SDO HMI 2014-04-23 07:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.77 | 380.90 | 37.01 | 214.23 | 17.78 | 166.70 | 17.03 | 323.93 | 0.4754 | -863.3 | -334.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.87 | 362.13 | 1.06 | 203.87 | 18.34 | 167.11 | 17.44 | 323.97 | 0.4857 | -790.6 | -393.3 | |
| 62.21 | -1.00 | 35.02 | -1.00 | 17.75 | 166.92 | 17.25 | 323.50 | 0.4768 | -1390.2 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.59 | 18.12 | 163.20 | 13.54 | 330.25 | 0.4501 | 635.0 | 519.2 | |
| 0.00 | 0.62 | 0.00 | 0.35 | 19.20 | 163.03 | 13.36 | 331.77 | 0.4633 | 698.0 | 557.4 | |
| 0.00 | 1.87 | 0.00 | 1.04 | 18.87 | 162.90 | 13.24 | 331.63 | 0.4579 | 718.0 | 597.4 | |
| 1.69 | 5.87 | 0.93 | 3.24 | 18.02 | 162.80 | 13.14 | 330.85 | 0.4456 | 998.4 | 812.0 | |
| 0.00 | 0.89 | 0.00 | 0.49 | 17.98 | 162.54 | 12.87 | 331.30 | 0.4431 | 899.0 | 798.0 | |
| 0.00 | 1.51 | 0.00 | 0.84 | 18.87 | 162.57 | 12.91 | 332.22 | 0.4554 | 794.0 | 657.5 | |
| 0.00 | 1.07 | 0.00 | 0.60 | 19.95 | 162.24 | 12.57 | 333.95 | 0.4679 | 698.0 | 565.8 | |
| 0.00 | 1.51 | 0.00 | 0.83 | 17.47 | 161.43 | 11.77 | 332.84 | 0.4279 | 957.0 | 772.1 | |
| 0.00 | 1.16 | 0.00 | 0.63 | 17.20 | 161.29 | 11.62 | 332.83 | 0.4232 | 854.0 | 681.6 | |
| 0.00 | 1.78 | 0.00 | 0.97 | 17.19 | 160.42 | 10.75 | 334.58 | 0.4169 | 946.0 | 823.5 | |
| 0.00 | 1.42 | 0.00 | 0.78 | 17.48 | 160.43 | 10.77 | 334.86 | 0.4212 | 811.0 | 655.9 | |
| 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. | |