SDO HMI 2014-09-26 18:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.04 | 144.31 | 45.49 | 212.56 | 12.26 | 169.59 | -71.24 | 79.40 | 0.9417 | -146.6 | -4.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.00 | 17.65 | 3.88 | 22.91 | 12.45 | 172.42 | -68.41 | 79.35 | 0.9255 | -681.3 | -381.6 | |
| 8.65 | 65.06 | 11.43 | 87.99 | 11.81 | 171.92 | -68.91 | 80.01 | 0.9289 | -733.8 | -140.9 | |
| 7.77 | -2.00 | 10.50 | -2.00 | 11.78 | 171.41 | -69.42 | 80.02 | 0.9321 | -380.3 | 999999 | |
| 0.00 | 0.62 | 0.00 | 0.81 | 9.92 | 172.25 | -68.57 | 82.07 | 0.9274 | -326.0 | -298.1 | |
| 3.00 | -2.00 | 4.15 | -2.00 | 11.94 | 170.87 | -69.95 | 79.82 | 0.9353 | -33.0 | 999999 | |
| 0.00 | 0.53 | 0.00 | 0.71 | 10.46 | 171.66 | -69.17 | 81.45 | 0.9310 | -345.0 | -341.7 | |
| 0.00 | 1.94 | 0.00 | 2.79 | 11.98 | 170.11 | -70.72 | 79.74 | 0.9399 | 434.0 | 365.3 | |
| 0.00 | 0.97 | 0.00 | 1.50 | 13.33 | 168.40 | -72.42 | 78.22 | 0.9490 | 360.0 | 380.2 | |
| 2.82 | 30.19 | 4.35 | 46.10 | 12.79 | 168.59 | -72.24 | 78.79 | 0.9482 | 660.6 | 255.9 | |
| 0.00 | 1.32 | 0.00 | 2.09 | 13.22 | 168.06 | -72.77 | 78.31 | 0.9509 | 460.0 | 443.8 | |
| 6.80 | 18.98 | 11.18 | 31.49 | 12.65 | 167.31 | -73.51 | 78.87 | 0.9549 | 308.6 | 22.2 | |
| 0.00 | 1.85 | 0.00 | 3.19 | 11.42 | 166.53 | -74.29 | 80.11 | 0.9591 | 261.0 | 265.1 | |
| 0.00 | 1.32 | 0.00 | 2.99 | 13.02 | 162.27 | -78.55 | 78.15 | 0.9767 | 135.0 | 87.4 | |
| 0.00 | 3.88 | 0.00 | 9.99 | 12.19 | 160.72 | -80.11 | 78.87 | 0.9822 | 18.0 | 91.7 | |
| 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. | |