SDO HMI 2014-09-06 10:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 100.66 | 544.46 | 105.21 | 568.11 | 14.92 | 86.68 | -62.59 | 76.91 | 0.8825 | 40.4 | -131.2 | |
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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 | 1.34 | 0.00 | 1.34 | 18.93 | 88.32 | -60.95 | 72.30 | 0.8700 | -63.0 | -105.2 | |
| 60.02 | 527.50 | 61.09 | 550.46 | 15.43 | 87.58 | -61.69 | 76.33 | 0.8754 | 636.6 | -127.0 | |
| 0.00 | 1.34 | 0.00 | 1.32 | 12.75 | 88.60 | -60.66 | 79.42 | 0.8670 | -292.0 | -317.4 | |
| 2.32 | 4.38 | 2.29 | 4.32 | 12.38 | 88.62 | -60.65 | 79.85 | 0.8669 | -388.2 | -372.8 | |
| 0.00 | 0.80 | 0.00 | 0.87 | 17.15 | 85.63 | -63.64 | 74.39 | 0.8908 | 161.0 | 192.9 | |
| 0.00 | 1.16 | 0.00 | 1.24 | 16.48 | 86.04 | -63.23 | 75.15 | 0.8876 | 226.0 | 227.5 | |
| 0.00 | 0.80 | 0.00 | 0.87 | 16.82 | 85.69 | -63.57 | 74.77 | 0.8903 | 75.0 | 125.1 | |
| 4.20 | -2.00 | 4.44 | -2.00 | 14.48 | 86.29 | -62.98 | 77.41 | 0.8857 | -721.1 | 999999 | |
| 0.00 | 3.84 | 0.00 | 3.99 | 12.78 | 86.89 | -62.38 | 79.35 | 0.8812 | -634.0 | -492.7 | |
| 0.00 | 2.23 | 0.00 | 2.47 | 16.01 | 84.88 | -64.39 | 75.68 | 0.8964 | -465.0 | -331.9 | |
| 24.65 | -2.00 | 27.05 | -2.00 | 14.42 | 85.19 | -64.08 | 77.46 | 0.8942 | -808.5 | 999999 | |
| 1.70 | -2.00 | 1.85 | -2.00 | 13.86 | 85.41 | -63.86 | 78.10 | 0.8926 | -808.2 | 999999 | |
| 2.23 | -2.00 | 2.42 | -2.00 | 13.62 | 85.53 | -63.74 | 78.37 | 0.8917 | -794.2 | 999999 | |
| 5.54 | -2.00 | 6.07 | -2.00 | 13.47 | 85.25 | -64.02 | 78.53 | 0.8939 | -593.3 | 999999 | |
| 0.00 | 1.07 | 0.00 | 1.23 | 13.40 | 83.81 | -65.46 | 78.57 | 0.9046 | -349.0 | -311.6 | |
| 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. | |