SDO HMI 2014-09-24 06:41:04 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.42 | 30.08 | 0.86 | 18.07 | -15.56 | 247.23 | -26.21 | 131.22 | 0.5677 | -603.2 | -533.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.98 | 0.00 | 2.33 | -17.17 | 252.15 | -21.29 | 139.16 | 0.5327 | 5.0 | 124.4 | |
| 0.00 | 1.24 | 0.00 | 0.72 | -14.73 | 250.07 | -23.37 | 133.21 | 0.5285 | 646.0 | 449.4 | |
| 0.00 | 0.80 | 0.00 | 0.47 | -14.53 | 247.56 | -25.88 | 130.04 | 0.5541 | -603.0 | -572.6 | |
| 0.00 | 0.71 | 0.00 | 0.42 | -15.36 | 247.24 | -26.20 | 130.86 | 0.5651 | -696.0 | -588.5 | |
| 0.00 | 3.54 | 0.00 | 2.13 | -15.57 | 247.00 | -26.44 | 130.89 | 0.5695 | -762.0 | -637.3 | |
| 0.00 | 0.88 | 0.00 | 0.53 | -14.27 | 247.18 | -26.26 | 129.25 | 0.5559 | -597.0 | -545.1 | |
| 0.00 | 0.80 | 0.00 | 0.48 | -15.35 | 246.93 | -26.51 | 130.51 | 0.5683 | -703.0 | -584.8 | |
| 0.00 | 0.97 | 0.00 | 0.59 | -15.70 | 246.49 | -26.95 | 130.53 | 0.5762 | -599.0 | -531.2 | |
| 0.00 | 1.68 | 0.00 | 1.01 | -14.73 | 246.39 | -27.06 | 129.08 | 0.5689 | -888.0 | -656.2 | |
| 0.00 | 4.60 | 0.00 | 2.78 | -15.28 | 246.31 | -27.13 | 129.77 | 0.5746 | -953.0 | -779.8 | |
| 0.00 | 3.72 | 0.00 | 2.27 | -15.96 | 245.86 | -27.59 | 130.23 | 0.5854 | -812.0 | -649.7 | |
| 1.42 | 4.16 | 0.86 | 2.52 | -15.37 | 245.87 | -27.57 | 129.45 | 0.5801 | -878.2 | -857.9 | |
| 0.00 | 1.50 | 0.00 | 0.91 | -15.11 | 245.91 | -27.53 | 129.13 | 0.5774 | -916.0 | -846.8 | |
| 0.00 | 1.50 | 0.00 | 0.91 | -15.32 | 245.63 | -27.81 | 129.14 | 0.5823 | -727.0 | -585.9 | |
| 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. | |