SDO HMI 2011-03-02 11:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.67 | 51.00 | 7.53 | 26.32 | -23.24 | 180.51 | 1.80 | 186.35 | 0.2806 | -98.8 | -390.2 | |
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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 |
| 12.51 | 15.62 | 6.42 | 8.01 | -21.73 | 182.72 | 4.01 | 194.53 | 0.2603 | 1096.4 | 793.5 | |
| 0.00 | 1.64 | 0.00 | 0.86 | -25.67 | 182.48 | 3.77 | 190.61 | 0.3236 | 851.0 | 639.4 | |
| 0.00 | 3.97 | 0.00 | 2.04 | -22.01 | 181.70 | 2.99 | 190.73 | 0.2612 | 977.0 | 854.7 | |
| 1.38 | 9.75 | 0.71 | 5.04 | -23.62 | 179.92 | 1.21 | 183.93 | 0.2844 | -1138.6 | -861.1 | |
| 0.00 | 1.38 | 0.00 | 0.71 | -23.41 | 179.76 | 1.05 | 183.45 | 0.2806 | -1035.0 | -807.4 | |
| 0.00 | 2.42 | 0.00 | 1.25 | -23.93 | 179.73 | 1.02 | 183.24 | 0.2894 | -868.0 | -761.4 | |
| 0.00 | 0.69 | 0.00 | 0.36 | -23.72 | 179.50 | 0.79 | 182.55 | 0.2856 | -694.0 | -562.0 | |
| 0.00 | 1.64 | 0.00 | 0.85 | -24.96 | 179.28 | 0.57 | 181.69 | 0.3063 | -772.0 | -676.5 | |
| 0.00 | 1.73 | 0.00 | 0.90 | -24.74 | 179.01 | 0.31 | 180.93 | 0.3025 | -907.0 | -667.7 | |
| 0.00 | 1.81 | 0.00 | 0.94 | -24.03 | 178.69 | -0.02 | 179.94 | 0.2905 | -1205.0 | -903.0 | |
| 0.00 | 2.76 | 0.00 | 1.43 | -24.18 | 178.52 | -0.18 | 179.43 | 0.2931 | -813.0 | -674.1 | |
| 0.00 | 2.07 | 0.00 | 1.07 | -24.43 | 178.33 | -0.38 | 178.84 | 0.2973 | -982.0 | -645.6 | |
| 0.00 | 0.95 | 0.00 | 0.49 | -23.84 | 178.26 | -0.44 | 178.59 | 0.2875 | -814.0 | -630.9 | |
| 0.78 | 2.33 | 0.40 | 1.21 | -24.37 | 178.13 | -0.57 | 178.23 | 0.2964 | -839.0 | -791.1 | |
| 0.00 | 2.24 | 0.00 | 1.16 | -24.62 | 177.35 | -1.36 | 175.88 | 0.3012 | -823.0 | -690.5 | |
| 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. | |