SDO HMI 2014-11-25 05:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.03 | 60.31 | 8.39 | 31.61 | 4.73 | 157.84 | -18.82 | 80.17 | 0.3277 | -149.9 | -4.3 | |
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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 |
| 1.80 | 3.94 | 0.93 | 2.03 | 4.04 | 160.50 | -16.16 | 81.17 | 0.2823 | -1164.9 | -826.0 | |
| 3.86 | 5.74 | 1.99 | 2.97 | 4.31 | 160.37 | -16.29 | 80.31 | 0.2851 | -1105.8 | -717.8 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 4.30 | 159.78 | -16.88 | 80.63 | 0.2948 | -820.0 | -706.5 | |
| 0.43 | 1.63 | 0.22 | 0.84 | 4.63 | 159.62 | -17.04 | 79.63 | 0.2983 | -732.8 | -543.4 | |
| 0.00 | 6.94 | 0.00 | 3.60 | 4.21 | 159.56 | -17.10 | 81.04 | 0.2982 | -976.0 | -822.5 | |
| 0.00 | 2.40 | 0.00 | 1.25 | 5.01 | 159.23 | -17.43 | 78.59 | 0.3057 | -1125.0 | -851.9 | |
| 1.46 | 5.74 | 0.76 | 3.00 | 5.21 | 158.29 | -18.37 | 78.50 | 0.3217 | -888.7 | -727.8 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 4.53 | 158.28 | -18.38 | 80.62 | 0.3201 | 715.0 | 708.6 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 5.36 | 158.16 | -18.50 | 78.13 | 0.3242 | -643.0 | -494.8 | |
| 0.43 | 2.48 | 0.22 | 1.30 | 5.29 | 157.88 | -18.78 | 78.47 | 0.3286 | -818.4 | -598.8 | |
| 4.54 | 9.00 | 2.40 | 4.75 | 5.85 | 156.79 | -19.87 | 77.46 | 0.3479 | 1032.0 | 715.9 | |
| 1.71 | 3.26 | 0.91 | 1.72 | 5.16 | 156.40 | -20.26 | 79.59 | 0.3522 | 1031.3 | 793.1 | |
| 0.00 | 0.86 | 0.00 | 0.45 | 4.78 | 156.35 | -20.31 | 80.70 | 0.3520 | 792.0 | 601.8 | |
| 0.43 | 5.65 | 0.23 | 2.99 | 4.21 | 155.99 | -20.67 | 82.42 | 0.3568 | 949.8 | 836.7 | |
| 1.37 | 9.42 | 0.73 | 5.01 | 4.24 | 155.54 | -21.12 | 82.49 | 0.3640 | 983.6 | 828.3 | |
| 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. | |