SDO HMI 2011-10-26 00:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.63 | 144.01 | 29.32 | 129.89 | -21.59 | 331.35 | 51.08 | 239.96 | 0.8375 | -237.4 | -325.5 | |
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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 |
| 8.95 | 11.03 | 9.20 | 11.35 | -18.79 | 337.53 | 57.27 | 245.35 | 0.8782 | 546.1 | 376.7 | |
| 0.00 | 1.04 | 0.00 | 1.04 | -17.78 | 336.96 | 56.69 | 246.27 | 0.8713 | 608.0 | 524.8 | |
| 0.00 | 0.61 | 0.00 | 0.62 | -19.02 | 337.25 | 56.98 | 245.00 | 0.8767 | 491.0 | 529.6 | |
| 0.00 | 0.78 | 0.00 | 0.80 | -19.49 | 337.04 | 56.77 | 244.42 | 0.8762 | 502.0 | 416.2 | |
| 0.35 | 1.65 | 0.35 | 1.66 | -19.08 | 336.70 | 56.43 | 244.76 | 0.8726 | 721.0 | 674.1 | |
| 0.00 | 1.22 | 0.00 | 1.21 | -19.17 | 336.23 | 55.97 | 244.50 | 0.8692 | 677.0 | 561.0 | |
| 0.00 | 1.30 | 0.00 | 1.25 | -20.25 | 334.62 | 54.35 | 242.76 | 0.8596 | -226.0 | -209.3 | |
| 0.00 | 1.39 | 0.00 | 1.27 | -21.00 | 332.27 | 52.00 | 241.04 | 0.8430 | -399.0 | -289.4 | |
| 0.00 | 1.30 | 0.00 | 1.18 | -20.68 | 332.01 | 51.74 | 241.29 | 0.8398 | -527.0 | -395.6 | |
| 0.00 | 1.22 | 0.00 | 1.10 | -21.56 | 331.46 | 51.19 | 240.09 | 0.8383 | -292.0 | -232.1 | |
| 3.73 | 13.03 | 3.33 | 11.59 | -21.39 | 330.92 | 50.65 | 240.05 | 0.8332 | -621.9 | -458.5 | |
| 0.00 | 1.91 | 0.00 | 1.70 | -21.71 | 330.77 | 50.50 | 239.63 | 0.8331 | -560.0 | -450.0 | |
| 1.48 | 107.53 | 1.31 | 95.12 | -22.03 | 330.62 | 50.35 | 239.21 | 0.8330 | -475.5 | -386.6 | |
| 7.30 | -13.00 | 6.42 | -13.00 | -21.93 | 330.17 | 49.90 | 239.13 | 0.8289 | -991.7 | 999999 | |
| 9.82 | -13.00 | 8.71 | -13.00 | -22.31 | 330.35 | 50.09 | 238.79 | 0.8319 | -751.7 | 999999 | |
| 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. | |