| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.55 | 293.53 | 50.40 | 275.66 | -14.60 | 207.83 | 54.18 | 247.58 | 0.8487 | 118.1 | 65.8 | |
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back to the solar disc SDO HMI 2014-09-06 02:00:36 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.90 | 190.49 | 30.91 | 190.97 | -14.23 | 210.46 | 56.81 | 249.03 | 0.8707 | 706.6 | 229.7 | |
| 0.00 | 0.71 | 0.00 | 0.74 | -16.36 | 211.02 | 57.37 | 246.90 | 0.8804 | -312.0 | -252.5 | |
| 0.00 | 1.43 | 0.00 | 1.46 | -16.13 | 210.45 | 56.80 | 246.95 | 0.8755 | 132.0 | 95.8 | |
| 0.71 | 1.88 | 0.73 | 1.91 | -16.25 | 210.33 | 56.67 | 246.78 | 0.8749 | 272.2 | 156.2 | |
| 0.00 | 0.36 | 0.00 | 0.36 | -16.13 | 209.87 | 56.22 | 246.75 | 0.8710 | 500.0 | 386.2 | |
| 0.00 | 1.16 | 0.00 | 1.12 | -14.32 | 208.98 | 55.33 | 248.43 | 0.8589 | 472.0 | 443.6 | |
| 0.00 | 1.07 | 0.00 | 1.00 | -14.19 | 208.06 | 54.41 | 248.25 | 0.8508 | 570.0 | 508.1 | |
| 0.00 | 1.25 | 0.00 | 1.15 | -14.68 | 207.22 | 53.56 | 247.40 | 0.8451 | 598.0 | 523.4 | |
| 0.00 | 0.71 | 0.00 | 0.65 | -16.42 | 206.23 | 52.58 | 245.07 | 0.8422 | -313.0 | -221.0 | |
| 3.30 | 4.82 | 2.90 | 4.23 | -14.82 | 205.14 | 51.49 | 246.45 | 0.8274 | -446.7 | -273.6 | |
| 0.00 | 1.16 | 0.00 | 1.00 | -14.63 | 204.58 | 50.93 | 246.44 | 0.8217 | 548.0 | 473.6 | |
| 0.00 | 0.80 | 0.00 | 0.69 | -16.31 | 203.91 | 50.25 | 244.24 | 0.8215 | -408.0 | -365.8 | |
| 0.00 | 0.98 | 0.00 | 0.82 | -14.08 | 202.99 | 49.34 | 246.42 | 0.8050 | 483.0 | 442.8 | |
| 0.00 | 1.43 | 0.00 | 1.19 | -14.34 | 202.97 | 49.32 | 246.11 | 0.8058 | 572.0 | 443.5 | |
| 0.00 | 1.43 | 0.00 | 1.26 | -17.99 | 204.04 | 50.38 | 242.40 | 0.8289 | -365.0 | -288.9 | |
| 0.00 | 0.80 | 0.00 | 0.67 | -14.54 | 202.79 | 49.14 | 245.79 | 0.8049 | 380.0 | 359.6 | |
| 0.00 | 1.07 | 0.00 | 0.89 | -14.55 | 202.56 | 48.90 | 245.68 | 0.8027 | 3.0 | 93.2 | |
| 0.00 | 0.45 | 0.00 | 0.37 | -15.27 | 202.01 | 48.36 | 244.60 | 0.8003 | -191.0 | -169.4 | |
| 0.00 | 2.68 | 0.00 | 2.20 | -15.54 | 201.76 | 48.11 | 244.18 | 0.7990 | -394.0 | -286.4 | |
| 1.16 | 2.86 | 0.94 | 2.31 | -14.74 | 201.48 | 47.82 | 244.99 | 0.7931 | -594.5 | -496.6 | |
| 0.00 | 0.80 | 0.00 | 0.68 | -17.87 | 202.51 | 48.86 | 241.85 | 0.8151 | -438.0 | -369.6 | |
| 0.00 | 2.23 | 0.00 | 1.85 | -16.37 | 201.94 | 48.28 | 243.30 | 0.8039 | -265.0 | -282.0 | |
| 4.73 | 7.86 | 3.90 | 6.48 | -15.96 | 201.76 | 48.10 | 243.69 | 0.8006 | -477.4 | -148.5 | |
| 1.25 | 4.73 | 1.01 | 3.83 | -15.14 | 201.27 | 47.61 | 244.43 | 0.7927 | -466.8 | -392.3 | |
| 0.00 | 1.88 | 0.00 | 1.54 | -16.40 | 201.57 | 47.91 | 243.09 | 0.8006 | -530.0 | -463.6 | |
| 1.52 | 4.38 | 1.23 | 3.55 | -15.75 | 201.22 | 47.57 | 243.69 | 0.7947 | -682.5 | -544.6 | |
| 0.00 | 1.52 | 0.00 | 1.24 | -16.38 | 201.37 | 47.72 | 243.03 | 0.7987 | -601.0 | -503.9 | |
| 4.82 | 7.06 | 3.92 | 5.73 | -16.06 | 201.08 | 47.43 | 243.26 | 0.7947 | -795.9 | -641.4 | |
| 0.89 | 1.96 | 0.71 | 1.55 | -14.06 | 200.50 | 46.85 | 245.35 | 0.7809 | -475.2 | -395.6 | |
| 0.00 | 1.70 | 0.00 | 1.33 | -14.19 | 200.12 | 46.47 | 245.02 | 0.7777 | -676.0 | -586.5 | |
| 0.89 | 39.20 | 0.71 | 30.78 | -15.36 | 200.27 | 46.62 | 243.69 | 0.7840 | -539.5 | -568.0 | |
| 4.38 | -31.00 | 3.44 | -31.00 | -15.00 | 199.89 | 46.24 | 243.94 | 0.7788 | -853.1 | 999999 | |
| 0.00 | 0.71 | 0.00 | 0.59 | -18.93 | 200.51 | 46.86 | 239.69 | 0.8018 | -497.0 | -437.8 | |
| 0.00 | 0.89 | 0.00 | 0.70 | -18.10 | 198.03 | 44.38 | 239.35 | 0.7750 | -445.0 | -333.8 | |
| 0.00 | 1.07 | 0.00 | 0.82 | -18.52 | 196.58 | 42.92 | 238.04 | 0.7634 | -278.0 | -293.0 | |
| 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. | |