SDO HMI 2014-03-08 08:25:13 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.35 | 20.46 | 0.18 | 10.40 | -15.93 | 45.60 | 9.86 | 226.66 | 0.2276 | 289.4 | 262.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.56 | 0.00 | 0.80 | -14.65 | 48.64 | 12.90 | 238.56 | 0.2543 | 691.0 | 533.0 | |
| 0.00 | 1.13 | 0.00 | 0.58 | -15.30 | 48.20 | 12.47 | 235.53 | 0.2537 | 755.0 | 630.2 | |
| 0.00 | 0.87 | 0.00 | 0.44 | -15.48 | 48.06 | 12.32 | 234.61 | 0.2534 | 885.0 | 764.6 | |
| 0.00 | 0.87 | 0.00 | 0.44 | -15.91 | 47.83 | 12.09 | 232.72 | 0.2543 | 934.0 | 846.2 | |
| 0.35 | 3.55 | 0.18 | 1.81 | -15.76 | 46.37 | 10.63 | 229.78 | 0.2336 | 1040.2 | 828.9 | |
| 0.00 | 1.65 | 0.00 | 0.84 | -15.55 | 46.11 | 10.37 | 229.80 | 0.2281 | 1094.0 | 932.4 | |
| 0.00 | 1.21 | 0.00 | 0.62 | -15.89 | 46.00 | 10.26 | 228.37 | 0.2303 | 931.0 | 810.1 | |
| 0.00 | 1.47 | 0.00 | 0.75 | -14.46 | 45.28 | 9.54 | 231.57 | 0.2058 | 756.0 | 581.1 | |
| 0.00 | 1.13 | 0.00 | 0.57 | -17.35 | 45.25 | 9.52 | 221.69 | 0.2383 | 674.0 | 552.7 | |
| 0.00 | 1.56 | 0.00 | 0.79 | -16.58 | 44.40 | 8.66 | 221.41 | 0.2192 | -455.0 | -437.6 | |
| 0.00 | 1.56 | 0.00 | 0.79 | -16.86 | 43.97 | 8.23 | 219.15 | 0.2180 | -748.0 | -518.8 | |
| 0.00 | 0.95 | 0.00 | 0.48 | -16.48 | 43.33 | 7.59 | 218.10 | 0.2062 | -887.0 | -741.8 | |
| 0.00 | 0.87 | 0.00 | 0.44 | -15.70 | 42.93 | 7.19 | 219.13 | 0.1917 | -779.0 | -655.3 | |
| 0.00 | 2.08 | 0.00 | 1.05 | -17.03 | 42.60 | 6.86 | 213.75 | 0.2065 | -975.0 | -762.2 | |
| 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. | |