SDO HMI 2014-06-04 20:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.27 | 36.98 | 9.53 | 21.45 | -19.42 | 332.31 | 25.22 | 230.57 | 0.5211 | 589.0 | 325.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.81 | 0.00 | 0.49 | -21.16 | 335.23 | 28.14 | 230.90 | 0.5689 | 500.0 | 421.9 | |
| 0.00 | 1.27 | 0.00 | 0.76 | -21.03 | 335.09 | 28.00 | 230.96 | 0.5663 | 762.0 | 594.7 | |
| 5.51 | 7.68 | 3.31 | 4.61 | -21.35 | 334.93 | 27.84 | 230.34 | 0.5672 | 891.3 | 611.5 | |
| 0.36 | 1.45 | 0.22 | 0.86 | -20.96 | 334.74 | 27.65 | 230.74 | 0.5619 | 857.0 | 694.2 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -16.88 | 333.70 | 26.61 | 236.22 | 0.5178 | 708.0 | 503.6 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -17.20 | 333.75 | 26.66 | 235.73 | 0.5207 | 849.0 | 725.3 | |
| 2.89 | 16.27 | 1.67 | 9.39 | -18.67 | 332.42 | 25.33 | 232.02 | 0.5162 | 863.9 | 742.7 | |
| 1.72 | -7.00 | 0.99 | -7.00 | -18.86 | 332.41 | 25.32 | 231.70 | 0.5178 | 768.5 | 999999 | |
| 5.79 | -7.00 | 3.34 | -7.00 | -18.80 | 332.12 | 25.03 | 231.50 | 0.5138 | 1041.2 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.72 | -18.76 | 329.76 | 22.67 | 228.93 | 0.4859 | 595.0 | 440.1 | |
| 0.00 | 1.18 | 0.00 | 0.66 | -18.03 | 329.45 | 22.36 | 229.79 | 0.4755 | 727.0 | 505.9 | |
| 0.00 | 3.35 | 0.00 | 1.86 | -18.73 | 327.34 | 20.25 | 225.92 | 0.4581 | -905.0 | -716.4 | |
| 0.00 | 0.81 | 0.00 | 0.45 | -18.47 | 327.06 | 19.97 | 225.98 | 0.4524 | -736.0 | -589.1 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -18.60 | 325.21 | 18.12 | 223.08 | 0.4334 | -674.0 | -553.7 | |
| 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. | |