SDO HMI 2014-06-08 06:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.69 | 188.81 | 20.40 | 125.53 | -3.64 | 303.50 | 41.63 | 264.28 | 0.6684 | 437.7 | 241.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.44 | 159.73 | 17.10 | 107.36 | -3.53 | 304.25 | 42.38 | 264.56 | 0.6782 | 1052.1 | 334.6 | |
| 0.00 | 1.18 | 0.00 | 0.76 | -4.38 | 301.70 | 39.83 | 262.95 | 0.6458 | 608.0 | 559.7 | |
| 1.63 | 3.08 | 1.05 | 1.98 | -2.64 | 301.34 | 39.47 | 265.62 | 0.6391 | 837.1 | 685.9 | |
| 0.00 | 0.91 | 0.00 | 0.58 | -2.36 | 301.09 | 39.22 | 266.03 | 0.6356 | 620.0 | 557.5 | |
| 0.00 | 2.35 | 0.00 | 1.48 | -2.60 | 299.77 | 37.90 | 265.52 | 0.6178 | -533.0 | -440.2 | |
| 2.99 | 9.51 | 1.87 | 5.95 | -2.36 | 299.38 | 37.51 | 265.88 | 0.6122 | -893.4 | -616.9 | |
| 0.00 | 1.09 | 0.00 | 0.68 | -2.66 | 299.08 | 37.21 | 265.35 | 0.6083 | -727.0 | -588.8 | |
| 0.00 | 2.35 | 0.00 | 1.48 | -6.82 | 299.07 | 37.20 | 258.57 | 0.6147 | -455.0 | -420.2 | |
| 0.00 | 0.81 | 0.00 | 0.51 | -4.74 | 298.87 | 37.00 | 261.91 | 0.6081 | -636.0 | -548.4 | |
| 0.00 | 2.90 | 0.00 | 1.81 | -6.73 | 298.75 | 36.88 | 258.63 | 0.6102 | -610.0 | -512.8 | |
| 0.00 | 0.91 | 0.00 | 0.56 | -7.06 | 298.63 | 36.76 | 258.05 | 0.6093 | -622.0 | -511.7 | |
| 0.00 | 1.18 | 0.00 | 0.71 | -8.59 | 295.35 | 33.48 | 254.41 | 0.5684 | 545.0 | 365.8 | |
| 0.63 | 1.54 | 0.38 | 0.92 | -7.70 | 294.68 | 32.81 | 255.71 | 0.5562 | -643.7 | -599.2 | |
| 0.00 | 1.27 | 0.00 | 0.75 | -8.00 | 294.52 | 32.65 | 255.11 | 0.5550 | -758.0 | -650.7 | |
| 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. | |