SDO HMI 2014-12-05 18:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.95 | 0.00 | 11.44 | 6.96 | 83.66 | 45.92 | 279.29 | 0.7243 | -69.4 | -48.7 | |
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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 | 0.94 | 0.00 | 0.73 | 7.31 | 87.72 | 49.97 | 279.25 | 0.7719 | -576.0 | -484.0 | |
| 0.00 | 0.85 | 0.00 | 0.65 | 8.45 | 86.53 | 48.78 | 280.90 | 0.7600 | -401.0 | -354.9 | |
| 0.00 | 0.94 | 0.00 | 0.71 | 8.12 | 86.47 | 48.73 | 280.48 | 0.7590 | -523.0 | -436.2 | |
| 0.00 | 0.26 | 0.00 | 0.19 | 7.20 | 86.06 | 48.31 | 279.32 | 0.7531 | -506.0 | -439.7 | |
| 0.00 | 0.94 | 0.00 | 0.70 | 7.85 | 86.02 | 48.27 | 280.19 | 0.7536 | -562.0 | -469.9 | |
| 0.00 | 2.47 | 0.00 | 1.86 | 8.18 | 86.07 | 48.33 | 280.62 | 0.7546 | -181.0 | -263.3 | |
| 0.00 | 0.94 | 0.00 | 0.70 | 8.45 | 85.94 | 48.19 | 281.00 | 0.7534 | -716.0 | -566.5 | |
| 0.00 | 0.94 | 0.00 | 0.66 | 3.85 | 82.96 | 45.22 | 275.11 | 0.7133 | 423.0 | 395.2 | |
| 0.00 | 0.60 | 0.00 | 0.42 | 3.00 | 82.66 | 44.91 | 273.92 | 0.7090 | 453.0 | 415.4 | |
| 0.00 | 2.81 | 0.00 | 1.96 | 5.99 | 82.23 | 44.48 | 278.20 | 0.7064 | 523.0 | 352.5 | |
| 0.00 | 0.85 | 0.00 | 0.61 | 12.34 | 82.97 | 45.22 | 286.84 | 0.7268 | -494.0 | -393.4 | |
| 0.00 | 0.77 | 0.00 | 0.52 | 7.10 | 80.33 | 42.59 | 280.10 | 0.6844 | -438.0 | -338.6 | |
| 0.00 | 0.94 | 0.00 | 0.62 | 5.18 | 78.70 | 40.96 | 277.51 | 0.6608 | 647.0 | 538.2 | |
| 0.00 | 1.02 | 0.00 | 0.67 | 4.29 | 78.52 | 40.77 | 276.19 | 0.6574 | 639.0 | 490.4 | |
| 0.00 | 0.68 | 0.00 | 0.44 | 4.88 | 77.74 | 40.00 | 277.20 | 0.6478 | 671.0 | 601.6 | |
| 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. | |