SDO HMI 2014-10-06 03:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.21 | 28.93 | 4.05 | 15.83 | 12.51 | 92.86 | -24.24 | 73.91 | 0.4183 | -104.3 | -170.9 | |
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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 | 2.55 | 0.00 | 1.31 | 9.79 | 102.25 | -14.85 | 76.30 | 0.2612 | -700.0 | -709.0 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 10.88 | 100.42 | -16.68 | 73.87 | 0.2948 | -915.0 | -787.7 | |
| 0.00 | 1.41 | 0.00 | 0.73 | 11.06 | 99.38 | -17.72 | 74.08 | 0.3119 | -763.0 | -556.8 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 13.22 | 99.11 | -17.99 | 67.78 | 0.3263 | -875.0 | -649.0 | |
| 0.00 | 2.11 | 0.00 | 1.11 | 13.85 | 98.93 | -18.17 | 66.15 | 0.3325 | -340.0 | -443.0 | |
| 0.00 | 1.32 | 0.00 | 0.70 | 10.43 | 96.88 | -20.23 | 77.43 | 0.3499 | -795.0 | -636.5 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 10.27 | 96.76 | -20.34 | 77.92 | 0.3514 | -667.0 | -561.3 | |
| 0.00 | 0.62 | 0.00 | 0.33 | 14.60 | 95.44 | -21.66 | 67.34 | 0.3887 | -548.0 | -537.9 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 11.15 | 95.38 | -21.72 | 76.16 | 0.3755 | -667.0 | -537.7 | |
| 0.00 | 1.32 | 0.00 | 0.73 | 16.67 | 91.86 | -25.24 | 65.36 | 0.4513 | 615.0 | 496.2 | |
| 0.00 | 1.41 | 0.00 | 0.77 | 4.79 | 91.39 | -25.71 | 92.41 | 0.4345 | -763.0 | -527.6 | |
| 7.21 | 11.51 | 4.05 | 6.47 | 13.33 | 89.32 | -27.78 | 73.78 | 0.4743 | 1031.5 | 699.8 | |
| 0.00 | 0.88 | 0.00 | 0.51 | 18.10 | 86.20 | -30.90 | 66.05 | 0.5362 | 450.0 | 423.3 | |
| 0.00 | 0.88 | 0.00 | 0.52 | 15.50 | 84.03 | -33.07 | 71.64 | 0.5562 | 582.0 | 436.8 | |
| 0.00 | 0.88 | 0.00 | 0.53 | 11.90 | 82.34 | -34.76 | 78.42 | 0.5717 | -675.0 | -583.3 | |
| 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. | |