SDO HMI 2014-07-09 06:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67.32 | 406.75 | 49.85 | 301.24 | -19.13 | 254.49 | 42.94 | 239.95 | 0.7458 | 796.1 | 307.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.91 | 0.00 | 0.81 | -20.64 | 263.04 | 51.50 | 241.98 | 0.8317 | 507.0 | 494.1 | |
| 0.00 | 0.55 | 0.00 | 0.48 | -20.87 | 263.00 | 51.45 | 241.70 | 0.8321 | 622.0 | 503.7 | |
| 0.00 | 0.73 | 0.00 | 0.55 | -17.28 | 256.59 | 45.04 | 243.26 | 0.7588 | -586.0 | -466.5 | |
| 0.00 | 1.09 | 0.00 | 0.83 | -19.27 | 255.88 | 44.33 | 240.48 | 0.7603 | -312.0 | -276.8 | |
| 0.00 | 1.18 | 0.00 | 0.94 | -23.16 | 256.63 | 45.09 | 236.27 | 0.7852 | -467.0 | -479.9 | |
| 0.00 | 1.09 | 0.00 | 0.87 | -23.80 | 256.49 | 44.94 | 235.46 | 0.7869 | -444.0 | -442.6 | |
| 65.41 | 389.93 | 48.46 | 288.62 | -19.04 | 254.50 | 42.96 | 240.08 | 0.7455 | 1142.9 | 330.5 | |
| 0.00 | 0.82 | 0.00 | 0.61 | -21.66 | 253.62 | 42.08 | 236.43 | 0.7497 | 417.0 | 344.2 | |
| 0.91 | 2.27 | 0.67 | 1.68 | -21.11 | 253.34 | 41.79 | 236.93 | 0.7442 | 598.6 | 475.3 | |
| 0.00 | 0.73 | 0.00 | 0.52 | -19.49 | 252.04 | 40.49 | 238.19 | 0.7226 | 379.0 | 354.2 | |
| 0.00 | 1.00 | 0.00 | 0.74 | -22.16 | 252.70 | 41.15 | 235.31 | 0.7435 | -643.0 | -462.0 | |
| 0.64 | 1.64 | 0.46 | 1.19 | -22.08 | 251.84 | 40.30 | 234.90 | 0.7348 | -714.7 | -668.3 | |
| 0.00 | 0.64 | 0.00 | 0.45 | -20.32 | 251.27 | 39.72 | 236.71 | 0.7192 | -496.0 | -405.7 | |
| 0.36 | 1.27 | 0.26 | 0.90 | -20.35 | 251.24 | 39.69 | 236.65 | 0.7191 | -564.0 | -504.7 | |
| 0.00 | 0.36 | 0.00 | 0.26 | -21.70 | 250.90 | 39.35 | 234.78 | 0.7235 | -266.0 | -465.5 | |
| 0.00 | 1.54 | 0.00 | 1.08 | -20.47 | 250.30 | 38.76 | 235.92 | 0.7103 | -574.0 | -489.1 | |
| 0.00 | 1.00 | 0.00 | 0.71 | -23.55 | 249.69 | 38.14 | 231.79 | 0.7229 | -547.0 | -467.7 | |
| 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. | |