SDO HMI 2014-12-08 00:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.94 | 0.00 | 10.50 | 16.21 | 17.55 | 9.48 | 329.82 | 0.3357 | -417.2 | -362.0 | |
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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 | 3.33 | 0.00 | 1.80 | 16.48 | 25.62 | 17.55 | 314.42 | 0.4065 | -782.0 | -552.6 | |
| 0.00 | 1.28 | 0.00 | 0.66 | 10.59 | 21.53 | 13.45 | 308.73 | 0.2944 | -760.0 | -791.7 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 16.95 | 20.99 | 12.92 | 323.69 | 0.3628 | -740.0 | -680.8 | |
| 0.00 | 1.28 | 0.00 | 0.66 | 12.52 | 18.99 | 10.92 | 319.49 | 0.2859 | -787.0 | -645.3 | |
| 0.00 | 1.53 | 0.00 | 0.80 | 13.76 | 18.74 | 10.67 | 322.88 | 0.2992 | -662.0 | -499.2 | |
| 0.00 | 1.02 | 0.00 | 0.52 | 11.31 | 17.87 | 9.80 | 319.57 | 0.2584 | -759.0 | -543.3 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 16.52 | 17.82 | 9.75 | 330.24 | 0.3285 | -902.0 | -667.5 | |
| 0.00 | 1.53 | 0.00 | 0.79 | 12.64 | 17.46 | 9.39 | 323.93 | 0.2715 | -765.0 | -578.4 | |
| 0.00 | 2.64 | 0.00 | 1.37 | 15.66 | 16.69 | 8.62 | 331.84 | 0.3071 | -715.0 | -606.6 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 15.47 | 16.50 | 8.42 | 332.08 | 0.3029 | -764.0 | -621.8 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 19.95 | 9.81 | 1.73 | 355.23 | 0.3435 | 760.0 | 629.8 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 19.29 | 8.77 | 0.69 | 358.02 | 0.3316 | 768.0 | 618.7 | |
| 0.00 | 2.30 | 0.00 | 1.25 | 24.22 | 8.73 | 0.66 | 358.54 | 0.4118 | 685.0 | 423.3 | |
| 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. | |