SDO HMI 2014-03-22 17:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.97 | 289.19 | 48.07 | 275.32 | 11.88 | 262.34 | 55.84 | 288.54 | 0.8553 | -581.2 | -225.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.05 | 0.00 | 1.11 | 13.22 | 265.57 | 59.07 | 289.01 | 0.8852 | 374.0 | 307.8 | |
| 0.00 | 0.44 | 0.00 | 0.46 | 12.96 | 265.47 | 58.97 | 288.75 | 0.8838 | 387.0 | 355.0 | |
| 0.00 | 0.52 | 0.00 | 0.55 | 13.59 | 265.48 | 58.98 | 289.44 | 0.8853 | 483.0 | 453.0 | |
| 49.97 | 276.80 | 48.07 | 265.93 | 11.86 | 262.72 | 56.22 | 288.36 | 0.8591 | -859.7 | -255.9 | |
| 0.00 | 0.26 | 0.00 | 0.19 | 12.74 | 249.50 | 43.00 | 294.66 | 0.7343 | 518.0 | 481.0 | |
| 0.00 | 0.87 | 0.00 | 0.62 | 11.47 | 248.95 | 42.45 | 293.31 | 0.7226 | 582.0 | 491.7 | |
| 0.00 | 2.01 | 0.00 | 1.45 | 12.86 | 249.06 | 42.57 | 295.03 | 0.7302 | 620.0 | 512.9 | |
| 0.00 | 2.27 | 0.00 | 1.61 | 11.68 | 248.49 | 42.00 | 293.82 | 0.7186 | 507.0 | 522.3 | |
| 0.00 | 1.05 | 0.00 | 0.75 | 13.06 | 248.77 | 42.27 | 295.44 | 0.7280 | 481.0 | 456.9 | |
| 0.00 | 1.22 | 0.00 | 0.87 | 13.05 | 248.27 | 41.78 | 295.69 | 0.7225 | 650.0 | 510.4 | |
| 0.00 | 0.61 | 0.00 | 0.41 | 7.42 | 246.05 | 39.56 | 289.27 | 0.6714 | 430.0 | 394.6 | |
| 0.00 | 1.13 | 0.00 | 0.75 | 13.18 | 242.75 | 36.26 | 299.18 | 0.6618 | 676.0 | 572.4 | |
| 0.00 | 0.96 | 0.00 | 0.62 | 11.37 | 242.05 | 35.55 | 297.15 | 0.6429 | 706.0 | 566.1 | |
| 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. | |