SDO HMI 2014-05-19 19:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.99 | 32.20 | 4.91 | 17.44 | 9.90 | 180.03 | 20.68 | 300.97 | 0.4079 | -230.8 | -212.7 | |
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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 | 1.08 | 0.00 | 0.59 | 7.42 | 183.02 | 23.67 | 292.29 | 0.4321 | -895.0 | -735.8 | |
| 0.00 | 1.35 | 0.00 | 0.74 | 11.65 | 181.76 | 22.41 | 302.27 | 0.4434 | -799.0 | -652.9 | |
| 3.78 | 19.87 | 2.06 | 10.84 | 9.16 | 181.40 | 22.05 | 297.55 | 0.4198 | -1056.6 | -746.7 | |
| 5.21 | -3.00 | 2.85 | -3.00 | 9.43 | 181.35 | 22.00 | 298.20 | 0.4211 | -1061.1 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.44 | 12.25 | 180.08 | 20.73 | 305.46 | 0.4264 | -641.0 | -525.7 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 6.77 | 178.13 | 18.78 | 295.60 | 0.3561 | 589.0 | 568.5 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 10.36 | 178.29 | 18.94 | 303.90 | 0.3864 | 704.0 | 613.8 | |
| 0.00 | 1.35 | 0.00 | 0.72 | 10.42 | 178.07 | 18.72 | 304.34 | 0.3839 | 710.0 | 560.7 | |
| 0.00 | 1.62 | 0.00 | 0.88 | 14.33 | 177.64 | 18.29 | 312.83 | 0.4163 | 620.0 | 520.6 | |
| 0.00 | 1.17 | 0.00 | 0.62 | 9.83 | 175.87 | 16.52 | 306.35 | 0.3493 | 839.0 | 729.7 | |
| 0.00 | 3.06 | 0.00 | 1.61 | 11.59 | 174.04 | 14.69 | 313.58 | 0.3444 | 864.0 | 623.5 | |
| 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. | |