SDO HMI 2014-09-26 17:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.48 | 134.62 | 39.63 | 198.34 | 12.28 | 170.08 | -71.30 | 79.38 | 0.9425 | -25.8 | -58.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.19 | 0.00 | 24.12 | 12.62 | 172.35 | -69.02 | 79.13 | 0.9294 | -680.0 | -418.6 | |
| 12.36 | 63.03 | 16.91 | 87.18 | 11.78 | 171.69 | -69.69 | 80.00 | 0.9338 | -597.8 | -178.2 | |
| 2.38 | -2.00 | 3.38 | -2.00 | 11.88 | 170.90 | -70.47 | 79.86 | 0.9385 | 21.5 | 999999 | |
| 0.00 | 0.88 | 0.00 | 1.21 | 10.49 | 171.66 | -69.71 | 81.38 | 0.9344 | -256.0 | -236.8 | |
| 0.00 | 0.71 | 0.00 | 1.03 | 11.88 | 170.34 | -71.04 | 79.83 | 0.9418 | 254.0 | 222.2 | |
| 0.00 | 0.97 | 0.00 | 1.42 | 11.74 | 170.23 | -71.15 | 79.96 | 0.9424 | 174.0 | 175.7 | |
| 0.00 | 1.32 | 0.00 | 1.97 | 12.22 | 169.83 | -71.55 | 79.44 | 0.9445 | 15.0 | 47.9 | |
| 0.00 | 0.26 | 0.00 | 0.42 | 13.26 | 168.37 | -73.01 | 78.26 | 0.9521 | 360.0 | 389.3 | |
| 4.06 | 28.69 | 6.42 | 45.16 | 12.76 | 168.64 | -72.74 | 78.79 | 0.9508 | 568.1 | 243.5 | |
| 1.41 | -9.00 | 2.30 | -9.00 | 12.94 | 168.07 | -73.31 | 78.57 | 0.9537 | 488.2 | 999999 | |
| 0.00 | 2.12 | 0.00 | 3.52 | 13.30 | 167.68 | -73.70 | 78.17 | 0.9556 | 452.0 | 432.9 | |
| 6.27 | 15.89 | 10.62 | 27.12 | 12.64 | 167.30 | -74.07 | 78.84 | 0.9577 | 315.1 | 60.4 | |
| 0.00 | 1.50 | 0.00 | 2.66 | 11.45 | 166.59 | -74.79 | 80.04 | 0.9615 | 333.0 | 285.5 | |
| 0.00 | 1.06 | 0.00 | 2.53 | 13.03 | 162.15 | -79.23 | 78.08 | 0.9791 | 11.0 | 55.0 | |
| 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. | |