SDO HMI 2014-04-06 19:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.71 | 0.00 | 8.65 | -15.66 | 353.98 | -13.55 | 127.36 | 0.2950 | -670.4 | -537.6 | |
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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 | 1.06 | 0.00 | 0.54 | -22.48 | 8.83 | 1.30 | 184.28 | 0.2820 | 849.0 | 562.4 | |
| 0.00 | 1.85 | 0.00 | 0.95 | -17.38 | 356.51 | -11.03 | 136.96 | 0.2687 | -934.0 | -800.4 | |
| 0.00 | 1.23 | 0.00 | 0.63 | -13.31 | 355.53 | -12.00 | 121.88 | 0.2394 | -714.0 | -569.2 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -18.11 | 354.85 | -12.69 | 134.97 | 0.2964 | -861.0 | -630.0 | |
| 0.00 | 1.94 | 0.00 | 1.00 | -18.38 | 354.76 | -12.77 | 135.47 | 0.3005 | -651.0 | -366.0 | |
| 0.00 | 1.32 | 0.00 | 0.67 | -11.49 | 354.74 | -12.79 | 113.52 | 0.2377 | -804.0 | -638.9 | |
| 0.00 | 1.58 | 0.00 | 0.82 | -15.81 | 353.41 | -14.13 | 125.86 | 0.2911 | -840.0 | -636.1 | |
| 0.00 | 1.76 | 0.00 | 0.91 | -15.71 | 352.93 | -14.60 | 124.72 | 0.2966 | -984.0 | -726.0 | |
| 0.00 | 0.70 | 0.00 | 0.37 | -17.24 | 352.03 | -15.50 | 127.36 | 0.3226 | -840.0 | -715.0 | |
| 0.00 | 1.58 | 0.00 | 0.82 | -9.82 | 350.12 | -17.41 | 102.92 | 0.3039 | -653.0 | -490.4 | |
| 0.00 | 1.14 | 0.00 | 0.60 | -14.28 | 349.19 | -18.34 | 115.52 | 0.3394 | -837.0 | -642.2 | |
| 0.00 | 0.70 | 0.00 | 0.37 | -15.70 | 348.80 | -18.73 | 118.83 | 0.3545 | -573.0 | -486.9 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -15.64 | 348.11 | -19.42 | 117.92 | 0.3639 | -873.0 | -671.7 | |
| 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. | |