SDO HMI 2014-11-02 13:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.80 | 0.00 | 8.87 | -19.96 | 77.74 | -37.77 | 124.55 | 0.7008 | 551.8 | 504.2 | |
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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 | 0.61 | 0.00 | 0.39 | -21.00 | 84.52 | -30.98 | 130.91 | 0.6383 | 588.0 | 510.0 | |
| 0.00 | 0.78 | 0.00 | 0.52 | -21.26 | 80.61 | -34.90 | 128.10 | 0.6799 | 198.0 | 263.3 | |
| 0.00 | 1.04 | 0.00 | 0.69 | -20.02 | 80.55 | -34.95 | 126.50 | 0.6720 | 504.0 | 458.1 | |
| 0.00 | 0.95 | 0.00 | 0.65 | -19.96 | 79.04 | -36.46 | 125.35 | 0.6872 | 681.0 | 552.8 | |
| 0.00 | 1.04 | 0.00 | 0.71 | -19.27 | 78.48 | -37.03 | 124.09 | 0.6888 | 627.0 | 496.8 | |
| 0.00 | 1.30 | 0.00 | 0.90 | -20.43 | 77.96 | -37.55 | 125.21 | 0.7013 | 587.0 | 442.3 | |
| 0.00 | 0.26 | 0.00 | 0.18 | -20.43 | 76.62 | -38.89 | 124.34 | 0.7149 | 391.0 | 483.7 | |
| 0.00 | 1.12 | 0.00 | 0.79 | -19.94 | 76.64 | -38.86 | 123.75 | 0.7118 | 811.0 | 688.6 | |
| 0.00 | 1.64 | 0.00 | 1.16 | -19.66 | 76.44 | -39.06 | 123.28 | 0.7122 | 566.0 | 597.0 | |
| 0.00 | 0.95 | 0.00 | 0.67 | -20.02 | 76.29 | -39.21 | 123.64 | 0.7158 | 411.0 | 422.7 | |
| 0.00 | 2.16 | 0.00 | 1.53 | -19.58 | 75.97 | -39.53 | 122.90 | 0.7166 | 726.0 | 520.4 | |
| 0.00 | 0.95 | 0.00 | 0.68 | -19.63 | 75.67 | -39.84 | 122.77 | 0.7199 | 531.0 | 454.4 | |
| 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. | |