | 999999 | |
| 0.00 | 2.37 | 0.00 | 1.28 | -13.33 | 178.99 | -11.71 | 149.62 | 0.3923 | 646.0 | 501.2 | |
| 1.32 | 4.30 | 0.70 | 2.30 | -12.04 | 178.49 | -12.22 | 146.74 | 0.3789 | 611.4 | 508.3 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -11.99 | 178.27 | -12.43 | 146.19 | 0.3801 | 228.0 | 331.4 | |
| 0.00 | 0.53 | 0.00 | 0.28 | -12.28 | 177.78 | -12.92 | 145.61 | 0.3884 | 332.0 | 254.2 | |
| 0.00 | 1.41 | 0.00 | 0.76 | -12.36 | 177.21 | -13.49 | 144.57 | 0.3947 | -765.0 | -550.6 | |
| 0.00 | 4.57 | 0.00 | 2.47 | -12.56 | 176.82 | -13.88 | 144.09 | 0.4009 | -888.0 | -581.9 | |
| 0.00 | 7.56 | 0.00 | 4.10 | -12.89 | 176.55 | -14.15 | 144.05 | 0.4077 | -786.0 | -742.3 | |
| 0.00 | 1.58 | 0.00 | 0.87 | -14.27 | 174.19 | -16.51 | 141.80 | 0.4473 | -826.0 | -693.1 | |
| 0.00 | 1.41 | 0.00 | 0.78 | -14.41 | 173.95 | -16.75 | 141.60 | 0.4513 | -687.0 | -547.3 | |
| 2.64 | 3.25 | 1.44 | 1.78 | -12.16 | 173.63 | -17.07 | 137.67 | 0.4279 | -959.1 | -925.6 | |
| 2.46 | 2.81 | 1.35 | 1.54 | -12.60 | 173.54 | -17.17 | 138.22 | 0.4341 | -884.6 | -847.2 | |
| 0.00 | 1.23 | 0.00 | 0.68 | -13.15 | 173.30 | -17.40 | 138.68 | 0.4429 | -765.0 | -659.6 | |
| 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. | |