SDO HMI 2011-11-24 10:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.33 | 69.18 | 6.68 | 37.28 | -16.45 | 266.88 | 14.43 | 217.58 | 0.3954 | 462.9 | 193.3 | |
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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 | 1.20 | 0.00 | 0.64 | -12.37 | 268.61 | 16.16 | 228.24 | 0.3661 | 809.0 | 616.6 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -12.06 | 268.56 | 16.11 | 228.80 | 0.3623 | 863.0 | 587.0 | |
| 0.00 | 1.20 | 0.00 | 0.64 | -12.49 | 268.08 | 15.63 | 227.06 | 0.3610 | 794.0 | 563.9 | |
| 0.00 | 2.14 | 0.00 | 1.13 | -12.39 | 267.89 | 15.44 | 226.90 | 0.3577 | 973.0 | 826.9 | |
| 0.00 | 2.48 | 0.00 | 1.32 | -12.94 | 267.61 | 15.16 | 225.26 | 0.3604 | 776.0 | 680.6 | |
| 0.00 | 0.77 | 0.00 | 0.41 | -12.76 | 267.53 | 15.08 | 225.49 | 0.3575 | 906.0 | 842.6 | |
| 12.33 | 40.68 | 6.68 | 22.03 | -16.90 | 267.61 | 15.16 | 218.14 | 0.4070 | 1085.0 | 470.4 | |
| 0.00 | 2.14 | 0.00 | 1.14 | -15.48 | 266.04 | 13.59 | 217.47 | 0.3739 | 864.0 | 682.2 | |
| 0.00 | 4.37 | 0.00 | 2.34 | -16.44 | 265.82 | 13.37 | 215.46 | 0.3840 | -1023.0 | -849.1 | |
| 0.00 | 3.34 | 0.00 | 1.81 | -19.27 | 264.79 | 12.34 | 209.40 | 0.4126 | 639.0 | 599.0 | |
| 0.00 | 5.22 | 0.00 | 2.80 | -17.47 | 264.40 | 11.95 | 211.02 | 0.3850 | -757.0 | -837.5 | |
| 0.00 | 2.74 | 0.00 | 1.47 | -17.24 | 264.13 | 11.68 | 210.77 | 0.3798 | -1018.0 | -934.3 | |
| 0.00 | 1.28 | 0.00 | 0.69 | -17.74 | 263.91 | 11.46 | 209.60 | 0.3848 | -1010.0 | -732.1 | |
| 0.00 | 0.51 | 0.00 | 0.27 | -15.68 | 263.07 | 10.62 | 210.67 | 0.3492 | -954.0 | -894.2 | |
| 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. | |