SDO HMI 2014-03-09 13:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.22 | 41.42 | 0.60 | 20.68 | -10.99 | 14.25 | -5.80 | 125.80 | 0.1206 | 507.8 | 263.3 | |
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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 | 1.82 | 0.00 | 0.90 | -10.76 | 18.15 | -1.90 | 152.12 | 0.0701 | 935.0 | 672.7 | |
| 0.00 | 5.63 | 0.00 | 2.79 | -9.03 | 17.44 | -2.61 | 125.01 | 0.0553 | 871.0 | 830.9 | |
| 0.00 | 1.91 | 0.00 | 0.95 | -10.04 | 17.21 | -2.84 | 135.29 | 0.0696 | 1210.0 | 1010.1 | |
| 0.00 | 1.30 | 0.00 | 0.65 | -10.16 | 16.91 | -3.14 | 133.57 | 0.0747 | 959.0 | 788.7 | |
| 0.00 | 4.07 | 0.00 | 2.03 | -11.01 | 15.81 | -4.24 | 132.40 | 0.0988 | 1010.0 | 818.8 | |
| 0.87 | 2.86 | 0.43 | 1.42 | -10.95 | 15.44 | -4.61 | 129.62 | 0.1028 | 1172.6 | 963.7 | |
| 0.00 | 1.47 | 0.00 | 0.73 | -11.57 | 15.19 | -4.86 | 132.54 | 0.1132 | 953.0 | 818.5 | |
| 0.35 | 3.21 | 0.17 | 1.60 | -10.02 | 14.94 | -5.11 | 119.28 | 0.1010 | 1080.5 | 863.2 | |
| 0.00 | 1.91 | 0.00 | 0.95 | -11.15 | 14.86 | -5.19 | 127.83 | 0.1128 | 817.0 | 641.4 | |
| 0.00 | 2.43 | 0.00 | 1.21 | -10.22 | 14.61 | -5.44 | 119.48 | 0.1078 | 1146.0 | 911.7 | |
| 0.00 | 1.56 | 0.00 | 0.78 | -11.47 | 14.46 | -5.59 | 128.00 | 0.1217 | 904.0 | 673.4 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -11.69 | 11.45 | -8.60 | 118.42 | 0.1672 | -804.0 | -575.9 | |
| 0.00 | 4.85 | 0.00 | 2.44 | -12.12 | 10.48 | -9.57 | 118.16 | 0.1851 | -952.0 | -918.5 | |
| 0.00 | 5.28 | 0.00 | 2.66 | -12.42 | 10.44 | -9.61 | 119.48 | 0.1881 | -1114.0 | -906.8 | |
| 0.00 | 1.91 | 0.00 | 0.96 | -12.71 | 10.34 | -9.71 | 120.61 | 0.1921 | -955.0 | -803.6 | |
| 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. | |