SDO HMI 2014-03-05 19:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.14 | 98.35 | 34.32 | 134.90 | -10.03 | 359.73 | -69.72 | 97.99 | 0.9342 | 385.4 | 229.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.69 | 0.00 | 0.90 | -15.90 | 0.67 | -68.78 | 104.26 | 0.9267 | 338.0 | 377.9 | |
| 0.00 | 0.86 | 0.00 | 1.09 | -14.44 | 1.52 | -67.93 | 102.65 | 0.9215 | 400.0 | 304.8 | |
| 0.00 | 2.51 | 0.00 | 3.29 | -9.54 | 0.76 | -68.69 | 97.39 | 0.9281 | 337.0 | 241.4 | |
| 9.16 | 81.92 | 12.43 | 111.07 | -10.45 | 359.99 | -69.46 | 98.42 | 0.9325 | 635.5 | 296.9 | |
| 1.12 | -4.00 | 1.53 | -4.00 | -10.13 | 359.88 | -69.57 | 98.09 | 0.9333 | 476.6 | 999999 | |
| 0.00 | 0.35 | 0.00 | 0.46 | -8.67 | 0.53 | -68.92 | 96.47 | 0.9299 | 62.0 | 7.2 | |
| 11.84 | -4.00 | 16.08 | -4.00 | -9.51 | 360.00 | -69.45 | 97.42 | 0.9329 | 531.1 | 999999 | |
| 0.00 | 1.04 | 0.00 | 1.45 | -10.36 | 359.23 | -70.22 | 98.38 | 0.9372 | -281.0 | -264.2 | |
| 1.81 | 3.28 | 2.48 | 4.48 | -8.30 | 359.99 | -69.46 | 96.12 | 0.9335 | -327.8 | -254.3 | |
| 1.21 | 3.63 | 1.80 | 5.39 | -10.76 | 357.98 | -71.46 | 98.89 | 0.9443 | 193.0 | 115.2 | |
| 0.00 | 1.21 | 0.00 | 1.89 | -10.25 | 357.09 | -72.36 | 98.43 | 0.9494 | -536.0 | -463.8 | |
| 0.00 | 0.35 | 0.00 | 0.53 | -8.85 | 357.53 | -71.92 | 96.92 | 0.9476 | 302.0 | 324.5 | |
| 0.00 | 0.95 | 0.00 | 1.81 | -14.10 | 353.28 | -76.17 | 102.71 | 0.9666 | -375.0 | -347.3 | |
| 0.00 | 1.56 | 0.00 | 2.54 | -9.81 | 356.20 | -73.25 | 98.04 | 0.9543 | -252.0 | -232.1 | |
| 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. | |