SDO HMI 2014-09-05 05:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.34 | 0.00 | 8.49 | 10.98 | 178.00 | 12.78 | 228.76 | 0.2752 | -102.2 | -63.2 | |
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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 | 1.61 | 0.00 | 0.88 | 4.31 | 190.41 | 25.19 | 264.73 | 0.4281 | -631.0 | -392.2 | |
| 0.00 | 0.80 | 0.00 | 0.43 | 11.52 | 187.55 | 22.33 | 282.69 | 0.3833 | -569.0 | -421.6 | |
| 0.00 | 0.80 | 0.00 | 0.43 | 11.60 | 187.09 | 21.87 | 283.10 | 0.3763 | -819.0 | -693.6 | |
| 0.00 | 1.70 | 0.00 | 0.91 | 11.74 | 186.77 | 21.55 | 283.60 | 0.3716 | -750.0 | -572.0 | |
| 0.00 | 1.61 | 0.00 | 0.86 | 11.20 | 186.69 | 21.48 | 282.18 | 0.3690 | -710.0 | -425.7 | |
| 0.00 | 0.98 | 0.00 | 0.52 | 11.89 | 186.18 | 20.97 | 284.28 | 0.3629 | -715.0 | -602.0 | |
| 0.00 | 1.34 | 0.00 | 0.71 | 10.87 | 185.84 | 20.63 | 281.63 | 0.3547 | -861.0 | -682.6 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 9.77 | 172.71 | 7.49 | 289.33 | 0.1368 | 862.0 | 679.4 | |
| 0.00 | 1.25 | 0.00 | 0.62 | 9.50 | 172.27 | 7.05 | 288.43 | 0.1282 | 773.0 | 600.2 | |
| 0.00 | 1.07 | 0.00 | 0.53 | 2.95 | 169.31 | 4.10 | 223.74 | 0.1037 | 984.0 | 818.0 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 12.08 | 166.22 | 1.01 | 348.43 | 0.0864 | 774.0 | 663.6 | |
| 0.00 | 3.40 | 0.00 | 1.71 | 16.51 | 161.17 | -4.04 | 22.72 | 0.1758 | 435.0 | 326.9 | |
| 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. | |