SDO HMI 2014-05-16 00:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.13 | 42.67 | 6.31 | 22.26 | 8.66 | 195.19 | -14.30 | 51.26 | 0.3134 | -221.7 | 134.3 | |
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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 | 0.99 | 0.00 | 0.51 | 7.25 | 198.18 | -11.31 | 48.85 | 0.2595 | -888.0 | -725.1 | |
| 5.66 | 7.72 | 2.91 | 3.97 | 8.08 | 198.03 | -11.45 | 46.86 | 0.2707 | -1148.9 | -781.7 | |
| 0.00 | 1.44 | 0.00 | 0.74 | 8.64 | 197.77 | -11.72 | 46.02 | 0.2803 | -916.0 | -638.6 | |
| 0.00 | 1.26 | 0.00 | 0.65 | 8.61 | 197.55 | -11.94 | 46.63 | 0.2826 | -833.0 | -647.5 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 8.46 | 197.30 | -12.19 | 47.60 | 0.2840 | -848.0 | -725.2 | |
| 0.00 | 2.78 | 0.00 | 1.44 | 8.56 | 197.11 | -12.38 | 47.80 | 0.2874 | -1144.0 | -818.2 | |
| 0.00 | 1.53 | 0.00 | 0.79 | 8.31 | 196.74 | -12.75 | 49.27 | 0.2894 | -831.0 | -709.9 | |
| 0.00 | 2.16 | 0.00 | 1.12 | 8.27 | 194.79 | -14.70 | 53.33 | 0.3144 | -783.0 | -676.8 | |
| 1.26 | 4.94 | 0.66 | 2.59 | 9.27 | 194.15 | -15.34 | 52.01 | 0.3328 | 1141.1 | 994.6 | |
| 1.89 | 7.63 | 0.99 | 4.02 | 9.28 | 193.73 | -15.76 | 52.73 | 0.3382 | 1033.6 | 777.5 | |
| 0.00 | 1.35 | 0.00 | 0.71 | 9.09 | 193.74 | -15.75 | 53.16 | 0.3363 | 817.0 | 618.1 | |
| 0.00 | 2.42 | 0.00 | 1.28 | 8.82 | 193.40 | -16.09 | 54.41 | 0.3382 | 833.0 | 601.2 | |
| 3.32 | 6.20 | 1.75 | 3.26 | 8.45 | 193.26 | -16.23 | 55.55 | 0.3367 | 1064.0 | 772.7 | |
| 0.00 | 1.44 | 0.00 | 0.76 | 8.90 | 191.89 | -17.60 | 56.58 | 0.3594 | 682.0 | 510.1 | |
| 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. | |