SDO HMI 2014-05-14 15:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.33 | 28.63 | 1.99 | 17.17 | 8.28 | 195.10 | -32.60 | 70.99 | 0.5659 | 42.1 | -106.1 | |
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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 |
| 0.99 | 2.15 | 0.58 | 1.27 | 7.73 | 196.39 | -31.31 | 71.26 | 0.5459 | -930.8 | -780.9 | |
| 0.36 | 8.08 | 0.21 | 4.78 | 8.10 | 196.21 | -31.49 | 70.71 | 0.5500 | -870.8 | -701.5 | |
| 0.00 | 2.33 | 0.00 | 1.38 | 7.70 | 196.14 | -31.56 | 71.44 | 0.5492 | -728.0 | -640.8 | |
| 0.00 | 0.99 | 0.00 | 0.59 | 7.99 | 195.86 | -31.84 | 71.09 | 0.5543 | -769.0 | -540.2 | |
| 0.36 | 2.15 | 0.21 | 1.29 | 7.70 | 195.20 | -32.50 | 71.94 | 0.5622 | -605.2 | -502.5 | |
| 0.00 | 1.17 | 0.00 | 0.71 | 8.61 | 194.46 | -33.24 | 70.77 | 0.5761 | 257.0 | 235.6 | |
| 0.00 | 2.06 | 0.00 | 1.25 | 8.40 | 194.22 | -33.48 | 71.24 | 0.5785 | 690.0 | 478.4 | |
| 0.00 | 1.62 | 0.00 | 0.98 | 9.03 | 194.05 | -33.65 | 70.31 | 0.5834 | 780.0 | 699.5 | |
| 0.00 | 0.63 | 0.00 | 0.38 | 8.41 | 193.97 | -33.73 | 71.36 | 0.5820 | 684.0 | 633.9 | |
| 0.00 | 0.99 | 0.00 | 0.60 | 9.12 | 193.86 | -33.84 | 70.25 | 0.5865 | 615.0 | 491.7 | |
| 0.00 | 0.27 | 0.00 | 0.16 | 9.00 | 193.79 | -33.91 | 70.48 | 0.5868 | 454.0 | 459.0 | |
| 1.62 | 6.19 | 0.99 | 3.78 | 8.69 | 193.79 | -33.91 | 70.98 | 0.5855 | 855.6 | 646.6 | |
| 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. | |