SDO HMI 2014-09-26 22:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.85 | 168.19 | 67.77 | 231.94 | 12.36 | 168.73 | -69.89 | 79.36 | 0.9331 | -76.3 | 16.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.91 | 18.36 | 7.04 | 21.87 | 12.47 | 172.38 | -66.24 | 79.41 | 0.9108 | -704.9 | -359.5 | |
| 16.07 | 64.45 | 19.67 | 79.65 | 11.81 | 171.61 | -67.00 | 80.11 | 0.9163 | -640.4 | -175.0 | |
| 1.50 | -2.00 | 1.88 | -2.00 | 12.24 | 171.07 | -67.54 | 79.61 | 0.9199 | -247.7 | 999999 | |
| 2.21 | -2.00 | 2.77 | -2.00 | 11.98 | 170.96 | -67.65 | 79.89 | 0.9207 | -175.1 | 999999 | |
| 0.00 | 1.24 | 0.00 | 1.51 | 10.38 | 171.72 | -66.89 | 81.67 | 0.9161 | -395.0 | -367.4 | |
| 0.00 | 1.50 | 0.00 | 1.92 | 11.65 | 170.47 | -68.14 | 80.22 | 0.9240 | 340.0 | 321.1 | |
| 0.00 | 1.77 | 0.00 | 2.33 | 12.22 | 169.74 | -68.87 | 79.58 | 0.9285 | 22.0 | 62.7 | |
| 0.00 | 1.24 | 0.00 | 1.72 | 13.40 | 168.48 | -70.13 | 78.25 | 0.9360 | 477.0 | 420.0 | |
| 7.77 | 41.93 | 10.87 | 57.79 | 12.86 | 168.37 | -70.24 | 78.82 | 0.9368 | 685.4 | 266.3 | |
| 0.00 | 1.15 | 0.00 | 1.66 | 13.34 | 167.68 | -70.94 | 78.28 | 0.9407 | 447.0 | 412.3 | |
| 0.00 | 4.68 | 0.00 | 6.93 | 13.07 | 167.19 | -71.43 | 78.54 | 0.9436 | 193.0 | 142.9 | |
| 7.33 | 14.30 | 10.75 | 21.05 | 12.63 | 167.39 | -71.23 | 79.02 | 0.9426 | 372.7 | 114.5 | |
| 0.35 | 1.50 | 0.54 | 2.31 | 11.35 | 166.42 | -72.19 | 80.31 | 0.9483 | 307.0 | 272.6 | |
| 1.24 | 6.27 | 2.34 | 11.84 | 12.86 | 162.66 | -75.95 | 78.49 | 0.9663 | -124.0 | -2.2 | |
| 5.47 | 9.80 | 11.91 | 21.36 | 12.17 | 160.69 | -77.93 | 79.07 | 0.9746 | 39.3 | 104.6 | |
| 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. | |