SDO HMI 2014-07-20 13:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67.77 | 214.69 | 37.62 | 119.27 | -21.28 | 68.08 | 5.94 | 192.38 | 0.4529 | 153.0 | 94.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.70 | 145.91 | 8.73 | 81.10 | -21.28 | 69.52 | 7.38 | 195.24 | 0.4571 | 1060.6 | 332.7 | |
| 1.36 | -1.00 | 0.75 | -1.00 | -20.56 | 69.39 | 7.25 | 195.43 | 0.4458 | 946.5 | 999999 | |
| 20.69 | -1.00 | 11.46 | -1.00 | -20.86 | 69.17 | 7.03 | 194.80 | 0.4495 | 1140.2 | 999999 | |
| 1.72 | -1.00 | 0.96 | -1.00 | -21.20 | 69.09 | 6.95 | 194.43 | 0.4543 | 603.7 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -20.42 | 68.69 | 6.55 | 194.10 | 0.4409 | 550.0 | 546.3 | |
| 0.45 | 3.99 | 0.25 | 2.19 | -20.04 | 67.67 | 5.53 | 192.15 | 0.4314 | 929.6 | 735.3 | |
| 0.00 | 1.18 | 0.00 | 0.65 | -20.54 | 66.80 | 4.66 | 190.08 | 0.4365 | -869.0 | -682.3 | |
| 0.00 | 2.36 | 0.00 | 1.30 | -21.27 | 65.71 | 3.57 | 187.52 | 0.4453 | -614.0 | -598.4 | |
| 0.00 | 5.90 | 0.00 | 3.29 | -22.43 | 65.57 | 3.43 | 186.89 | 0.4630 | -735.0 | -645.1 | |
| 13.16 | 19.69 | 7.29 | 10.91 | -21.58 | 65.52 | 3.38 | 187.03 | 0.4496 | -1137.9 | -787.0 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -21.99 | 65.43 | 3.29 | 186.73 | 0.4558 | -744.0 | -703.9 | |
| 1.54 | -10.00 | 0.85 | -10.00 | -21.61 | 65.22 | 3.08 | 186.41 | 0.4496 | -952.6 | 999999 | |
| 7.80 | 33.39 | 4.35 | 18.58 | -22.29 | 65.01 | 2.87 | 185.80 | 0.4598 | -791.3 | -700.0 | |
| 5.35 | -13.00 | 2.98 | -13.00 | -22.02 | 64.87 | 2.73 | 185.59 | 0.4554 | -1055.2 | 999999 | |
| 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. | |