SDO HMI 2014-07-10 10:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.63 | 0.00 | 8.28 | -20.86 | 217.66 | 21.54 | 218.48 | 0.5796 | -601.6 | -520.9 | |
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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 | 1.00 | 0.00 | 0.66 | -17.63 | 232.05 | 35.93 | 237.67 | 0.6642 | -618.0 | -517.0 | |
| 0.00 | 1.00 | 0.00 | 0.64 | -14.62 | 231.36 | 35.23 | 241.35 | 0.6384 | -592.0 | -527.6 | |
| 0.00 | 0.91 | 0.00 | 0.58 | -14.51 | 231.07 | 34.94 | 241.32 | 0.6343 | -385.0 | -423.8 | |
| 0.00 | 0.55 | 0.00 | 0.35 | -16.73 | 230.92 | 34.80 | 238.11 | 0.6459 | -582.0 | -477.5 | |
| 0.00 | 2.00 | 0.00 | 1.21 | -12.57 | 227.13 | 31.01 | 241.46 | 0.5745 | -449.0 | -470.9 | |
| 0.00 | 1.18 | 0.00 | 0.71 | -12.74 | 226.50 | 30.38 | 240.72 | 0.5676 | -558.0 | -454.5 | |
| 0.00 | 1.09 | 0.00 | 0.64 | -22.24 | 216.17 | 20.05 | 216.05 | 0.5414 | -714.0 | -630.3 | |
| 0.00 | 1.36 | 0.00 | 0.81 | -28.60 | 205.19 | 9.07 | 194.48 | 0.5556 | -645.0 | -483.3 | |
| 0.00 | 0.91 | 0.00 | 0.54 | -28.48 | 204.16 | 8.04 | 192.97 | 0.5503 | -709.0 | -564.7 | |
| 0.00 | 2.27 | 0.00 | 1.34 | -28.44 | 203.74 | 7.62 | 192.33 | 0.5484 | -558.0 | -535.9 | |
| 0.00 | 1.36 | 0.00 | 0.80 | -27.89 | 203.39 | 7.27 | 192.01 | 0.5395 | -808.0 | -638.4 | |
| 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. | |