SDO HMI 2011-10-21 22:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.53 | 0.00 | 10.81 | 24.17 | 330.77 | -3.35 | 8.20 | 0.3332 | -617.5 | -477.6 | |
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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 | 1.39 | 0.00 | 0.73 | 23.19 | 336.33 | 2.21 | 353.40 | 0.3095 | -840.0 | -676.0 | |
| 0.00 | 1.22 | 0.00 | 0.63 | 20.64 | 336.07 | 1.95 | 353.12 | 0.2665 | -814.0 | -603.6 | |
| 0.00 | 1.39 | 0.00 | 0.72 | 22.07 | 335.31 | 1.19 | 356.16 | 0.2892 | -958.0 | -742.0 | |
| 0.00 | 1.31 | 0.00 | 0.68 | 22.19 | 335.18 | 1.06 | 356.60 | 0.2912 | -819.0 | -659.7 | |
| 0.00 | 2.09 | 0.00 | 1.10 | 24.86 | 332.77 | -1.35 | 3.66 | 0.3358 | -757.0 | -556.0 | |
| 0.00 | 1.13 | 0.00 | 0.58 | 20.33 | 332.72 | -1.40 | 5.07 | 0.2603 | -895.0 | -684.9 | |
| 0.00 | 1.13 | 0.00 | 0.59 | 22.78 | 330.88 | -3.24 | 9.86 | 0.3051 | -944.0 | -728.2 | |
| 0.00 | 1.13 | 0.00 | 0.60 | 24.88 | 329.71 | -4.41 | 11.79 | 0.3429 | -789.0 | -606.2 | |
| 0.00 | 0.96 | 0.00 | 0.51 | 25.23 | 329.63 | -4.49 | 11.76 | 0.3487 | -632.0 | -558.4 | |
| 0.00 | 1.65 | 0.00 | 0.87 | 25.03 | 329.51 | -4.61 | 12.21 | 0.3461 | -815.0 | -718.3 | |
| 0.00 | 1.39 | 0.00 | 0.73 | 24.75 | 329.52 | -4.60 | 12.38 | 0.3415 | -848.0 | -733.2 | |
| 0.00 | 1.13 | 0.00 | 0.59 | 24.43 | 329.53 | -4.59 | 12.57 | 0.3364 | -902.0 | -734.2 | |
| 0.00 | 1.91 | 0.00 | 1.02 | 26.95 | 329.33 | -4.79 | 11.43 | 0.3771 | -790.0 | -508.5 | |
| 0.00 | 1.22 | 0.00 | 0.66 | 26.36 | 322.86 | -11.26 | 25.93 | 0.4017 | 685.0 | 537.6 | |
| 0.00 | 1.48 | 0.00 | 0.80 | 26.10 | 322.75 | -11.37 | 26.46 | 0.3989 | 856.0 | 674.6 | |
| 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. | |