SDO HMI 2014-11-24 21:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.89 | 0.00 | 10.91 | -13.28 | 226.48 | 45.42 | 250.13 | 0.7390 | -30.9 | 162.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.51 | 0.00 | 0.39 | -12.95 | 228.65 | 47.59 | 251.31 | 0.7619 | 429.0 | 393.5 | |
| 0.00 | 0.26 | 0.00 | 0.19 | -12.61 | 228.52 | 47.46 | 251.70 | 0.7596 | 391.0 | 394.7 | |
| 0.00 | 0.77 | 0.00 | 0.58 | -12.57 | 228.28 | 47.23 | 251.68 | 0.7570 | 560.0 | 508.6 | |
| 0.00 | 1.37 | 0.00 | 1.04 | -13.16 | 228.38 | 47.32 | 250.96 | 0.7597 | 317.0 | 305.4 | |
| 0.00 | 2.31 | 0.00 | 1.75 | -12.91 | 228.23 | 47.17 | 251.23 | 0.7573 | 345.0 | 433.2 | |
| 0.00 | 3.00 | 0.00 | 2.25 | -12.87 | 227.91 | 46.85 | 251.18 | 0.7537 | 794.0 | 660.9 | |
| 0.00 | 1.20 | 0.00 | 0.89 | -13.32 | 227.49 | 46.43 | 250.47 | 0.7504 | 697.0 | 591.5 | |
| 0.00 | 0.94 | 0.00 | 0.68 | -15.57 | 225.19 | 44.13 | 246.70 | 0.7327 | -426.0 | -341.5 | |
| 0.00 | 0.77 | 0.00 | 0.53 | -10.50 | 223.83 | 42.77 | 253.05 | 0.7004 | -582.0 | -470.0 | |
| 0.00 | 0.34 | 0.00 | 0.24 | -14.78 | 224.22 | 43.16 | 247.36 | 0.7190 | -478.0 | -433.5 | |
| 0.00 | 1.03 | 0.00 | 0.72 | -13.45 | 223.58 | 42.52 | 248.90 | 0.7069 | -644.0 | -587.2 | |
| 0.00 | 0.68 | 0.00 | 0.47 | -13.13 | 223.26 | 42.20 | 249.20 | 0.7021 | -623.0 | -596.1 | |
| 0.00 | 0.60 | 0.00 | 0.41 | -12.64 | 223.08 | 42.02 | 249.81 | 0.6983 | -594.0 | -439.3 | |
| 0.00 | 1.11 | 0.00 | 0.77 | -15.99 | 221.75 | 40.69 | 244.64 | 0.6959 | -618.0 | -477.5 | |
| 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. | |