SDO HMI 2014-10-06 02:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.93 | 0.00 | 10.79 | -18.14 | 77.55 | -40.10 | 122.65 | 0.7278 | 429.7 | 511.4 | |
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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 | 1.32 | 0.00 | 0.91 | -20.64 | 82.41 | -35.24 | 128.95 | 0.6966 | 667.0 | 593.6 | |
| 0.00 | 4.92 | 0.00 | 3.44 | -18.15 | 79.61 | -38.03 | 123.94 | 0.7080 | 889.0 | 706.7 | |
| 0.00 | 1.58 | 0.00 | 1.08 | -15.20 | 79.68 | -37.97 | 120.25 | 0.6897 | 749.0 | 648.9 | |
| 0.00 | 1.05 | 0.00 | 0.75 | -16.35 | 77.15 | -40.50 | 120.16 | 0.7230 | 584.0 | 517.2 | |
| 0.00 | 0.79 | 0.00 | 0.57 | -16.82 | 76.95 | -40.70 | 120.61 | 0.7277 | 671.0 | 584.7 | |
| 0.00 | 0.53 | 0.00 | 0.38 | -16.41 | 76.35 | -41.30 | 119.76 | 0.7317 | 469.0 | 353.8 | |
| 0.00 | 1.85 | 0.00 | 1.34 | -16.81 | 76.20 | -41.45 | 120.17 | 0.7353 | 661.0 | 555.9 | |
| 0.00 | 1.05 | 0.00 | 0.80 | -19.44 | 75.20 | -42.45 | 122.74 | 0.7590 | 485.0 | 428.1 | |
| 0.00 | 0.79 | 0.00 | 0.58 | -17.06 | 75.58 | -42.07 | 120.11 | 0.7428 | 432.0 | 383.6 | |
| 0.00 | 0.26 | 0.00 | 0.21 | -18.93 | 72.64 | -45.01 | 120.73 | 0.7806 | -514.0 | -536.7 | |
| 0.00 | 0.79 | 0.00 | 0.73 | -24.80 | 68.14 | -49.51 | 125.00 | 0.8448 | -366.0 | -288.6 | |
| 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. | |