SDO HMI 2014-07-17 04:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.79 | 0.00 | 9.53 | -18.91 | 147.94 | 41.16 | 237.34 | 0.7408 | 83.5 | 159.6 | |
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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 | 1.09 | 0.00 | 0.94 | -20.44 | 156.50 | 49.72 | 241.02 | 0.8194 | 261.0 | 289.0 | |
| 0.00 | 1.45 | 0.00 | 1.07 | -9.19 | 152.41 | 45.64 | 253.15 | 0.7397 | 611.0 | 524.6 | |
| 0.00 | 1.72 | 0.00 | 1.27 | -9.60 | 152.39 | 45.62 | 252.61 | 0.7407 | 612.0 | 430.9 | |
| 0.00 | 0.54 | 0.00 | 0.40 | -9.12 | 152.22 | 45.45 | 253.18 | 0.7373 | 564.0 | 511.3 | |
| 0.00 | 1.72 | 0.00 | 1.43 | -21.80 | 154.12 | 47.34 | 238.41 | 0.8038 | 564.0 | 492.1 | |
| 0.00 | 0.45 | 0.00 | 0.34 | -17.67 | 150.47 | 43.69 | 241.53 | 0.7510 | 478.0 | 454.2 | |
| 0.00 | 1.09 | 0.00 | 0.82 | -21.38 | 148.68 | 41.90 | 236.09 | 0.7517 | 662.0 | 624.5 | |
| 0.00 | 0.64 | 0.00 | 0.47 | -24.56 | 146.33 | 39.56 | 230.96 | 0.7480 | -533.0 | -476.3 | |
| 0.00 | 1.18 | 0.00 | 0.86 | -23.88 | 145.22 | 38.45 | 231.02 | 0.7337 | -517.0 | -504.0 | |
| 0.00 | 1.18 | 0.00 | 0.86 | -24.56 | 145.04 | 38.26 | 230.12 | 0.7363 | -414.0 | -294.7 | |
| 0.00 | 0.82 | 0.00 | 0.55 | -26.99 | 135.63 | 28.85 | 219.91 | 0.6724 | -578.0 | -444.3 | |
| 0.00 | 0.91 | 0.00 | 0.52 | -24.21 | 113.00 | 6.23 | 191.64 | 0.4924 | -708.0 | -534.4 | |
| 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. | |