SDO HMI 2014-10-05 19:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.34 | 20.45 | 2.48 | 15.93 | -18.61 | 77.22 | -44.29 | 120.79 | 0.7710 | 251.5 | 268.2 | |
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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 | 0.97 | 0.00 | 0.73 | -22.00 | 80.75 | -40.76 | 126.72 | 0.7576 | 381.0 | 358.8 | |
| 3.34 | 7.90 | 2.48 | 5.87 | -18.20 | 79.64 | -41.87 | 121.61 | 0.7469 | 809.3 | 574.0 | |
| 0.00 | 1.23 | 0.00 | 0.89 | -15.92 | 79.77 | -41.74 | 118.91 | 0.7337 | 155.0 | 261.9 | |
| 0.00 | 1.49 | 0.00 | 1.09 | -15.43 | 79.43 | -42.08 | 118.12 | 0.7348 | 590.0 | 510.9 | |
| 0.00 | 1.05 | 0.00 | 0.78 | -16.78 | 79.03 | -42.48 | 119.56 | 0.7456 | 214.0 | 281.9 | |
| 0.00 | 0.79 | 0.00 | 0.63 | -19.52 | 75.95 | -45.56 | 121.14 | 0.7885 | 559.0 | 429.2 | |
| 0.00 | 2.02 | 0.00 | 1.56 | -16.83 | 76.80 | -44.71 | 118.43 | 0.7680 | 662.0 | 517.3 | |
| 0.00 | 0.70 | 0.00 | 0.56 | -17.21 | 75.43 | -46.08 | 118.19 | 0.7830 | 507.0 | 458.4 | |
| 0.00 | 0.79 | 0.00 | 0.64 | -18.11 | 74.76 | -46.75 | 118.92 | 0.7932 | 414.0 | 348.1 | |
| 0.00 | 0.88 | 0.00 | 0.82 | -24.10 | 70.87 | -50.64 | 123.72 | 0.8507 | -545.0 | -428.3 | |
| 0.00 | 1.23 | 0.00 | 1.13 | -22.89 | 71.10 | -50.41 | 122.53 | 0.8441 | -361.0 | -280.6 | |
| 0.00 | 0.61 | 0.00 | 0.53 | -18.93 | 72.46 | -49.05 | 118.78 | 0.8173 | -501.0 | -443.1 | |
| 0.00 | 0.79 | 0.00 | 0.70 | -20.13 | 71.21 | -50.30 | 119.56 | 0.8327 | -440.0 | -376.9 | |
| 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. | |