SDO HMI 2014-11-07 01:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.13 | 132.41 | 25.95 | 135.66 | 13.43 | 117.28 | 61.14 | 283.24 | 0.8766 | -437.8 | -186.7 | |
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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 | 0.86 | 0.00 | 0.97 | 13.73 | 120.14 | 64.00 | 283.45 | 0.8996 | -342.0 | -290.7 | |
| 22.88 | 112.82 | 23.98 | 118.28 | 13.98 | 118.02 | 61.88 | 283.84 | 0.8834 | -673.2 | -206.8 | |
| 0.00 | 1.29 | 0.00 | 1.16 | 7.70 | 112.63 | 56.49 | 276.74 | 0.8342 | -352.0 | -293.1 | |
| 1.38 | 5.87 | 1.23 | 5.22 | 8.07 | 112.44 | 56.30 | 277.19 | 0.8324 | -647.4 | -479.3 | |
| 0.00 | 1.64 | 0.00 | 1.52 | 13.33 | 113.82 | 57.68 | 283.39 | 0.8474 | -314.0 | -309.2 | |
| 0.35 | 1.38 | 0.30 | 1.22 | 7.90 | 112.18 | 56.04 | 276.99 | 0.8299 | -717.2 | -711.8 | |
| 0.00 | 1.04 | 0.00 | 0.93 | 11.55 | 112.53 | 56.39 | 281.37 | 0.8345 | 391.0 | 307.5 | |
| 0.00 | 0.69 | 0.00 | 0.61 | 12.87 | 112.25 | 56.11 | 282.98 | 0.8326 | 454.0 | 400.4 | |
| 0.52 | 3.71 | 0.44 | 3.15 | 8.39 | 110.48 | 54.34 | 277.62 | 0.8132 | 565.8 | 388.8 | |
| 0.00 | 0.78 | 0.00 | 0.66 | 10.92 | 110.36 | 54.22 | 280.74 | 0.8131 | 442.0 | 364.0 | |
| 0.00 | 1.12 | 0.00 | 0.94 | 10.78 | 110.02 | 53.88 | 280.60 | 0.8095 | 529.0 | 439.0 | |
| 0.00 | 1.21 | 0.00 | 1.00 | 12.28 | 109.10 | 52.96 | 282.54 | 0.8013 | 508.0 | 441.1 | |
| 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. | |