SDO HMI 2014-03-09 14:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.94 | 42.36 | 1.48 | 21.18 | -11.15 | 13.56 | -5.94 | 127.32 | 0.1244 | 268.3 | 64.8 | |
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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 |
| 0.00 | 1.21 | 0.00 | 0.60 | -10.74 | 18.17 | -1.33 | 159.61 | 0.0657 | 906.0 | 717.9 | |
| 0.00 | 6.41 | 0.00 | 3.18 | -9.04 | 17.43 | -2.07 | 131.55 | 0.0480 | 966.0 | 819.0 | |
| 0.00 | 1.82 | 0.00 | 0.90 | -10.05 | 17.27 | -2.23 | 142.14 | 0.0627 | 1244.0 | 954.5 | |
| 0.00 | 0.78 | 0.00 | 0.39 | -9.66 | 17.15 | -2.35 | 136.49 | 0.0590 | 938.0 | 792.2 | |
| 0.00 | 4.16 | 0.00 | 2.07 | -10.99 | 15.81 | -3.70 | 136.16 | 0.0918 | 941.0 | 762.1 | |
| 1.04 | 2.94 | 0.52 | 1.47 | -10.99 | 15.53 | -3.97 | 134.12 | 0.0951 | 1208.1 | 966.6 | |
| 0.00 | 1.21 | 0.00 | 0.60 | -11.55 | 15.19 | -4.31 | 135.79 | 0.1062 | 903.0 | 644.3 | |
| 0.43 | 1.39 | 0.22 | 0.69 | -10.00 | 15.00 | -4.50 | 122.24 | 0.0918 | 974.8 | 879.5 | |
| 0.00 | 1.56 | 0.00 | 0.78 | -10.23 | 14.66 | -4.84 | 122.51 | 0.0989 | 1114.0 | 862.4 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -9.90 | 14.18 | -5.32 | 117.32 | 0.1032 | 769.0 | 612.8 | |
| 0.00 | 0.87 | 0.00 | 0.43 | -11.64 | 11.18 | -8.32 | 118.91 | 0.1626 | -908.0 | -620.0 | |
| 0.00 | 1.99 | 0.00 | 1.00 | -11.91 | 11.05 | -8.45 | 119.98 | 0.1668 | -840.0 | -663.0 | |
| 0.52 | 15.16 | 0.26 | 7.63 | -12.16 | 10.43 | -9.07 | 119.60 | 0.1781 | -1014.2 | -807.6 | |
| 0.95 | -13.00 | 0.48 | -13.00 | -12.40 | 10.39 | -9.11 | 120.67 | 0.1807 | -1008.5 | 999999 | |
| 0.00 | 1.82 | 0.00 | 0.92 | -12.70 | 10.31 | -9.19 | 121.90 | 0.1843 | -927.0 | -781.5 | |
| 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. | |