SDO HMI 2014-04-22 09:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.55 | 0.00 | 8.01 | -17.32 | 166.50 | 4.72 | 200.27 | 0.2565 | -599.2 | -528.4 | |
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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 | 0.36 | 0.00 | 0.21 | -31.28 | 181.27 | 19.49 | 212.54 | 0.5323 | 486.0 | 562.5 | |
| 0.00 | 1.51 | 0.00 | 0.78 | -5.47 | 177.19 | 15.41 | 267.55 | 0.2660 | 797.0 | 507.5 | |
| 0.00 | 1.87 | 0.00 | 0.94 | -12.28 | 171.35 | 9.57 | 231.77 | 0.2076 | -1034.0 | -809.8 | |
| 0.00 | 1.07 | 0.00 | 0.57 | -25.03 | 168.29 | 6.51 | 196.67 | 0.3596 | -562.0 | -501.2 | |
| 0.00 | 1.15 | 0.00 | 0.60 | -20.22 | 167.97 | 6.19 | 201.05 | 0.2831 | -865.0 | -676.4 | |
| 0.00 | 2.22 | 0.00 | 1.15 | -20.50 | 167.82 | 6.04 | 200.21 | 0.2866 | -790.0 | -637.4 | |
| 0.00 | 0.53 | 0.00 | 0.28 | -24.30 | 166.56 | 4.78 | 192.92 | 0.3409 | -770.0 | -617.7 | |
| 0.00 | 1.33 | 0.00 | 0.66 | -9.40 | 162.88 | 1.10 | 193.82 | 0.0794 | -913.0 | -668.3 | |
| 0.00 | 2.04 | 0.00 | 1.04 | -18.99 | 161.86 | 0.08 | 180.31 | 0.2429 | -790.0 | -688.5 | |
| 0.00 | 1.07 | 0.00 | 0.55 | -21.68 | 161.50 | -0.28 | 179.10 | 0.2884 | -812.0 | -589.0 | |
| 0.00 | 1.07 | 0.00 | 0.53 | -10.15 | 159.57 | -2.21 | 157.11 | 0.0979 | -905.0 | -670.3 | |
| 0.00 | 1.33 | 0.00 | 0.70 | -23.34 | 158.21 | -3.57 | 169.72 | 0.3214 | -1032.0 | -777.1 | |
| 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. | |