SDO HMI 2014-11-30 15:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.78 | 22.23 | 8.79 | 28.51 | -14.82 | 39.20 | -66.10 | 106.61 | 0.9224 | 275.4 | 56.5 | |
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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 |
| 7.78 | 10.85 | 8.79 | 12.26 | -16.40 | 42.81 | -62.48 | 108.81 | 0.9006 | 518.5 | 283.1 | |
| 0.00 | 2.05 | 0.00 | 2.60 | -15.93 | 39.54 | -65.76 | 107.77 | 0.9224 | 369.0 | 275.1 | |
| 0.00 | 0.26 | 0.00 | 0.32 | -15.68 | 39.54 | -65.75 | 107.51 | 0.9222 | 316.0 | 318.0 | |
| 0.00 | 0.26 | 0.00 | 0.32 | -15.56 | 39.62 | -65.67 | 107.38 | 0.9215 | 349.0 | 369.7 | |
| 0.00 | 1.37 | 0.00 | 1.74 | -14.30 | 39.25 | -66.05 | 105.98 | 0.9229 | 391.0 | 362.9 | |
| 0.00 | 0.68 | 0.00 | 0.87 | -14.03 | 39.25 | -66.04 | 105.68 | 0.9226 | 447.0 | 399.9 | |
| 0.00 | 1.20 | 0.00 | 1.82 | -13.39 | 35.19 | -70.11 | 104.53 | 0.9465 | -217.0 | -234.3 | |
| 0.00 | 0.60 | 0.00 | 0.92 | -13.15 | 34.89 | -70.41 | 104.25 | 0.9479 | -319.0 | -255.1 | |
| 0.00 | 0.26 | 0.00 | 0.39 | -12.84 | 34.91 | -70.39 | 103.93 | 0.9477 | -262.0 | -251.0 | |
| 0.00 | 2.39 | 0.00 | 3.65 | -12.60 | 34.98 | -70.32 | 103.68 | 0.9472 | -392.0 | -261.7 | |
| 0.00 | 2.31 | 0.00 | 3.62 | -12.58 | 34.43 | -70.86 | 103.60 | 0.9501 | -65.0 | -19.6 | |
| 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. | |