SDO HMI 2014-07-17 05:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.45 | 0.00 | 10.92 | -19.76 | 147.95 | 41.73 | 235.83 | 0.7488 | 179.2 | 225.4 | |
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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 | 1.27 | 0.00 | 1.10 | -20.14 | 156.54 | 50.31 | 241.60 | 0.8235 | 550.0 | 456.7 | |
| 0.00 | 1.00 | 0.00 | 0.86 | -20.39 | 156.24 | 50.02 | 241.20 | 0.8218 | 458.0 | 438.4 | |
| 0.00 | 0.64 | 0.00 | 0.55 | -20.89 | 156.21 | 49.99 | 240.62 | 0.8233 | 515.0 | 447.1 | |
| 0.00 | 1.36 | 0.00 | 1.01 | -9.16 | 152.40 | 46.17 | 253.38 | 0.7456 | 580.0 | 501.0 | |
| 0.00 | 1.18 | 0.00 | 0.99 | -21.77 | 154.20 | 47.98 | 238.74 | 0.8092 | 551.0 | 466.6 | |
| 0.00 | 2.27 | 0.00 | 1.75 | -17.57 | 151.65 | 45.43 | 242.49 | 0.7680 | 568.0 | 386.6 | |
| 0.00 | 0.64 | 0.00 | 0.51 | -20.90 | 152.01 | 45.78 | 238.71 | 0.7858 | 498.0 | 455.6 | |
| 0.00 | 0.82 | 0.00 | 0.60 | -18.76 | 148.50 | 42.28 | 239.45 | 0.7419 | 335.0 | 292.2 | |
| 0.00 | 1.27 | 0.00 | 0.96 | -21.34 | 148.79 | 42.57 | 236.50 | 0.7578 | 654.0 | 521.1 | |
| 0.00 | 0.27 | 0.00 | 0.19 | -18.17 | 144.24 | 38.02 | 237.70 | 0.6946 | -604.0 | -578.0 | |
| 0.00 | 0.73 | 0.00 | 0.53 | -23.98 | 145.32 | 39.09 | 231.33 | 0.7402 | -591.0 | -491.0 | |
| 0.00 | 1.18 | 0.00 | 0.84 | -23.21 | 143.73 | 37.51 | 231.17 | 0.7206 | -581.0 | -368.4 | |
| 0.00 | 1.82 | 0.00 | 1.03 | -24.28 | 113.20 | 6.97 | 192.95 | 0.4959 | -603.0 | -518.2 | |
| 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. | |