SDO HMI 2014-09-29 20:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.36 | 215.27 | 32.40 | 160.06 | -1.32 | 152.48 | -47.65 | 97.90 | 0.7482 | 665.1 | 349.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.82 | 189.02 | 21.28 | 139.69 | -1.30 | 152.85 | -47.28 | 97.96 | 0.7440 | 1103.7 | 371.9 | |
| 2.73 | -1.00 | 2.03 | -1.00 | -1.76 | 152.75 | -47.38 | 98.55 | 0.7461 | 741.2 | 999999 | |
| 2.11 | -1.00 | 1.57 | -1.00 | -1.81 | 152.56 | -47.56 | 98.56 | 0.7483 | 705.6 | 999999 | |
| 1.32 | -1.00 | 0.98 | -1.00 | -1.02 | 152.54 | -47.59 | 97.52 | 0.7469 | 693.8 | 999999 | |
| 0.00 | 0.97 | 0.00 | 0.73 | -2.26 | 152.23 | -47.90 | 99.07 | 0.7531 | 400.0 | 296.9 | |
| 0.88 | -1.00 | 0.66 | -1.00 | -1.64 | 152.08 | -48.05 | 98.22 | 0.7535 | 370.3 | 999999 | |
| 0.00 | 0.97 | 0.00 | 0.72 | 1.34 | 151.87 | -48.26 | 94.25 | 0.7504 | 512.0 | 375.8 | |
| 1.59 | 8.81 | 1.21 | 6.69 | -0.65 | 151.24 | -48.89 | 96.74 | 0.7610 | 594.0 | 488.4 | |
| 0.00 | 0.97 | 0.00 | 0.74 | -0.08 | 151.20 | -48.93 | 95.99 | 0.7604 | 580.0 | 421.2 | |
| 0.53 | 1.32 | 0.40 | 1.01 | -0.32 | 150.87 | -49.26 | 96.23 | 0.7644 | 308.8 | 215.7 | |
| 0.00 | 2.38 | 0.00 | 1.84 | -2.06 | 150.73 | -49.40 | 98.44 | 0.7693 | 406.0 | 459.9 | |
| 5.38 | 9.16 | 4.27 | 7.28 | -1.10 | 149.26 | -50.87 | 96.89 | 0.7835 | -660.8 | -423.4 | |
| 0.00 | 0.70 | 0.00 | 0.56 | -0.53 | 149.27 | -50.86 | 96.16 | 0.7823 | -569.0 | -524.6 | |
| 0.00 | 0.97 | 0.00 | 0.80 | -3.48 | 147.87 | -52.26 | 99.53 | 0.8026 | -478.0 | -396.9 | |
| 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. | |