SDO HMI 2014-10-07 07:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.14 | 22.24 | 0.85 | 16.06 | -13.55 | 59.18 | -42.53 | 115.47 | 0.7296 | 255.6 | 284.2 | |
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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 | 2.90 | 0.00 | 2.00 | -12.83 | 61.77 | -39.94 | 115.90 | 0.6982 | 884.0 | 699.9 | |
| 0.00 | 1.41 | 0.00 | 0.97 | -13.04 | 61.49 | -40.22 | 116.02 | 0.7024 | 618.0 | 468.1 | |
| 0.00 | 0.79 | 0.00 | 0.55 | -13.51 | 61.11 | -40.60 | 116.42 | 0.7089 | 499.0 | 361.1 | |
| 0.00 | 4.92 | 0.00 | 3.43 | -12.95 | 61.06 | -40.65 | 115.66 | 0.7067 | 574.0 | 607.7 | |
| 0.00 | 0.79 | 0.00 | 0.56 | -14.17 | 60.81 | -40.91 | 117.10 | 0.7156 | 568.0 | 511.3 | |
| 0.00 | 1.05 | 0.00 | 0.76 | -15.45 | 59.92 | -41.79 | 118.23 | 0.7314 | 600.0 | 469.2 | |
| 0.00 | 0.97 | 0.00 | 0.69 | -13.01 | 59.45 | -42.27 | 114.88 | 0.7247 | 419.0 | 332.3 | |
| 0.00 | 0.79 | 0.00 | 0.58 | -13.49 | 58.16 | -43.56 | 114.84 | 0.7407 | -409.0 | -410.1 | |
| 1.14 | 3.07 | 0.85 | 2.28 | -13.31 | 57.64 | -44.07 | 114.36 | 0.7454 | -741.7 | -554.3 | |
| 0.00 | 0.88 | 0.00 | 0.66 | -13.37 | 57.24 | -44.48 | 114.25 | 0.7499 | -469.0 | -375.4 | |
| 0.00 | 1.32 | 0.00 | 0.98 | -12.25 | 57.06 | -44.65 | 112.76 | 0.7472 | -757.0 | -575.6 | |
| 0.00 | 0.97 | 0.00 | 0.75 | -15.49 | 55.84 | -45.87 | 116.18 | 0.7731 | 705.0 | 520.5 | |
| 0.00 | 1.41 | 0.00 | 1.10 | -15.64 | 55.53 | -46.19 | 116.22 | 0.7768 | 490.0 | 431.3 | |
| 0.00 | 0.97 | 0.00 | 0.75 | -14.73 | 55.79 | -45.92 | 115.24 | 0.7704 | 448.0 | 380.9 | |
| 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. | |