SDO HMI 2014-11-30 12:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.10 | 37.28 | 3.74 | 19.66 | -19.10 | 108.16 | 1.21 | 183.32 | 0.3459 | 225.9 | 67.6 | |
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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 |
| 1.03 | 6.07 | 0.54 | 3.21 | -19.24 | 109.43 | 2.48 | 186.76 | 0.3494 | 1070.2 | 850.3 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -19.05 | 109.30 | 2.36 | 186.48 | 0.3460 | 468.0 | 352.8 | |
| 0.00 | 1.28 | 0.00 | 0.68 | -19.49 | 109.18 | 2.24 | 186.01 | 0.3530 | 395.0 | 603.1 | |
| 0.00 | 0.51 | 0.00 | 0.27 | -19.55 | 108.99 | 2.05 | 185.49 | 0.3537 | 261.0 | 494.2 | |
| 6.07 | 13.08 | 3.20 | 6.90 | -19.21 | 108.93 | 1.98 | 185.41 | 0.3479 | 1018.0 | 391.1 | |
| 0.00 | 0.60 | 0.00 | 0.32 | -19.96 | 108.94 | 1.99 | 185.22 | 0.3603 | 622.0 | 505.9 | |
| 0.00 | 1.20 | 0.00 | 0.63 | -18.73 | 108.55 | 1.60 | 184.49 | 0.3397 | -411.0 | -340.2 | |
| 0.00 | 1.11 | 0.00 | 0.58 | -18.26 | 108.04 | 1.10 | 183.17 | 0.3313 | -643.0 | -460.8 | |
| 0.00 | 1.54 | 0.00 | 0.81 | -18.86 | 107.74 | 0.79 | 182.21 | 0.3409 | 903.0 | 775.4 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -18.70 | 107.55 | 0.60 | 181.70 | 0.3382 | 464.0 | 480.6 | |
| 0.00 | 1.80 | 0.00 | 0.94 | -18.26 | 107.05 | 0.11 | 180.30 | 0.3308 | -836.0 | -667.3 | |
| 0.00 | 3.42 | 0.00 | 1.80 | -19.17 | 106.64 | -0.30 | 179.17 | 0.3459 | -831.0 | -745.4 | |
| 0.00 | 4.53 | 0.00 | 2.39 | -19.04 | 105.27 | -1.68 | 175.38 | 0.3449 | -897.0 | -829.4 | |
| 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. | |