SDO HMI 2014-05-17 13:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.06 | 359.45 | 43.28 | 237.74 | -13.70 | 229.23 | 40.11 | 251.31 | 0.6619 | 350.6 | 233.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.89 | 0.00 | 1.78 | -11.05 | 247.37 | 58.25 | 258.49 | 0.8537 | 415.0 | 297.9 | |
| 0.00 | 1.89 | 0.00 | 1.62 | -11.18 | 243.59 | 54.46 | 257.99 | 0.8184 | 129.0 | 247.0 | |
| 0.00 | 2.61 | 0.00 | 1.99 | -9.71 | 238.56 | 49.44 | 259.29 | 0.7644 | 595.0 | 535.0 | |
| 0.00 | 1.17 | 0.00 | 0.86 | -9.64 | 236.68 | 47.56 | 259.14 | 0.7431 | 343.0 | 355.2 | |
| 0.00 | 0.81 | 0.00 | 0.60 | -11.09 | 236.60 | 47.48 | 257.19 | 0.7440 | 533.0 | 446.0 | |
| 0.00 | 0.99 | 0.00 | 0.71 | -5.97 | 235.74 | 46.62 | 264.04 | 0.7290 | 462.0 | 407.8 | |
| 0.00 | 0.99 | 0.00 | 0.73 | -11.04 | 236.27 | 47.15 | 257.21 | 0.7402 | 594.0 | 588.1 | |
| 0.00 | 1.26 | 0.00 | 0.89 | -7.25 | 234.87 | 45.75 | 262.22 | 0.7195 | 574.0 | 502.9 | |
| 0.00 | 1.98 | 0.00 | 1.40 | -7.86 | 234.69 | 45.57 | 261.34 | 0.7178 | 620.0 | 429.0 | |
| 0.00 | 1.98 | 0.00 | 1.40 | -7.56 | 234.61 | 45.48 | 261.76 | 0.7165 | 676.0 | 478.8 | |
| 0.00 | 1.35 | 0.00 | 0.95 | -6.93 | 234.44 | 45.32 | 262.63 | 0.7140 | 687.0 | 535.6 | |
| 0.00 | 1.53 | 0.00 | 1.08 | -7.32 | 234.45 | 45.32 | 262.08 | 0.7144 | 611.0 | 511.2 | |
| 0.00 | 0.90 | 0.00 | 0.61 | -12.43 | 231.56 | 42.44 | 254.32 | 0.6868 | 271.0 | 277.7 | |
| 34.15 | 286.11 | 22.81 | 190.67 | -13.24 | 230.30 | 41.18 | 252.82 | 0.6732 | 1105.3 | 376.2 | |
| 29.74 | -14.00 | 19.79 | -14.00 | -13.84 | 229.93 | 40.81 | 251.84 | 0.6701 | 973.9 | 999999 | |
| 0.00 | 1.17 | 0.00 | 0.78 | -15.13 | 230.22 | 41.10 | 250.04 | 0.6774 | 537.0 | 467.1 | |
| 0.00 | 1.08 | 0.00 | 0.72 | -16.31 | 229.67 | 40.55 | 248.16 | 0.6745 | -537.0 | -512.2 | |
| 0.00 | 0.99 | 0.00 | 0.64 | -12.72 | 228.53 | 39.40 | 253.06 | 0.6495 | 733.0 | 588.6 | |
| 0.00 | 1.35 | 0.00 | 0.87 | -12.05 | 228.41 | 39.28 | 254.05 | 0.6462 | -438.0 | -353.1 | |
| 0.00 | 0.99 | 0.00 | 0.64 | -11.56 | 228.12 | 39.00 | 254.72 | 0.6414 | -459.0 | -362.8 | |
| 0.00 | 1.44 | 0.00 | 0.92 | -11.36 | 227.61 | 38.49 | 254.89 | 0.6343 | -608.0 | -474.1 | |
| 0.00 | 1.71 | 0.00 | 1.09 | -11.37 | 227.34 | 38.21 | 254.80 | 0.6307 | -696.0 | -587.7 | |
| 0.00 | 1.98 | 0.00 | 1.25 | -10.06 | 226.83 | 37.71 | 256.74 | 0.6210 | -554.0 | -437.7 | |
| 0.00 | 2.07 | 0.00 | 1.31 | -11.35 | 226.82 | 37.70 | 254.69 | 0.6239 | -588.0 | -458.6 | |
