SDO HMI 2014-11-07 13:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.59 | 19.08 | 1.64 | 11.85 | -15.94 | 18.10 | -31.48 | 123.39 | 0.6002 | -47.1 | -88.3 | |
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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 | 1.12 | 0.00 | 0.62 | -12.37 | 27.47 | -22.11 | 126.53 | 0.4594 | 776.0 | 620.6 | |
| 0.00 | 1.04 | 0.00 | 0.59 | -14.47 | 25.56 | -24.02 | 127.88 | 0.5013 | 821.0 | 648.1 | |
| 0.00 | 1.29 | 0.00 | 0.74 | -14.66 | 25.50 | -24.07 | 128.12 | 0.5037 | 529.0 | 396.1 | |
| 0.00 | 0.95 | 0.00 | 0.56 | -14.36 | 22.75 | -26.83 | 124.76 | 0.5343 | 733.0 | 583.7 | |
| 0.00 | 1.47 | 0.00 | 0.86 | -14.14 | 22.78 | -26.80 | 124.44 | 0.5322 | 739.0 | 492.6 | |
| 0.00 | 0.95 | 0.00 | 0.59 | -18.18 | 18.66 | -30.92 | 126.72 | 0.6113 | 664.0 | 534.0 | |
| 0.00 | 0.95 | 0.00 | 0.59 | -15.17 | 17.14 | -32.44 | 121.22 | 0.6076 | 483.0 | 371.9 | |
| 0.00 | 1.04 | 0.00 | 0.66 | -17.25 | 16.26 | -33.31 | 123.52 | 0.6315 | -656.0 | -588.8 | |
| 0.00 | 1.04 | 0.00 | 0.66 | -16.45 | 16.42 | -33.15 | 122.53 | 0.6244 | -807.0 | -617.3 | |
| 0.00 | 1.38 | 0.00 | 0.88 | -16.58 | 16.21 | -33.37 | 122.56 | 0.6277 | -839.0 | -743.2 | |
| 2.59 | 4.14 | 1.64 | 2.63 | -16.18 | 15.99 | -33.58 | 121.84 | 0.6276 | -909.1 | -742.9 | |
| 0.00 | 1.12 | 0.00 | 0.74 | -18.68 | 14.66 | -34.92 | 124.29 | 0.6587 | -612.0 | -497.5 | |
| 0.00 | 1.21 | 0.00 | 0.79 | -17.20 | 14.08 | -35.50 | 121.91 | 0.6558 | -531.0 | -419.3 | |
| 0.00 | 1.38 | 0.00 | 0.94 | -16.13 | 10.78 | -38.80 | 118.42 | 0.6868 | -498.0 | -397.8 | |
| 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. | |