SDO HMI 2014-11-14 01:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.23 | 54.28 | 14.99 | 35.16 | 8.63 | 3.75 | 39.90 | 279.90 | 0.6459 | -29.2 | -99.2 | |
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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 | 2.24 | 0.00 | 1.50 | 8.28 | 6.33 | 42.48 | 278.99 | 0.6789 | -652.0 | -435.3 | |
| 1.03 | 2.75 | 0.69 | 1.83 | 8.39 | 5.62 | 41.77 | 279.24 | 0.6700 | -590.8 | -427.7 | |
| 0.00 | 3.18 | 0.00 | 2.11 | 8.07 | 5.37 | 41.52 | 278.79 | 0.6665 | -648.0 | -507.2 | |
| 0.00 | 1.46 | 0.00 | 0.97 | 8.29 | 5.16 | 41.31 | 279.15 | 0.6640 | -538.0 | -591.5 | |
| 10.50 | 14.54 | 6.90 | 9.55 | 8.06 | 4.81 | 40.96 | 278.85 | 0.6592 | -862.1 | -660.9 | |
| 0.00 | 2.32 | 0.00 | 1.52 | 8.29 | 4.32 | 40.47 | 279.25 | 0.6531 | -690.0 | -614.9 | |
| 1.29 | 4.30 | 0.84 | 2.80 | 8.11 | 4.22 | 40.37 | 279.00 | 0.6516 | -817.9 | -603.0 | |
| 0.00 | 1.55 | 0.00 | 1.00 | 9.54 | 3.51 | 39.66 | 281.31 | 0.6442 | 581.0 | 415.4 | |
| 0.00 | 1.29 | 0.00 | 0.82 | 9.30 | 2.58 | 38.73 | 281.11 | 0.6315 | 492.0 | 361.1 | |
| 1.38 | 4.39 | 0.87 | 2.78 | 9.44 | 2.14 | 38.29 | 281.41 | 0.6258 | 810.2 | 626.2 | |
| 0.77 | 3.27 | 0.49 | 2.08 | 9.97 | 2.21 | 38.36 | 282.25 | 0.6277 | 796.8 | 674.6 | |
| 0.00 | 1.12 | 0.00 | 0.71 | 9.68 | 2.17 | 38.32 | 281.78 | 0.6267 | 730.0 | 557.5 | |
| 0.00 | 1.03 | 0.00 | 0.66 | 10.16 | 2.20 | 38.35 | 282.53 | 0.6279 | 754.0 | 577.9 | |
| 8.26 | 10.84 | 5.20 | 6.83 | 8.88 | 1.80 | 37.95 | 280.58 | 0.6203 | 850.4 | 554.4 | |
| 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. | |