SDO HMI 2014-11-02 12:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.23 | 0.00 | 9.29 | -20.09 | 77.44 | -38.61 | 124.18 | 0.7101 | 620.5 | 487.2 | |
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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 | 1.21 | 0.00 | 0.78 | -20.99 | 84.55 | -31.51 | 130.45 | 0.6435 | 659.0 | 513.0 | |
| 0.00 | 0.78 | 0.00 | 0.53 | -20.02 | 78.94 | -37.12 | 124.98 | 0.6944 | 573.0 | 476.1 | |
| 0.00 | 1.30 | 0.00 | 0.90 | -20.34 | 78.24 | -37.81 | 124.93 | 0.7035 | 541.0 | 460.5 | |
| 0.00 | 1.12 | 0.00 | 0.79 | -20.36 | 77.83 | -38.22 | 124.69 | 0.7077 | 507.0 | 345.2 | |
| 0.00 | 2.08 | 0.00 | 1.48 | -20.42 | 76.55 | -39.51 | 123.96 | 0.7211 | 549.0 | 413.7 | |
| 0.00 | 1.30 | 0.00 | 0.92 | -19.90 | 76.63 | -39.43 | 123.36 | 0.7173 | 820.0 | 680.1 | |
| 0.00 | 0.52 | 0.00 | 0.37 | -19.48 | 76.50 | -39.55 | 122.77 | 0.7162 | 568.0 | 532.2 | |
| 0.00 | 1.47 | 0.00 | 1.05 | -20.01 | 76.30 | -39.75 | 123.30 | 0.7212 | 519.0 | 410.5 | |
| 0.00 | 0.69 | 0.00 | 0.49 | -19.72 | 76.35 | -39.70 | 122.97 | 0.7191 | 773.0 | 659.8 | |
| 0.00 | 1.64 | 0.00 | 1.17 | -19.54 | 75.95 | -40.10 | 122.51 | 0.7222 | 781.0 | 573.6 | |
| 0.00 | 1.12 | 0.00 | 0.81 | -19.69 | 75.66 | -40.40 | 122.52 | 0.7260 | 536.0 | 401.5 | |
| 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. | |