SDO HMI 2014-11-30 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 |
| 5.30 | 31.72 | 2.80 | 16.73 | -19.04 | 108.17 | 0.68 | 181.82 | 0.3445 | 164.3 | 210.9 | |
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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 | 0.59 | -19.40 | 109.63 | 2.14 | 185.79 | 0.3514 | 883.0 | 670.2 | |
| 1.03 | 8.29 | 0.54 | 4.38 | -19.21 | 109.32 | 1.83 | 184.99 | 0.3478 | 1009.8 | 609.6 | |
| 0.00 | 1.28 | 0.00 | 0.68 | -19.52 | 109.04 | 1.55 | 184.16 | 0.3526 | 803.0 | 658.7 | |
| 4.27 | 10.00 | 2.26 | 5.28 | -19.21 | 108.82 | 1.33 | 183.63 | 0.3471 | 1014.0 | 590.4 | |
| 0.00 | 1.20 | 0.00 | 0.63 | -18.64 | 107.50 | 0.01 | 180.04 | 0.3371 | 579.0 | 474.4 | |
| 0.00 | 1.37 | 0.00 | 0.72 | -18.26 | 107.13 | -0.36 | 178.96 | 0.3309 | -718.0 | -594.2 | |
| 0.00 | 0.85 | 0.00 | 0.45 | -18.26 | 106.76 | -0.73 | 177.89 | 0.3311 | -714.0 | -490.3 | |
| 0.00 | 3.08 | 0.00 | 1.62 | -19.17 | 106.63 | -0.86 | 177.63 | 0.3462 | -1054.0 | -837.6 | |
| 0.00 | 1.80 | 0.00 | 0.94 | -17.70 | 106.42 | -1.07 | 176.81 | 0.3220 | 838.0 | 671.2 | |
| 0.00 | 1.37 | 0.00 | 0.72 | -18.92 | 105.38 | -2.11 | 174.15 | 0.3435 | -935.0 | -817.1 | |
| 0.00 | 1.37 | 0.00 | 0.72 | -19.17 | 105.37 | -2.12 | 174.22 | 0.3476 | -580.0 | -499.9 | |
| 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. | |