SDO HMI 2014-03-05 06:37:13 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.82 | 0.00 | 9.29 | 9.76 | 114.06 | 37.81 | 295.21 | 0.6593 | 252.0 | 59.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.86 | 0.00 | 0.73 | 4.54 | 129.25 | 53.00 | 280.97 | 0.8132 | -486.0 | -396.2 | |
| 0.00 | 0.52 | 0.00 | 0.44 | 4.72 | 129.22 | 52.97 | 281.19 | 0.8133 | -515.0 | -434.8 | |
| 0.00 | 0.86 | 0.00 | 0.74 | 6.40 | 129.00 | 52.75 | 283.27 | 0.8149 | -352.0 | -324.0 | |
| 0.00 | 2.51 | 0.00 | 1.86 | 12.67 | 120.28 | 44.03 | 294.29 | 0.7463 | -521.0 | -400.6 | |
| 0.00 | 1.21 | 0.00 | 0.82 | 12.22 | 114.70 | 38.45 | 296.77 | 0.6831 | -570.0 | -465.5 | |
| 0.00 | 0.78 | 0.00 | 0.50 | 7.34 | 112.89 | 36.65 | 290.99 | 0.6363 | 590.0 | 388.8 | |
| 0.00 | 1.12 | 0.00 | 0.71 | 9.49 | 110.75 | 34.51 | 295.46 | 0.6212 | 695.0 | 548.2 | |
| 0.00 | 0.78 | 0.00 | 0.46 | 10.41 | 104.20 | 27.95 | 302.08 | 0.5463 | 643.0 | 560.0 | |
| 0.00 | 0.69 | 0.00 | 0.41 | 10.53 | 104.08 | 27.83 | 302.38 | 0.5456 | 705.0 | 555.2 | |
| 0.00 | 1.12 | 0.00 | 0.66 | 10.89 | 103.77 | 27.52 | 303.23 | 0.5446 | 663.0 | 446.9 | |
| 0.00 | 0.95 | 0.00 | 0.56 | 10.96 | 103.44 | 27.19 | 303.67 | 0.5411 | 555.0 | 416.4 | |
| 0.00 | 1.21 | 0.00 | 0.70 | 10.38 | 102.56 | 26.32 | 303.63 | 0.5258 | 764.0 | 624.3 | |
| 0.00 | 0.95 | 0.00 | 0.55 | 9.72 | 101.87 | 25.62 | 303.27 | 0.5118 | 683.0 | 512.2 | |
| 0.00 | 0.26 | 0.00 | 0.15 | 9.85 | 101.48 | 25.23 | 303.90 | 0.5080 | 674.0 | 561.0 | |
| 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. | |