SDO HMI 2014-11-02 14:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.56 | 0.00 | 10.58 | -19.90 | 78.58 | -36.38 | 125.46 | 0.6858 | 593.2 | 487.6 | |
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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 |
| 0.00 | 1.21 | 0.00 | 0.77 | -21.01 | 84.57 | -30.39 | 131.44 | 0.6323 | 642.0 | 507.7 | |
| 0.00 | 1.64 | 0.00 | 1.03 | -18.23 | 84.13 | -30.82 | 127.41 | 0.6150 | 443.0 | 296.4 | |
| 0.00 | 0.86 | 0.00 | 0.56 | -21.15 | 82.63 | -32.33 | 129.97 | 0.6531 | 537.0 | 435.7 | |
| 0.00 | 1.38 | 0.00 | 0.93 | -19.96 | 79.05 | -35.91 | 125.74 | 0.6815 | 676.0 | 561.6 | |
| 0.00 | 0.95 | 0.00 | 0.65 | -20.14 | 78.60 | -36.35 | 125.66 | 0.6873 | 554.0 | 441.5 | |
| 0.00 | 1.73 | 0.00 | 1.19 | -20.43 | 77.97 | -36.99 | 125.59 | 0.6956 | 604.0 | 464.2 | |
| 0.00 | 1.30 | 0.00 | 0.91 | -20.43 | 76.56 | -38.39 | 124.66 | 0.7099 | 531.0 | 412.1 | |
| 0.00 | 1.12 | 0.00 | 0.78 | -19.91 | 76.68 | -38.28 | 124.08 | 0.7056 | 777.0 | 691.5 | |
| 0.00 | 1.30 | 0.00 | 0.90 | -19.46 | 76.64 | -38.31 | 123.49 | 0.7033 | 361.0 | 414.6 | |
| 0.00 | 1.21 | 0.00 | 0.85 | -19.69 | 76.41 | -38.54 | 123.65 | 0.7071 | 706.0 | 612.6 | |
| 0.00 | 1.82 | 0.00 | 1.28 | -19.59 | 75.96 | -39.00 | 123.23 | 0.7111 | 685.0 | 569.6 | |
| 0.00 | 1.04 | 0.00 | 0.73 | -19.63 | 75.70 | -39.26 | 123.12 | 0.7140 | 603.0 | 438.5 | |
| 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. | |