SDO HMI 2014-07-08 11:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.07 | 164.87 | 14.60 | 85.86 | 6.58 | 204.35 | -17.69 | 79.84 | 0.3083 | -869.9 | -424.4 | |
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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 | 1.36 | 0.00 | 0.71 | 10.60 | 206.03 | -16.01 | 65.53 | 0.2992 | -749.0 | -580.9 | |
| 0.00 | 1.82 | 0.00 | 0.94 | 6.43 | 205.95 | -16.09 | 79.50 | 0.2814 | -964.0 | -703.2 | |
| 0.00 | 2.54 | 0.00 | 1.32 | 10.78 | 205.76 | -16.28 | 65.31 | 0.3044 | -933.0 | -708.0 | |
| 1.64 | 6.36 | 0.85 | 3.29 | 7.10 | 205.54 | -16.50 | 77.45 | 0.2900 | -1142.4 | -888.6 | |
| 0.27 | -4.00 | 0.14 | -4.00 | 7.22 | 205.44 | -16.60 | 77.11 | 0.2920 | -987.3 | 999999 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 11.34 | 204.59 | -17.45 | 65.06 | 0.3256 | -844.0 | -700.1 | |
| 26.16 | 142.08 | 13.61 | 73.88 | 6.35 | 204.51 | -17.53 | 80.52 | 0.3049 | -1346.5 | -439.1 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 8.88 | 204.34 | -17.70 | 72.60 | 0.3162 | -718.0 | -582.2 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 8.64 | 203.12 | -18.92 | 74.24 | 0.3346 | -693.0 | -609.3 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 4.36 | 202.50 | -19.54 | 87.25 | 0.3353 | -833.0 | -645.1 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 7.05 | 201.26 | -20.78 | 79.80 | 0.3593 | 672.0 | 534.3 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 6.66 | 200.16 | -21.88 | 81.24 | 0.3761 | 739.0 | 564.0 | |
| 0.00 | 1.82 | 0.00 | 1.00 | 8.82 | 197.08 | -24.96 | 77.05 | 0.4296 | 700.0 | 536.4 | |
| 0.00 | 1.54 | 0.00 | 0.84 | 6.31 | 197.20 | -24.84 | 82.86 | 0.4226 | 905.0 | 700.8 | |
| 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. | |