SDO HMI 2014-07-08 17:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.98 | 0.00 | 11.65 | -22.25 | 200.15 | -18.57 | 146.23 | 0.5288 | 176.0 | 204.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.82 | 0.00 | 1.01 | -20.95 | 206.19 | -12.53 | 153.98 | 0.4637 | 920.0 | 772.2 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -22.38 | 205.15 | -13.57 | 153.61 | 0.4902 | -623.0 | -445.0 | |
| 0.00 | 2.18 | 0.00 | 1.22 | -20.77 | 204.84 | -13.89 | 151.41 | 0.4709 | 697.0 | 653.0 | |
| 0.00 | 1.82 | 0.00 | 1.03 | -21.73 | 203.32 | -15.41 | 149.96 | 0.4949 | 898.0 | 671.6 | |
| 0.00 | 0.45 | 0.00 | 0.26 | -22.45 | 203.13 | -15.59 | 150.44 | 0.5055 | 603.0 | 593.8 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -21.90 | 203.16 | -15.56 | 149.90 | 0.4983 | 816.0 | 696.6 | |
| 0.00 | 1.63 | 0.00 | 1.00 | -26.97 | 200.06 | -18.67 | 150.62 | 0.5836 | -714.0 | -603.9 | |
| 0.00 | 1.45 | 0.00 | 0.85 | -22.66 | 199.33 | -19.39 | 145.15 | 0.5383 | 940.0 | 833.8 | |
| 0.00 | 2.63 | 0.00 | 1.55 | -22.86 | 199.23 | -19.49 | 145.25 | 0.5415 | 729.0 | 582.0 | |
| 0.00 | 0.73 | 0.00 | 0.43 | -23.77 | 198.24 | -20.49 | 144.98 | 0.5602 | 632.0 | 496.0 | |
| 0.00 | 0.82 | 0.00 | 0.49 | -21.39 | 195.79 | -22.93 | 139.09 | 0.5561 | -636.0 | -534.0 | |
| 0.00 | 2.18 | 0.00 | 1.30 | -20.96 | 195.22 | -23.50 | 137.88 | 0.5573 | -545.0 | -445.4 | |
| 0.00 | 1.00 | 0.00 | 0.60 | -21.04 | 193.49 | -25.24 | 136.01 | 0.5752 | -752.0 | -651.4 | |
| 0.00 | 1.09 | 0.00 | 0.67 | -22.09 | 192.30 | -26.42 | 136.08 | 0.5967 | -501.0 | -295.9 | |
| 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. | |