SDO HMI 2014-12-07 11:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.24 | 0.00 | 10.95 | 14.60 | 16.13 | 0.89 | 353.35 | 0.2659 | -588.9 | -542.6 | |
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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 | 1.11 | 0.00 | 0.58 | 13.39 | 28.29 | 13.05 | 316.35 | 0.3197 | -795.0 | -622.5 | |
| 0.00 | 1.71 | 0.00 | 0.87 | 12.64 | 21.25 | 6.01 | 334.85 | 0.2414 | -986.0 | -778.6 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 17.82 | 19.29 | 4.05 | 347.56 | 0.3134 | -930.0 | -750.1 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 18.16 | 18.02 | 2.78 | 351.55 | 0.3152 | -795.0 | -580.0 | |
| 0.00 | 1.28 | 0.00 | 0.65 | 12.65 | 17.43 | 2.19 | 350.30 | 0.2218 | -745.0 | -610.7 | |
| 0.00 | 1.96 | 0.00 | 0.99 | 12.17 | 17.39 | 2.15 | 350.06 | 0.2135 | -921.0 | -776.3 | |
| 0.00 | 4.44 | 0.00 | 2.23 | 10.06 | 17.28 | 2.04 | 348.55 | 0.1776 | -847.0 | -710.8 | |
| 0.00 | 2.81 | 0.00 | 1.43 | 13.16 | 17.16 | 1.92 | 351.81 | 0.2298 | -955.0 | -782.6 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 15.15 | 13.63 | -1.61 | 5.96 | 0.2626 | -843.0 | -716.5 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 16.19 | 13.38 | -1.87 | 6.43 | 0.2805 | -721.0 | -526.3 | |
| 0.00 | 0.68 | 0.00 | 0.35 | 16.01 | 13.22 | -2.02 | 7.03 | 0.2777 | -567.0 | -444.8 | |
| 0.00 | 1.02 | 0.00 | 0.55 | 21.79 | 10.58 | -4.66 | 11.53 | 0.3791 | 678.0 | 439.6 | |
| 0.00 | 1.45 | 0.00 | 0.82 | 24.47 | 359.05 | -16.19 | 31.58 | 0.4867 | 771.0 | 588.1 | |
| 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. | |