SDO HMI 2011-10-11 18:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 100.08 | 591.96 | 80.49 | 474.96 | 26.88 | 58.27 | -49.96 | 60.36 | 0.7877 | -909.0 | -254.6 | |
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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 | 0.61 | 0.00 | 0.47 | 24.97 | 59.97 | -48.27 | 62.30 | 0.7664 | 581.0 | 500.7 | |
| 92.30 | 575.08 | 73.54 | 459.41 | 26.96 | 58.54 | -49.69 | 60.20 | 0.7855 | -1107.5 | -272.2 | |
| 0.70 | -2.00 | 0.57 | -2.00 | 27.45 | 57.71 | -50.53 | 59.83 | 0.7945 | -269.8 | 999999 | |
| 1.14 | -2.00 | 0.93 | -2.00 | 27.43 | 57.40 | -50.83 | 59.95 | 0.7972 | -308.2 | 999999 | |
| 0.96 | -2.00 | 0.78 | -2.00 | 27.02 | 57.61 | -50.63 | 60.39 | 0.7943 | -232.8 | 999999 | |
| 1.57 | -2.00 | 1.26 | -2.00 | 26.18 | 58.07 | -50.17 | 61.31 | 0.7879 | -482.6 | 999999 | |
| 0.79 | -2.00 | 0.64 | -2.00 | 26.47 | 57.63 | -50.60 | 61.07 | 0.7927 | -399.6 | 999999 | |
| 0.00 | 4.81 | 0.00 | 3.80 | 24.95 | 58.46 | -49.77 | 62.73 | 0.7811 | 576.0 | 406.7 | |
| 0.00 | 1.57 | 0.00 | 1.26 | 24.96 | 57.84 | -50.40 | 62.88 | 0.7871 | 410.0 | 390.5 | |
| 0.00 | 0.70 | 0.00 | 0.58 | 26.84 | 56.16 | -52.08 | 60.99 | 0.8071 | -359.0 | -285.5 | |
| 0.00 | 1.14 | 0.00 | 0.99 | 27.35 | 54.35 | -53.88 | 60.81 | 0.8241 | -579.0 | -490.9 | |
| 0.00 | 0.70 | 0.00 | 0.56 | 20.57 | 57.01 | -51.23 | 68.55 | 0.7865 | -554.0 | -468.0 | |
| 0.00 | 1.49 | 0.00 | 1.63 | 26.18 | 45.17 | -63.07 | 63.71 | 0.8943 | 410.0 | 362.2 | |
| 2.62 | 4.81 | 2.77 | 5.08 | 23.55 | 46.17 | -62.07 | 66.55 | 0.8848 | 541.1 | 402.7 | |
| 0.00 | 1.05 | 0.00 | 1.18 | 23.36 | 44.15 | -64.09 | 66.95 | 0.8992 | 513.0 | 458.6 | |
| 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. | |