SDO HMI 2014-11-26 01:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.44 | 331.08 | 124.48 | 837.50 | -15.39 | 243.07 | 77.40 | 253.88 | 0.9780 | -342.4 | -64.2 | |
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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 |
| 5.31 | 23.37 | 35.80 | 169.83 | -12.86 | 251.01 | 85.34 | 256.98 | 0.9976 | -54.2 | 89.3 | |
| 0.00 | 0.86 | 0.00 | 1.88 | -11.91 | 242.01 | 76.34 | 257.40 | 0.9753 | 293.0 | 218.2 | |
| 0.00 | 1.63 | 0.00 | 3.45 | -12.87 | 241.46 | 75.79 | 256.37 | 0.9735 | -329.0 | -275.2 | |
| 6.68 | 304.19 | 14.15 | 660.15 | -14.46 | 241.36 | 75.69 | 254.74 | 0.9736 | -602.7 | -99.5 | |
| 4.97 | -4.00 | 11.34 | -4.00 | -15.47 | 242.21 | 76.54 | 253.78 | 0.9771 | -320.1 | 999999 | |
| 3.42 | -4.00 | 7.12 | -4.00 | -14.85 | 241.01 | 75.34 | 254.30 | 0.9724 | -552.2 | 999999 | |
| 2.83 | -4.00 | 5.75 | -4.00 | -15.64 | 240.62 | 74.94 | 253.46 | 0.9712 | -223.2 | 999999 | |
| 9.08 | -4.00 | 20.28 | -4.00 | -17.01 | 241.81 | 76.14 | 252.17 | 0.9763 | -261.2 | 999999 | |
| 3.94 | -4.00 | 8.40 | -4.00 | -16.71 | 241.06 | 75.39 | 252.41 | 0.9734 | -569.2 | 999999 | |
| 2.48 | -4.00 | 5.01 | -4.00 | -16.94 | 240.35 | 74.68 | 252.10 | 0.9707 | -266.2 | 999999 | |
| 8.73 | -4.00 | 16.63 | -4.00 | -16.72 | 239.42 | 73.75 | 252.22 | 0.9668 | -770.1 | 999999 | |
| 0.00 | 1.03 | 0.00 | 2.19 | -18.14 | 240.93 | 75.26 | 250.93 | 0.9734 | -81.0 | -142.9 | |
| 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. | |