SDO HMI 2014-10-09 19:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 90.85 | 331.08 | 84.25 | 308.47 | -15.26 | 122.84 | 54.10 | 247.49 | 0.8473 | 263.2 | 109.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.54 | 0.00 | 2.52 | -13.89 | 125.65 | 56.91 | 249.98 | 0.8676 | 25.0 | 116.4 | |
| 11.30 | 129.75 | 11.19 | 127.86 | -15.28 | 125.23 | 56.50 | 248.31 | 0.8677 | 497.1 | 76.3 | |
| 2.63 | -2.00 | 2.56 | -2.00 | -15.22 | 124.65 | 55.91 | 248.18 | 0.8628 | 615.0 | 999999 | |
| 18.05 | -2.00 | 17.51 | -2.00 | -15.42 | 124.45 | 55.72 | 247.89 | 0.8617 | 815.2 | 999999 | |
| 1.93 | -2.00 | 1.85 | -2.00 | -15.38 | 123.99 | 55.26 | 247.79 | 0.8578 | 682.4 | 999999 | |
| 12.18 | 104.43 | 11.46 | 97.46 | -14.49 | 123.59 | 54.86 | 248.66 | 0.8521 | 797.6 | 418.8 | |
| 0.00 | 1.49 | 0.00 | 1.41 | -15.57 | 123.63 | 54.89 | 247.45 | 0.8554 | 371.0 | 389.5 | |
| 13.67 | -6.00 | 12.84 | -6.00 | -15.07 | 123.38 | 54.65 | 247.93 | 0.8519 | 817.1 | 999999 | |
| 0.00 | 0.44 | 0.00 | 0.41 | -15.61 | 123.32 | 54.58 | 247.31 | 0.8528 | 502.0 | 461.8 | |
| 1.31 | -6.00 | 1.22 | -6.00 | -15.00 | 122.92 | 54.19 | 247.86 | 0.8478 | 778.6 | 999999 | |
| 2.45 | -6.00 | 2.25 | -6.00 | -14.95 | 122.38 | 53.64 | 247.72 | 0.8429 | 752.7 | 999999 | |
| 0.00 | 1.49 | 0.00 | 1.33 | -14.61 | 121.53 | 52.79 | 247.80 | 0.8346 | 604.0 | 512.4 | |
| 5.08 | 7.10 | 4.54 | 6.34 | -15.63 | 121.17 | 52.44 | 246.51 | 0.8345 | -422.2 | -140.7 | |
| 0.00 | 1.66 | 0.00 | 1.45 | -14.37 | 120.53 | 51.79 | 247.72 | 0.8248 | -293.0 | -278.2 | |
| 0.00 | 1.05 | 0.00 | 0.92 | -14.58 | 120.45 | 51.71 | 247.44 | 0.8248 | 265.0 | 217.8 | |
| 0.00 | 0.88 | 0.00 | 0.76 | -14.77 | 120.46 | 51.73 | 247.23 | 0.8255 | -143.0 | -93.8 | |
| 1.49 | 3.24 | 1.29 | 2.80 | -14.37 | 120.18 | 51.44 | 247.59 | 0.8216 | -582.7 | -366.5 | |
| 0.44 | 1.93 | 0.38 | 1.67 | -15.02 | 120.00 | 51.26 | 246.77 | 0.8220 | -425.4 | -232.1 | |
| 0.00 | 1.49 | 0.00 | 1.30 | -15.53 | 120.07 | 51.34 | 246.20 | 0.8244 | -211.0 | -198.2 | |
| 0.61 | 2.28 | 0.52 | 1.93 | -14.14 | 119.42 | 50.68 | 247.56 | 0.8138 | 413.7 | 320.9 | |
| 0.00 | 1.58 | 0.00 | 1.35 | -14.95 | 119.58 | 50.84 | 246.69 | 0.8179 | -402.0 | -353.2 | |
| 0.00 | 0.70 | 0.00 | 0.59 | -13.51 | 119.08 | 50.35 | 248.17 | 0.8086 | -371.0 | -298.0 | |
| 0.00 | 1.23 | 0.00 | 1.05 | -15.10 | 119.48 | 50.74 | 246.47 | 0.8175 | -383.0 | -313.9 | |
| 0.00 | 0.79 | 0.00 | 0.68 | -15.82 | 119.67 | 50.94 | 245.72 | 0.8217 | -229.0 | -178.2 | |
| 0.00 | 0.79 | 0.00 | 0.67 | -15.05 | 119.31 | 50.58 | 246.46 | 0.8159 | -511.0 | -452.2 | |
| 2.54 | 5.43 | 2.12 | 4.54 | -13.78 | 118.87 | 50.13 | 247.78 | 0.8075 | -701.8 | -454.6 | |
| 0.00 | 1.58 | 0.00 | 1.34 | -15.19 | 119.12 | 50.38 | 246.22 | 0.8145 | -322.0 | -312.6 | |
| 0.70 | 2.45 | 0.59 | 2.07 | -15.27 | 118.85 | 50.11 | 246.03 | 0.8123 | -564.8 | -473.4 | |
| 0.00 | 1.31 | 0.00 | 1.12 | -16.12 | 119.09 | 50.35 | 245.14 | 0.8174 | -222.0 | -83.3 | |
| 12.00 | 47.40 | 10.20 | 40.28 | -16.37 | 118.69 | 49.95 | 244.68 | 0.8147 | -705.1 | -219.1 | |
| 0.00 | 1.58 | 0.00 | 1.31 | -15.29 | 118.03 | 49.30 | 245.67 | 0.8048 | -611.0 | -502.4 | |
| 2.89 | -30.00 | 2.43 | -30.00 | -16.48 | 118.09 | 49.36 | 244.31 | 0.8096 | -808.3 | 999999 | |
| 1.58 | 3.85 | 1.30 | 3.17 | -15.18 | 117.53 | 48.79 | 245.58 | 0.7996 | -649.7 | -486.4 | |
| 0.00 | 0.96 | 0.00 | 0.79 | -15.46 | 117.37 | 48.64 | 245.20 | 0.7992 | -341.0 | -481.9 | |
| 0.00 | 1.66 | 0.00 | 1.35 | -15.36 | 117.02 | 48.28 | 245.16 | 0.7954 | -640.0 | -567.5 | |
| 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. | |