SDO HMI 2014-07-10 04:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.08 | 0.00 | 7.92 | -23.50 | 197.64 | -1.77 | 177.79 | 0.4715 | -131.4 | -31.1 | |
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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 | 1.45 | 0.00 | 0.80 | -22.04 | 204.36 | 4.95 | 190.40 | 0.4453 | 823.0 | 591.6 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -22.10 | 203.93 | 4.53 | 189.49 | 0.4451 | 809.0 | 735.7 | |
| 0.00 | 1.00 | 0.00 | 0.57 | -24.71 | 203.82 | 4.41 | 188.32 | 0.4847 | -301.0 | -362.8 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -22.17 | 203.67 | 4.26 | 188.93 | 0.4455 | 762.0 | 697.4 | |
| 0.00 | 1.91 | 0.00 | 1.05 | -21.86 | 203.47 | 4.06 | 188.61 | 0.4402 | 952.0 | 792.7 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -21.98 | 196.86 | -2.55 | 174.59 | 0.4392 | -687.0 | -499.2 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -22.09 | 196.56 | -2.85 | 173.98 | 0.4413 | -876.0 | -671.8 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -22.05 | 196.26 | -3.15 | 173.36 | 0.4413 | -779.0 | -581.0 | |
| 0.00 | 0.82 | 0.00 | 0.44 | -19.17 | 195.29 | -4.12 | 170.15 | 0.3982 | -765.0 | -616.6 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -22.22 | 191.56 | -7.85 | 163.92 | 0.4583 | -797.0 | -526.5 | |
| 0.00 | 2.09 | 0.00 | 1.30 | -30.72 | 184.63 | -14.77 | 158.81 | 0.6086 | -586.0 | -507.3 | |
| 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. | |