SDO HMI 2014-09-06 18:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.27 | 169.87 | 35.51 | 218.34 | -14.52 | 209.05 | 64.19 | 250.85 | 0.9230 | 275.6 | 97.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.50 | 140.87 | 28.70 | 188.61 | -14.37 | 210.14 | 65.28 | 251.33 | 0.9304 | 651.3 | 154.2 | |
| 0.00 | 1.25 | 0.00 | 1.71 | -16.49 | 210.13 | 65.27 | 249.12 | 0.9337 | 150.0 | 133.7 | |
| 0.62 | 1.78 | 0.72 | 2.05 | -16.28 | 205.52 | 60.66 | 248.05 | 0.9040 | 505.6 | 405.2 | |
| 0.00 | 1.43 | 0.00 | 1.58 | -14.87 | 204.83 | 59.97 | 249.33 | 0.8962 | -20.0 | -25.9 | |
| 0.00 | 0.98 | 0.00 | 1.11 | -16.58 | 204.78 | 59.92 | 247.50 | 0.8996 | -245.0 | -151.8 | |
| 0.00 | 1.43 | 0.00 | 1.57 | -16.44 | 204.15 | 59.29 | 247.44 | 0.8948 | -400.0 | -327.2 | |
| 1.43 | 3.21 | 1.43 | 3.21 | -14.97 | 201.40 | 56.54 | 248.13 | 0.8704 | -520.3 | -433.1 | |
| 1.87 | 3.57 | 1.90 | 3.61 | -15.64 | 201.62 | 56.76 | 247.48 | 0.8739 | -280.8 | -159.1 | |
| 0.00 | 0.80 | 0.00 | 0.78 | -13.90 | 200.70 | 55.84 | 249.08 | 0.8620 | -487.0 | -423.6 | |
| 0.00 | 1.61 | 0.00 | 1.60 | -15.46 | 201.14 | 56.29 | 247.51 | 0.8697 | -572.0 | -512.7 | |
| 0.00 | 0.54 | 0.00 | 0.54 | -16.07 | 201.41 | 56.55 | 246.93 | 0.8734 | -291.0 | -299.2 | |
| 0.00 | 1.43 | 0.00 | 1.42 | -15.60 | 200.98 | 56.12 | 247.30 | 0.8687 | -618.0 | -524.9 | |
| 0.62 | 2.05 | 0.62 | 2.04 | -15.92 | 200.94 | 56.08 | 246.94 | 0.8693 | -604.0 | -514.1 | |
| 0.00 | 1.52 | 0.00 | 1.44 | -14.26 | 199.89 | 55.04 | 248.40 | 0.8563 | -470.0 | -398.1 | |
| 0.00 | 1.78 | 0.00 | 1.69 | -14.56 | 199.68 | 54.82 | 248.00 | 0.8553 | -522.0 | -436.0 | |
| 2.23 | 5.62 | 2.14 | 5.38 | -15.25 | 199.77 | 54.91 | 247.27 | 0.8580 | -647.5 | -546.8 | |
| 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. | |