SDO HMI 2014-05-10 21:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.45 | 299.00 | 29.19 | 176.85 | 14.74 | 249.16 | -28.11 | 56.53 | 0.5484 | -594.4 | -271.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.80 | 278.85 | 15.24 | 164.65 | 15.02 | 249.40 | -27.87 | 55.88 | 0.5475 | -1088.9 | -349.0 | |
| 23.65 | -1.00 | 13.95 | -1.00 | 14.58 | 249.32 | -27.95 | 56.65 | 0.5451 | -1137.8 | 999999 | |
| 0.00 | 1.52 | 0.00 | 0.90 | 12.45 | 247.61 | -29.66 | 61.53 | 0.5519 | 702.0 | 534.2 | |
| 0.00 | 2.51 | 0.00 | 1.49 | 12.20 | 247.50 | -29.77 | 62.02 | 0.5517 | 666.0 | 582.6 | |
| 0.00 | 4.39 | 0.00 | 2.63 | 13.37 | 247.20 | -30.07 | 60.36 | 0.5630 | 659.0 | 615.9 | |
| 0.00 | 0.81 | 0.00 | 0.49 | 15.61 | 246.61 | -30.66 | 57.38 | 0.5854 | 683.0 | 641.8 | |
| 0.00 | 2.33 | 0.00 | 1.42 | 15.45 | 246.49 | -30.78 | 57.71 | 0.5857 | 645.0 | 607.5 | |
| 0.00 | 1.34 | 0.00 | 0.81 | 14.15 | 246.66 | -30.62 | 59.57 | 0.5749 | 822.0 | 671.0 | |
| 0.00 | 1.16 | 0.00 | 0.70 | 13.86 | 246.59 | -30.68 | 60.06 | 0.5739 | 800.0 | 685.2 | |
| 0.00 | 1.43 | 0.00 | 0.87 | 14.06 | 246.34 | -30.93 | 59.94 | 0.5782 | 659.0 | 543.2 | |
| 0.00 | 1.16 | 0.00 | 0.71 | 14.35 | 246.23 | -31.05 | 59.59 | 0.5815 | 575.0 | 636.2 | |
| 0.00 | 1.88 | 0.00 | 1.12 | 11.76 | 246.51 | -30.76 | 63.47 | 0.5618 | 655.0 | 475.1 | |
| 0.00 | 0.72 | 0.00 | 0.47 | 17.35 | 241.47 | -35.80 | 58.63 | 0.6563 | 565.0 | 491.8 | |
| 0.00 | 0.90 | 0.00 | 0.59 | 16.75 | 241.05 | -36.22 | 59.71 | 0.6575 | 554.0 | 485.0 | |
| 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. | |