| 0.00 | 1.26 | 0.00 | 0.80 | -15.61 | 226.07 | 36.94 | 247.76 | 0.6276 | -573.0 | -485.1 | |
| 0.00 | 1.17 | 0.00 | 0.71 | -9.69 | 224.18 | 35.06 | 256.64 | 0.5841 | -509.0 | -448.2 | |
| 0.00 | 0.72 | 0.00 | 0.44 | -9.76 | 224.00 | 34.88 | 256.48 | 0.5818 | -670.0 | -573.9 | |
| 0.00 | 0.99 | 0.00 | 0.61 | -14.14 | 223.62 | 34.49 | 249.01 | 0.5904 | -776.0 | -668.2 | |
| 0.00 | 1.26 | 0.00 | 0.79 | -17.63 | 224.11 | 34.99 | 243.71 | 0.6118 | -575.0 | -476.7 | |
| 0.00 | 1.17 | 0.00 | 0.73 | -17.51 | 223.97 | 34.84 | 243.82 | 0.6094 | -752.0 | -643.6 | |
| 0.00 | 1.98 | 0.00 | 1.20 | -13.50 | 223.02 | 33.90 | 249.80 | 0.5800 | -677.0 | -550.5 | |
| 0.00 | 2.43 | 0.00 | 1.48 | -18.61 | 221.33 | 32.21 | 240.54 | 0.5823 | -823.0 | -625.5 | |
| 0.00 | 1.17 | 0.00 | 0.71 | -20.15 | 220.34 | 31.22 | 237.44 | 0.5794 | -649.0 | -443.5 | |
| 0.00 | 1.80 | 0.00 | 1.05 | -14.27 | 219.04 | 29.92 | 246.41 | 0.5296 | -779.0 | -589.8 | |
| 0.00 | 1.71 | 0.00 | 1.00 | -14.52 | 218.97 | 29.85 | 245.92 | 0.5298 | -721.0 | -667.8 | |
| 0.00 | 1.44 | 0.00 | 0.85 | -19.04 | 218.47 | 29.34 | 237.82 | 0.5495 | -693.0 | -585.2 | |
| 0.00 | 0.99 | 0.00 | 0.59 | -19.55 | 218.42 | 29.30 | 236.95 | 0.5522 | -507.0 | -500.0 | |
| 0.00 | 1.26 | 0.00 | 0.74 | -19.08 | 218.07 | 28.95 | 237.44 | 0.5448 | -624.0 | -535.4 | |
| 0.00 | 1.35 | 0.00 | 0.81 | -21.98 | 218.60 | 29.48 | 233.29 | 0.5714 | -374.0 | -343.8 | |
| 0.00 | 1.44 | 0.00 | 0.85 | -20.32 | 218.09 | 28.97 | 235.46 | 0.5536 | -621.0 | -562.6 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -21.32 | 216.05 | 26.93 | 232.09 | 0.5368 | -594.0 | -512.9 | |
| 0.00 | 1.53 | 0.00 | 0.90 | -21.80 | 216.11 | 26.99 | 231.39 | 0.5413 | -627.0 | -493.8 | |
| 1.17 | 8.09 | 0.68 | 4.73 | -21.55 | 215.70 | 26.57 | 231.39 | 0.5345 | -905.1 | -745.7 | |
| 0.00 | 1.26 | 0.00 | 0.73 | -21.46 | 215.31 | 26.19 | 231.17 | 0.5294 | -814.0 | -719.1 | |
| 0.00 | 1.08 | 0.00 | 0.63 | -21.24 | 215.24 | 26.11 | 231.45 | 0.5266 | -861.0 | -654.1 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -14.40 | 212.85 | 23.72 | 241.51 | 0.4452 | -723.0 | -441.2 | |
| 0.00 | 0.90 | 0.00 | 0.52 | -22.73 | 212.74 | 23.61 | 226.49 | 0.5114 | -743.0 | -568.5 | |
| 0.00 | 1.26 | 0.00 | 0.68 | -13.27 | 209.70 | 20.57 | 240.78 | 0.3935 | -867.0 | -741.9 | |
| 0.00 | 3.15 | 0.00 | 1.66 | -19.24 | 199.89 | 10.76 | 211.25 | 0.3413 | -921.0 | -726.0 | |
| 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. | |