SDO HMI 2011-11-25 02:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.64 | 53.43 | 10.11 | 30.44 | -16.23 | 267.35 | 23.71 | 231.70 | 0.4952 | 472.6 | 348.8 | |
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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 | 1.71 | 0.00 | 0.97 | -12.26 | 268.77 | 25.13 | 240.14 | 0.4805 | 694.0 | 582.5 | |
| 0.00 | 1.11 | 0.00 | 0.63 | -12.65 | 268.21 | 24.57 | 238.88 | 0.4759 | 576.0 | 413.8 | |
| 0.00 | 1.54 | 0.00 | 0.87 | -12.56 | 268.00 | 24.36 | 238.85 | 0.4724 | 688.0 | 606.4 | |
| 0.00 | 4.11 | 0.00 | 2.30 | -12.28 | 267.84 | 24.20 | 239.20 | 0.4683 | 981.0 | 843.8 | |
| 0.00 | 1.11 | 0.00 | 0.62 | -12.52 | 267.80 | 24.16 | 238.70 | 0.4695 | 716.0 | 617.4 | |
| 1.03 | 38.11 | 0.59 | 21.83 | -16.91 | 267.98 | 24.34 | 231.27 | 0.5076 | 609.8 | 473.5 | |
| 12.76 | -6.00 | 7.32 | -6.00 | -16.94 | 267.78 | 24.14 | 231.01 | 0.5055 | 969.0 | 999999 | |
| 3.85 | -6.00 | 2.20 | -6.00 | -16.65 | 267.54 | 23.90 | 231.20 | 0.5002 | 1053.3 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -17.84 | 264.94 | 21.30 | 226.15 | 0.4816 | -856.0 | -692.6 | |
| 0.00 | 1.46 | 0.00 | 0.82 | -17.62 | 264.78 | 21.14 | 226.29 | 0.4775 | -871.0 | -717.4 | |
| 0.00 | 1.11 | 0.00 | 0.63 | -18.37 | 264.71 | 21.07 | 225.01 | 0.4844 | -688.0 | -530.0 | |
| 0.00 | 0.77 | 0.00 | 0.43 | -19.77 | 262.55 | 18.91 | 219.94 | 0.4771 | -606.0 | -503.8 | |
| 0.00 | 1.37 | 0.00 | 0.76 | -18.46 | 260.56 | 16.92 | 218.82 | 0.4422 | -900.0 | -784.1 | |
| 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. | |