SDO HMI 2014-11-12 00:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.88 | 0.00 | 8.83 | -9.94 | 338.29 | -12.48 | 139.29 | 0.3158 | -272.2 | -243.6 | |
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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 | 1.21 | 0.00 | 0.60 | -4.52 | 351.11 | 0.34 | 182.52 | 0.1356 | 796.0 | 583.6 | |
| 0.00 | 0.95 | 0.00 | 0.48 | -7.88 | 342.60 | -8.16 | 143.79 | 0.2392 | 970.0 | 781.3 | |
| 0.00 | 1.72 | 0.00 | 0.88 | -8.00 | 342.39 | -8.38 | 143.39 | 0.2430 | 890.0 | 688.7 | |
| 0.00 | 1.55 | 0.00 | 0.81 | -11.40 | 340.55 | -10.22 | 145.36 | 0.3072 | 802.0 | 599.3 | |
| 0.00 | 1.64 | 0.00 | 0.87 | -12.27 | 336.95 | -13.82 | 138.68 | 0.3552 | -928.0 | -743.6 | |
| 0.00 | 2.15 | 0.00 | 1.14 | -12.08 | 336.83 | -13.94 | 138.10 | 0.3542 | -910.0 | -737.2 | |
| 0.00 | 1.12 | 0.00 | 0.59 | -10.34 | 336.73 | -14.04 | 134.31 | 0.3349 | -891.0 | -726.1 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -9.94 | 336.56 | -14.20 | 133.10 | 0.3325 | -838.0 | -595.3 | |
| 0.00 | 1.12 | 0.00 | 0.59 | -11.67 | 335.63 | -15.14 | 134.94 | 0.3629 | -564.0 | -406.8 | |
| 0.00 | 1.38 | 0.00 | 0.73 | -9.11 | 334.86 | -15.91 | 128.03 | 0.3451 | -831.0 | -617.3 | |
| 0.00 | 1.12 | 0.00 | 0.59 | -8.18 | 334.46 | -16.31 | 125.14 | 0.3413 | -866.0 | -654.2 | |
| 0.00 | 1.89 | 0.00 | 1.01 | -10.59 | 334.15 | -16.62 | 130.08 | 0.3690 | -897.0 | -652.3 | |
| 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. | |