SDO HMI 2014-08-05 20:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.80 | 0.00 | 9.00 | -19.33 | 238.38 | 31.75 | 230.11 | 0.6487 | 34.5 | 56.4 | |
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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 | 0.90 | 0.00 | 0.60 | -18.32 | 240.51 | 33.88 | 233.17 | 0.6634 | 543.0 | 429.3 | |
| 0.00 | 0.81 | 0.00 | 0.55 | -19.67 | 240.75 | 34.12 | 231.67 | 0.6756 | 410.0 | 425.7 | |
| 0.00 | 1.63 | 0.00 | 1.11 | -21.69 | 241.03 | 34.40 | 229.47 | 0.6930 | 525.0 | 370.2 | |
| 0.00 | 0.90 | 0.00 | 0.61 | -19.86 | 240.56 | 33.93 | 231.29 | 0.6751 | 427.0 | 371.4 | |
| 0.00 | 1.17 | 0.00 | 0.76 | -18.37 | 239.18 | 32.55 | 232.04 | 0.6499 | 611.0 | 560.6 | |
| 0.00 | 0.81 | 0.00 | 0.53 | -19.32 | 238.81 | 32.18 | 230.54 | 0.6533 | 705.0 | 644.4 | |
| 0.00 | 1.45 | 0.00 | 0.94 | -19.13 | 238.43 | 31.80 | 230.45 | 0.6479 | 748.0 | 579.2 | |
| 0.00 | 0.81 | 0.00 | 0.52 | -18.27 | 236.98 | 30.35 | 230.26 | 0.6261 | -656.0 | -537.0 | |
| 0.00 | 0.99 | 0.00 | 0.63 | -18.74 | 236.96 | 30.33 | 229.65 | 0.6297 | -554.0 | -480.0 | |
| 0.00 | 0.99 | 0.00 | 0.64 | -19.92 | 237.13 | 30.50 | 228.31 | 0.6411 | -501.0 | -421.5 | |
| 0.00 | 1.27 | 0.00 | 0.80 | -18.13 | 236.76 | 30.13 | 230.26 | 0.6227 | -679.0 | -563.9 | |
| 0.00 | 0.90 | 0.00 | 0.58 | -19.91 | 236.30 | 29.67 | 227.57 | 0.6328 | -652.0 | -545.4 | |
| 0.00 | 1.17 | 0.00 | 0.73 | -18.70 | 234.48 | 27.85 | 227.34 | 0.6040 | -479.0 | -435.0 | |
| 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. | |