SDO HMI 2014-07-07 22:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.45 | 17.42 | 1.89 | 13.14 | 11.75 | 277.77 | 48.58 | 282.55 | 0.7542 | -104.6 | -154.5 | |
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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 | 1.03 | 11.01 | 281.54 | 52.36 | 281.14 | 0.7944 | -233.0 | -314.8 | |
| 0.00 | 1.45 | 0.00 | 1.15 | 7.03 | 280.52 | 51.34 | 276.14 | 0.7817 | -643.0 | -526.2 | |
| 2.45 | 3.90 | 1.89 | 3.01 | 11.54 | 279.04 | 49.85 | 282.06 | 0.7681 | -641.7 | -489.2 | |
| 0.00 | 0.82 | 0.00 | 0.62 | 12.53 | 278.32 | 49.14 | 283.45 | 0.7614 | -229.0 | -308.8 | |
| 0.00 | 0.54 | 0.00 | 0.42 | 12.99 | 278.40 | 49.21 | 284.05 | 0.7628 | -315.0 | -384.5 | |
| 0.00 | 0.27 | 0.00 | 0.21 | 12.69 | 278.32 | 49.13 | 283.66 | 0.7615 | -405.0 | -386.0 | |
| 0.00 | 2.63 | 0.00 | 1.98 | 12.25 | 277.63 | 48.45 | 283.18 | 0.7534 | -510.0 | -418.7 | |
| 0.00 | 1.45 | 0.00 | 1.09 | 12.39 | 277.43 | 48.25 | 283.38 | 0.7513 | -430.0 | -347.0 | |
| 0.00 | 0.91 | 0.00 | 0.66 | 13.01 | 276.01 | 46.82 | 284.44 | 0.7360 | 449.0 | 461.4 | |
| 0.00 | 1.63 | 0.00 | 1.16 | 10.44 | 274.59 | 45.40 | 281.13 | 0.7160 | 290.0 | 281.1 | |
| 0.00 | 0.91 | 0.00 | 0.66 | 14.35 | 275.30 | 46.12 | 286.39 | 0.7301 | 226.0 | 293.1 | |
| 0.00 | 0.27 | 0.00 | 0.19 | 14.04 | 273.92 | 44.73 | 286.25 | 0.7135 | 519.0 | 561.0 | |
| 0.00 | 0.64 | 0.00 | 0.45 | 14.47 | 273.94 | 44.75 | 286.85 | 0.7146 | 509.0 | 522.4 | |
| 0.00 | 0.73 | 0.00 | 0.51 | 14.17 | 273.73 | 44.54 | 286.47 | 0.7115 | 427.0 | 417.6 | |
| 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. | |