SDO HMI 2014-10-14 01:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.78 | 0.00 | 7.87 | 16.88 | 355.36 | -17.30 | 54.11 | 0.3427 | -463.5 | -395.0 | |
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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 | 2.71 | 0.00 | 1.38 | 14.60 | 3.58 | -9.07 | 45.26 | 0.2159 | -716.0 | -704.6 | |
| 0.00 | 1.22 | 0.00 | 0.63 | 14.69 | 0.15 | -12.51 | 53.69 | 0.2612 | -897.0 | -701.9 | |
| 0.00 | 1.75 | 0.00 | 0.90 | 14.96 | 0.04 | -12.62 | 53.07 | 0.2652 | -1025.0 | -825.2 | |
| 0.00 | 1.92 | 0.00 | 0.99 | 14.50 | 359.97 | -12.69 | 54.65 | 0.2619 | -1098.0 | -815.0 | |
| 0.00 | 0.70 | 0.00 | 0.36 | 14.35 | 359.85 | -12.81 | 55.39 | 0.2621 | -683.0 | -490.9 | |
| 0.00 | 0.79 | 0.00 | 0.41 | 15.46 | 355.87 | -16.79 | 58.71 | 0.3272 | -793.0 | -698.0 | |
| 0.00 | 1.05 | 0.00 | 0.55 | 15.64 | 355.56 | -17.10 | 58.67 | 0.3329 | -817.0 | -652.7 | |
| 0.00 | 0.70 | 0.00 | 0.37 | 16.53 | 355.12 | -17.53 | 56.94 | 0.3461 | -800.0 | -626.1 | |
| 0.00 | 2.10 | 0.00 | 1.20 | 22.11 | 346.50 | -26.15 | 54.81 | 0.5017 | 416.0 | 252.4 | |
| 0.00 | 0.70 | 0.00 | 0.40 | 20.74 | 344.46 | -28.19 | 58.90 | 0.5181 | 599.0 | 520.0 | |
| 0.00 | 1.14 | 0.00 | 0.68 | 21.43 | 340.64 | -32.02 | 60.32 | 0.5703 | 715.0 | 567.8 | |
| 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. | |