SDO HMI 2014-04-09 07:05:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.64 | 0.00 | 9.03 | -17.91 | 327.43 | -7.06 | 153.26 | 0.2428 | 455.2 | 446.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.53 | 0.00 | 0.26 | -14.40 | 333.00 | -1.49 | 170.16 | 0.1482 | 606.0 | 683.5 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -14.57 | 332.90 | -1.59 | 169.73 | 0.1514 | 676.0 | 587.3 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -16.30 | 332.24 | -2.25 | 168.07 | 0.1829 | 785.0 | 592.4 | |
| 0.00 | 1.23 | 0.00 | 0.63 | -16.29 | 327.89 | -6.60 | 148.27 | 0.2109 | 842.0 | 691.6 | |
| 0.00 | 1.68 | 0.00 | 0.85 | -17.84 | 331.65 | -2.84 | 167.00 | 0.2109 | 1019.0 | 835.9 | |
| 0.00 | 2.03 | 0.00 | 1.03 | -17.66 | 329.04 | -5.45 | 155.85 | 0.2222 | 584.0 | 674.1 | |
| 0.00 | 1.32 | 0.00 | 0.67 | -17.29 | 327.12 | -7.37 | 148.00 | 0.2321 | 781.0 | 615.3 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -17.97 | 329.94 | -4.55 | 159.96 | 0.2213 | 750.0 | 589.7 | |
| 0.00 | 2.03 | 0.00 | 1.03 | -17.77 | 328.85 | -5.64 | 155.35 | 0.2253 | 1017.0 | 801.5 | |
| 0.00 | 0.79 | 0.00 | 0.41 | -18.38 | 327.83 | -6.66 | 152.82 | 0.2421 | 682.0 | 558.0 | |
| 0.00 | 1.76 | 0.00 | 0.90 | -18.61 | 326.01 | -8.48 | 147.41 | 0.2607 | 841.0 | 673.7 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -18.92 | 319.58 | -14.91 | 132.91 | 0.3338 | -766.0 | -654.5 | |
| 0.00 | 1.15 | 0.00 | 0.61 | -21.04 | 317.50 | -16.99 | 133.98 | 0.3806 | -737.0 | -616.2 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -21.93 | 319.93 | -14.56 | 139.89 | 0.3637 | -707.0 | -575.9 | |
| 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. | |