SDO HMI 2014-08-02 12:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.11 | 109.90 | 31.31 | 256.39 | 9.03 | 172.24 | -78.49 | 81.99 | 0.9777 | 43.5 | 64.4 | |
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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 | 1.00 | 0.00 | 1.40 | 7.83 | 180.85 | -69.88 | 83.82 | 0.9371 | -338.0 | -294.9 | |
| 0.00 | 2.08 | 0.00 | 3.34 | 10.52 | 178.00 | -72.73 | 80.81 | 0.9524 | -561.0 | -463.4 | |
| 4.16 | 9.41 | 6.65 | 14.97 | 10.22 | 178.07 | -72.66 | 81.13 | 0.9521 | -582.7 | -404.3 | |
| 0.00 | 0.63 | 0.00 | 1.04 | 11.10 | 177.53 | -73.20 | 80.18 | 0.9547 | -288.0 | -267.3 | |
| 0.00 | 0.27 | 0.00 | 0.48 | 9.72 | 176.38 | -74.35 | 81.57 | 0.9607 | -211.0 | -163.3 | |
| 0.00 | 1.09 | 0.00 | 2.00 | 10.38 | 175.59 | -75.14 | 80.83 | 0.9642 | 146.0 | 156.0 | |
| 0.00 | 1.54 | 0.00 | 2.90 | 10.25 | 175.18 | -75.55 | 80.94 | 0.9661 | 398.0 | 398.6 | |
| 0.00 | 0.91 | 0.00 | 1.91 | 11.05 | 173.48 | -77.24 | 80.02 | 0.9730 | 279.0 | 244.3 | |
| 0.00 | 1.63 | 0.00 | 3.58 | 11.21 | 172.90 | -77.83 | 79.82 | 0.9752 | 103.0 | 161.1 | |
| 0.00 | 1.27 | 0.00 | 3.01 | 11.39 | 171.93 | -78.80 | 79.57 | 0.9787 | 426.0 | 324.4 | |
| 0.00 | 0.27 | 0.00 | 0.61 | 9.19 | 172.64 | -78.08 | 81.86 | 0.9767 | 459.0 | 452.3 | |
| 2.26 | 48.25 | 5.34 | 114.77 | 8.62 | 172.15 | -78.58 | 82.41 | 0.9786 | 402.9 | 192.9 | |
| 5.16 | 41.55 | 12.84 | 106.38 | 9.20 | 171.51 | -79.22 | 81.77 | 0.9807 | 260.9 | -37.0 | |
| 2.53 | -12.00 | 6.48 | -12.00 | 8.31 | 171.23 | -79.50 | 82.66 | 0.9818 | -37.3 | 999999 | |
| 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. | |