SDO HMI 2014-07-08 19:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.95 | 139.62 | 45.09 | 213.44 | -19.38 | 149.35 | -68.27 | 111.98 | 0.9461 | 294.1 | -29.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.27 | 0.00 | 1.80 | -20.06 | 150.94 | -66.67 | 113.00 | 0.9385 | 332.0 | 302.0 | |
| 2.45 | 55.20 | 3.65 | 83.19 | -20.13 | 149.87 | -67.75 | 112.85 | 0.9444 | 381.0 | 1.0 | |
| 0.00 | 2.18 | 0.00 | 2.72 | -15.65 | 153.10 | -64.51 | 108.79 | 0.9198 | 509.0 | 473.4 | |
| 14.43 | -2.00 | 21.56 | -2.00 | -19.71 | 149.72 | -67.89 | 112.39 | 0.9447 | 467.4 | 999999 | |
| 4.36 | 44.66 | 6.33 | 66.91 | -18.57 | 150.09 | -67.52 | 111.28 | 0.9414 | 810.0 | 88.2 | |
| 1.63 | 6.81 | 2.44 | 10.16 | -19.06 | 149.60 | -68.02 | 111.69 | 0.9447 | 402.5 | 299.5 | |
| 1.36 | 26.42 | 2.17 | 43.09 | -20.08 | 148.48 | -69.14 | 112.53 | 0.9515 | -155.2 | -340.3 | |
| 0.27 | -5.00 | 0.40 | -5.00 | -18.77 | 149.59 | -68.03 | 111.38 | 0.9444 | 274.0 | 999999 | |
| 0.00 | 0.27 | 0.00 | 0.42 | -19.36 | 149.07 | -68.54 | 111.89 | 0.9477 | 157.0 | 139.3 | |
| 3.00 | -5.00 | 4.52 | -5.00 | -18.49 | 149.30 | -68.32 | 111.04 | 0.9456 | -282.5 | 999999 | |
| 2.45 | -7.00 | 4.02 | -7.00 | -20.12 | 147.78 | -69.84 | 112.44 | 0.9549 | -400.1 | 999999 | |
| 0.00 | 1.27 | 0.00 | 2.27 | -20.81 | 146.35 | -71.26 | 112.89 | 0.9621 | -310.0 | -277.6 | |
| 0.00 | 1.54 | 0.00 | 2.88 | -19.55 | 145.35 | -72.26 | 111.44 | 0.9654 | -403.0 | -330.5 | |
| 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. | |