SDO HMI 2014-02-22 11:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.28 | 230.17 | 63.23 | 355.98 | -1.53 | 147.40 | -71.34 | 89.23 | 0.9471 | -135.2 | -38.5 | |
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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 |
| 11.87 | 138.23 | 15.74 | 185.70 | -2.24 | 150.53 | -68.21 | 89.57 | 0.9295 | -746.2 | -180.8 | |
| 15.22 | -1.00 | 20.72 | -1.00 | -2.38 | 149.94 | -68.80 | 89.80 | 0.9331 | -364.1 | 999999 | |
| 1.55 | 3.87 | 2.21 | 5.54 | -2.31 | 148.84 | -69.90 | 89.86 | 0.9399 | -207.4 | -90.5 | |
| 0.00 | 4.30 | 0.00 | 6.17 | -2.82 | 148.77 | -69.97 | 90.40 | 0.9399 | -400.0 | -241.3 | |
| 0.00 | 0.95 | 0.00 | 1.35 | -2.61 | 148.80 | -69.94 | 90.18 | 0.9399 | -306.0 | -286.8 | |
| 0.00 | 0.34 | 0.00 | 0.50 | -1.93 | 148.35 | -70.40 | 89.52 | 0.9430 | 357.0 | 335.2 | |
| 0.00 | 1.55 | 0.00 | 2.30 | -2.70 | 148.07 | -70.67 | 90.37 | 0.9441 | -100.0 | -118.1 | |
| 0.00 | 2.75 | 0.00 | 4.14 | -2.58 | 147.81 | -70.93 | 90.27 | 0.9456 | -183.0 | -15.4 | |
| 0.00 | 2.58 | 0.00 | 3.91 | -1.18 | 147.86 | -70.88 | 88.79 | 0.9463 | 490.0 | 417.4 | |
| 0.00 | 1.46 | 0.00 | 2.23 | -2.76 | 147.51 | -71.23 | 90.49 | 0.9472 | 436.0 | 350.4 | |
| 0.00 | 1.20 | 0.00 | 1.98 | -2.97 | 146.01 | -72.73 | 90.89 | 0.9551 | 383.0 | 376.7 | |
| 0.00 | 1.29 | 0.00 | 2.12 | -3.17 | 145.98 | -72.76 | 91.11 | 0.9552 | 394.0 | 319.8 | |
| 10.58 | 71.13 | 20.40 | 139.03 | -0.26 | 143.67 | -75.07 | 88.39 | 0.9678 | 434.4 | 121.6 | |
| 0.00 | 0.52 | 0.00 | 1.01 | -0.67 | 143.54 | -75.20 | 88.82 | 0.9681 | 302.0 | 283.0 | |
| 2.06 | -13.00 | 4.16 | -13.00 | -0.34 | 143.07 | -75.67 | 88.55 | 0.9703 | -94.1 | 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. | |