SDO HMI 2014-09-24 23:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.74 | 100.95 | 10.88 | 50.48 | 14.44 | 262.31 | -2.14 | 14.30 | 0.1378 | 25.2 | 22.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.62 | 3.71 | 0.31 | 1.85 | 13.30 | 264.57 | 0.11 | 358.99 | 0.1106 | -1097.4 | -824.6 | |
| 0.00 | 2.47 | 0.00 | 1.24 | 13.94 | 264.48 | 0.02 | 359.82 | 0.1216 | -1051.0 | -823.0 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 14.21 | 264.39 | -0.07 | 0.54 | 0.1264 | -844.0 | -600.8 | |
| 2.56 | 8.40 | 1.28 | 4.18 | 12.97 | 264.36 | -0.10 | 0.95 | 0.1048 | -1078.7 | -745.5 | |
| 0.00 | 4.07 | 0.00 | 2.03 | 13.85 | 264.26 | -0.19 | 1.58 | 0.1201 | -1080.0 | -825.7 | |
| 0.00 | 2.39 | 0.00 | 1.19 | 13.18 | 264.08 | -0.38 | 3.42 | 0.1086 | -452.0 | -402.7 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 14.94 | 264.08 | -0.38 | 2.65 | 0.1392 | -796.0 | -504.4 | |
| 0.00 | 1.15 | 0.00 | 0.57 | 14.15 | 263.83 | -0.63 | 4.87 | 0.1258 | -829.0 | -623.5 | |
| 0.80 | 3.45 | 0.40 | 1.72 | 14.33 | 263.67 | -0.78 | 5.91 | 0.1292 | -1052.8 | -752.5 | |
| 0.00 | 1.77 | 0.00 | 0.88 | 15.24 | 263.61 | -0.85 | 5.68 | 0.1450 | -802.0 | -578.7 | |
| 3.62 | 12.37 | 1.81 | 6.19 | 14.70 | 263.55 | -0.91 | 6.52 | 0.1357 | -1041.0 | -478.8 | |
| 2.74 | -11.00 | 1.37 | -11.00 | 14.97 | 263.52 | -0.94 | 6.51 | 0.1404 | -976.8 | 999999 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 14.48 | 263.24 | -1.22 | 8.96 | 0.1327 | -640.0 | -496.6 | |
| 0.00 | 1.33 | 0.00 | 0.66 | 15.27 | 263.24 | -1.22 | 8.12 | 0.1463 | -37.0 | -74.0 | |
| 0.00 | 2.39 | 0.00 | 1.19 | 14.88 | 262.55 | -1.90 | 13.16 | 0.1417 | 905.0 | 714.0 | |
| 0.00 | 3.71 | 0.00 | 1.85 | 13.97 | 262.25 | -2.21 | 17.09 | 0.1278 | 719.0 | 580.0 | |
| 3.89 | 6.63 | 1.94 | 3.31 | 14.33 | 262.22 | -2.24 | 16.50 | 0.1340 | 994.9 | 648.6 | |
| 0.00 | 1.41 | 0.00 | 0.71 | 15.48 | 262.11 | -2.35 | 14.94 | 0.1537 | -69.0 | -206.5 | |
| 1.68 | 6.81 | 0.84 | 3.39 | 12.75 | 262.07 | -2.38 | 21.95 | 0.1090 | 1106.8 | 544.7 | |
| 2.56 | 4.24 | 1.29 | 2.13 | 15.57 | 261.77 | -2.69 | 16.84 | 0.1568 | -891.9 | -604.1 | |
| 0.00 | 1.33 | 0.00 | 0.66 | 13.09 | 261.73 | -2.73 | 23.52 | 0.1166 | 774.0 | 499.1 | |
| 2.65 | 4.60 | 1.33 | 2.30 | 14.02 | 261.69 | -2.77 | 20.89 | 0.1319 | 1085.2 | 805.5 | |
| 0.00 | 2.30 | 0.00 | 1.15 | 13.87 | 261.13 | -3.32 | 25.11 | 0.1332 | -834.0 | -590.9 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 14.72 | 260.81 | -3.65 | 24.53 | 0.1488 | 888.0 | 694.7 | |
| 0.62 | 2.56 | 0.31 | 1.29 | 15.54 | 260.71 | -3.75 | 22.95 | 0.1625 | 688.1 | 543.1 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 13.75 | 260.73 | -3.72 | 28.14 | 0.1344 | -721.0 | -572.7 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 14.75 | 260.66 | -3.80 | 25.36 | 0.1504 | 752.0 | 544.0 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 13.44 | 260.46 | -4.00 | 31.03 | 0.1322 | 889.0 | 733.6 | |
| 0.00 | 1.50 | 0.00 | 0.75 | 15.29 | 260.33 | -4.12 | 25.60 | 0.1612 | 1011.0 | 883.1 | |
| 0.00 | 5.04 | 0.00 | 2.53 | 15.62 | 259.64 | -4.82 | 28.25 | 0.1717 | 1277.0 | 978.5 | |
| 0.00 | 3.71 | 0.00 | 1.87 | 15.56 | 259.39 | -5.07 | 29.65 | 0.1728 | 863.0 | 604.4 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 15.71 | 259.20 | -5.26 | 30.12 | 0.1766 | 929.0 | 841.8 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 15.52 | 259.02 | -5.44 | 31.53 | 0.1756 | 1078.0 | 799.5 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 15.40 | 258.64 | -5.81 | 33.63 | 0.1772 | 886.0 | 778.4 | |
| 0.00 | 2.21 | 0.00 | 1.12 | 17.98 | 258.18 | -6.27 | 28.49 | 0.2188 | 775.0 | 672.7 | |
| 0.00 | 1.15 | 0.00 | 0.58 | 17.77 | 258.10 | -6.36 | 29.32 | 0.2164 | 873.0 | 661.5 | |
| 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. | |