SDO HMI 2014-07-17 08:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 11.45 | 0.00 | 8.98 | -20.62 | 149.04 | 44.46 | 238.11 | 0.7756 | 77.3 | 109.3 | |
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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 | 1.18 | 0.00 | 1.06 | -20.18 | 156.58 | 52.00 | 242.22 | 0.8380 | 481.0 | 417.3 | |
| 0.00 | 0.82 | 0.00 | 0.74 | -20.45 | 156.60 | 52.02 | 241.93 | 0.8391 | 372.0 | 325.3 | |
| 0.00 | 1.36 | 0.00 | 1.04 | -9.05 | 152.19 | 47.61 | 253.98 | 0.7611 | 549.0 | 447.1 | |
| 0.00 | 1.09 | 0.00 | 0.90 | -18.86 | 153.07 | 48.48 | 242.30 | 0.8024 | 276.0 | 235.4 | |
| 0.00 | 1.00 | 0.00 | 0.76 | -18.79 | 148.50 | 43.92 | 240.28 | 0.7585 | 454.0 | 315.1 | |
| 0.00 | 1.36 | 0.00 | 1.06 | -21.36 | 148.74 | 44.15 | 237.33 | 0.7729 | 494.0 | 417.2 | |
| 0.00 | 0.91 | 0.00 | 0.70 | -21.42 | 148.53 | 43.95 | 237.16 | 0.7712 | 291.0 | 247.5 | |
| 0.00 | 1.00 | 0.00 | 0.75 | -22.93 | 146.04 | 41.46 | 234.00 | 0.7560 | -454.0 | -385.7 | |
| 0.00 | 1.09 | 0.00 | 0.79 | -26.78 | 140.60 | 36.02 | 226.04 | 0.7316 | -581.0 | -471.2 | |
| 0.00 | 0.91 | 0.00 | 0.66 | -26.91 | 140.48 | 35.90 | 225.80 | 0.7315 | -561.0 | -518.9 | |
| 0.00 | 0.73 | 0.00 | 0.52 | -27.31 | 139.78 | 35.20 | 224.85 | 0.7284 | -471.0 | -436.1 | |
| 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. | |