SDO HMI 2014-05-13 13:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.70 | 311.56 | 26.05 | 163.12 | 15.01 | 248.46 | 6.43 | 340.65 | 0.3269 | -694.1 | -391.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.34 | 297.36 | 8.05 | 155.77 | 15.27 | 248.87 | 6.85 | 339.68 | 0.3327 | -1088.8 | -444.2 | |
| 21.35 | -1.00 | 11.18 | -1.00 | 14.86 | 248.80 | 6.77 | 339.44 | 0.3258 | -1335.8 | 999999 | |
| 12.65 | -1.00 | 6.63 | -1.00 | 15.11 | 248.27 | 6.24 | 341.18 | 0.3268 | -1203.1 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 15.45 | 246.89 | 4.86 | 345.41 | 0.3257 | -752.0 | -562.7 | |
| 0.00 | 0.63 | 0.00 | 0.33 | 14.53 | 246.62 | 4.59 | 345.45 | 0.3098 | 731.0 | 602.9 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 15.74 | 246.36 | 4.33 | 347.14 | 0.3282 | 815.0 | 650.8 | |
| 0.00 | 1.35 | 0.00 | 0.70 | 14.12 | 246.26 | 4.24 | 346.20 | 0.3016 | 549.0 | 408.3 | |
| 0.00 | 1.79 | 0.00 | 0.92 | 11.69 | 245.94 | 3.91 | 345.09 | 0.2608 | 827.0 | 652.2 | |
| 0.00 | 0.99 | 0.00 | 0.51 | 15.00 | 245.90 | 3.88 | 347.97 | 0.3147 | 653.0 | 555.1 | |
| 0.36 | 1.08 | 0.19 | 0.56 | 14.88 | 245.75 | 3.72 | 348.37 | 0.3121 | 872.2 | 776.6 | |
| 0.00 | 3.68 | 0.00 | 1.91 | 15.04 | 241.29 | -0.73 | 2.31 | 0.3087 | 977.0 | 792.7 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 14.53 | 240.76 | -1.27 | 4.09 | 0.3007 | 859.0 | 559.2 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 11.15 | 236.66 | -5.36 | 20.79 | 0.2596 | 955.0 | 718.5 | |
| 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. | |