SDO HMI 2014-08-29 12:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.21 | 40.08 | 14.82 | 33.05 | -17.49 | 206.26 | -47.57 | 118.27 | 0.8008 | 220.0 | 136.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.12 | 17.66 | 3.28 | 14.11 | -17.71 | 208.09 | -45.75 | 119.39 | 0.7854 | 683.0 | 435.2 | |
| 7.89 | -1.00 | 6.31 | -1.00 | -17.54 | 207.77 | -46.06 | 119.03 | 0.7876 | 635.6 | 999999 | |
| 0.90 | 2.87 | 0.70 | 2.23 | -14.95 | 208.20 | -45.64 | 116.19 | 0.7721 | 668.2 | 540.5 | |
| 0.00 | 0.81 | 0.00 | 0.63 | -15.20 | 207.95 | -45.89 | 116.37 | 0.7757 | 258.0 | 301.2 | |
| 0.00 | 2.24 | 0.00 | 1.82 | -17.29 | 206.93 | -46.91 | 118.33 | 0.7943 | 416.0 | 358.2 | |
| 0.90 | 2.15 | 0.76 | 1.81 | -18.75 | 205.79 | -48.05 | 119.45 | 0.8109 | 414.4 | 322.1 | |
| 0.54 | 2.60 | 0.44 | 2.12 | -16.77 | 206.50 | -47.34 | 117.52 | 0.7962 | 545.5 | 430.0 | |
| 0.99 | 2.33 | 0.81 | 1.91 | -16.56 | 206.24 | -47.60 | 117.16 | 0.7978 | 392.5 | 326.3 | |
| 0.00 | 0.63 | 0.00 | 0.52 | -17.83 | 205.70 | -48.14 | 118.36 | 0.8079 | -390.0 | -362.9 | |
| 2.42 | 4.66 | 2.10 | 4.04 | -18.53 | 204.32 | -49.52 | 118.51 | 0.8229 | -634.1 | -517.5 | |
| 0.00 | 0.27 | 0.00 | 0.24 | -17.80 | 202.40 | -51.44 | 116.85 | 0.8367 | -587.0 | -597.7 | |
| 0.00 | 0.72 | 0.00 | 0.65 | -17.69 | 202.13 | -51.71 | 116.62 | 0.8385 | -462.0 | -498.1 | |
| 0.00 | 1.17 | 0.00 | 1.11 | -19.34 | 200.56 | -53.28 | 117.79 | 0.8570 | -310.0 | -303.5 | |
| 0.45 | 1.97 | 0.42 | 1.86 | -17.71 | 200.39 | -53.45 | 115.94 | 0.8531 | -499.2 | -392.4 | |
| 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. | |