SDO HMI 2011-06-06 04:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.37 | 164.90 | 20.24 | 87.23 | 9.30 | 336.53 | -18.25 | 62.19 | 0.3509 | -845.4 | -392.7 | |
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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 | 1.27 | 0.00 | 0.66 | 7.85 | 339.08 | -15.71 | 62.78 | 0.3030 | -912.0 | -618.5 | |
| 29.05 | 127.87 | 15.32 | 67.46 | 9.30 | 336.98 | -17.80 | 61.63 | 0.3444 | -1296.1 | -444.6 | |
| 1.45 | 1.54 | 0.76 | 0.81 | 8.16 | 336.78 | -18.00 | 64.90 | 0.3393 | -767.3 | -1004.0 | |
| 3.80 | 16.74 | 2.01 | 8.84 | 8.34 | 336.48 | -18.30 | 64.76 | 0.3450 | -1067.2 | -775.1 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 9.14 | 336.31 | -18.48 | 62.87 | 0.3531 | -39.0 | -73.8 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 11.09 | 336.13 | -18.66 | 58.32 | 0.3705 | -836.0 | -565.8 | |
| 2.62 | -4.00 | 1.39 | -4.00 | 8.19 | 336.23 | -18.56 | 65.46 | 0.3478 | -908.0 | 999999 | |
| 1.45 | 2.26 | 0.76 | 1.19 | 7.55 | 336.16 | -18.62 | 67.26 | 0.3447 | 856.1 | 672.9 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 8.16 | 335.91 | -18.88 | 65.90 | 0.3524 | -572.0 | -402.0 | |
| 0.00 | 1.63 | 0.00 | 0.87 | 9.21 | 334.02 | -20.77 | 65.25 | 0.3871 | -877.0 | -686.6 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 9.39 | 333.97 | -20.82 | 64.86 | 0.3889 | -661.0 | -555.1 | |
| 0.00 | 2.71 | 0.00 | 1.47 | 10.26 | 332.88 | -21.90 | 63.95 | 0.4103 | 729.0 | 688.6 | |
| 0.00 | 4.62 | 0.00 | 2.57 | 12.65 | 330.55 | -24.24 | 61.19 | 0.4590 | 783.0 | 573.9 | |
| 0.00 | 1.27 | 0.00 | 0.71 | 13.40 | 329.78 | -25.01 | 60.45 | 0.4746 | 861.0 | 656.9 | |
| 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. | |