SDO HMI 2014-03-29 15:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 79.69 | 322.47 | 48.86 | 196.90 | 10.09 | 146.81 | 31.53 | 297.89 | 0.5843 | -345.0 | -252.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.93 | 0.00 | 1.20 | 4.91 | 150.64 | 35.36 | 287.27 | 0.6061 | -807.0 | -686.9 | |
| 0.00 | 1.31 | 0.00 | 0.81 | 4.91 | 150.24 | 34.95 | 287.48 | 0.6007 | -812.0 | -664.0 | |
| 0.00 | 1.84 | 0.00 | 1.17 | 9.48 | 150.51 | 35.22 | 294.33 | 0.6266 | -604.0 | -562.4 | |
| 0.00 | 3.77 | 0.00 | 2.36 | 9.79 | 149.51 | 34.22 | 295.42 | 0.6159 | -501.0 | -410.7 | |
| 1.40 | 2.89 | 0.88 | 1.82 | 10.62 | 149.35 | 34.07 | 296.75 | 0.6189 | -560.8 | -399.7 | |
| 0.00 | 1.93 | 0.00 | 1.21 | 10.43 | 149.29 | 34.01 | 296.51 | 0.6170 | -352.0 | -360.3 | |
| 15.59 | 38.27 | 9.75 | 23.91 | 10.13 | 149.07 | 33.79 | 296.23 | 0.6125 | -866.3 | -484.5 | |
| 0.00 | 1.49 | 0.00 | 0.92 | 9.49 | 148.74 | 33.46 | 295.49 | 0.6047 | 441.0 | 267.9 | |
| 2.01 | 4.82 | 1.25 | 2.99 | 9.73 | 148.66 | 33.37 | 295.92 | 0.6051 | -698.7 | -370.4 | |
| 0.00 | 1.40 | 0.00 | 0.87 | 10.04 | 148.66 | 33.37 | 296.38 | 0.6069 | -821.0 | -704.1 | |
| 3.50 | -7.00 | 2.18 | -7.00 | 10.44 | 148.56 | 33.28 | 297.05 | 0.6081 | -792.7 | 999999 | |
| 3.94 | 118.40 | 2.43 | 72.52 | 9.91 | 147.99 | 32.71 | 296.65 | 0.5978 | -741.6 | -521.4 | |
| 25.57 | -12.00 | 15.66 | -12.00 | 9.66 | 147.49 | 32.21 | 296.63 | 0.5900 | -1198.6 | 999999 | |
| 1.93 | 116.91 | 1.18 | 71.19 | 11.15 | 146.91 | 31.63 | 299.33 | 0.5924 | 614.3 | -45.6 | |
| 0.00 | 2.01 | 0.00 | 1.22 | 10.12 | 146.36 | 31.08 | 298.19 | 0.5788 | -185.0 | -201.7 | |
| 17.34 | -14.00 | 10.51 | -14.00 | 10.54 | 146.13 | 30.84 | 299.03 | 0.5786 | 234.6 | 999999 | |
| 1.93 | -14.00 | 1.16 | -14.00 | 10.64 | 145.75 | 30.46 | 299.49 | 0.5746 | 891.0 | 999999 | |
| 1.75 | -14.00 | 1.06 | -14.00 | 10.39 | 145.68 | 30.40 | 299.15 | 0.5721 | 522.8 | 999999 | |
| 3.24 | -14.00 | 1.95 | -14.00 | 10.31 | 145.39 | 30.11 | 299.26 | 0.5679 | 735.4 | 999999 | |
| 0.00 | 1.49 | 0.00 | 0.88 | 9.94 | 144.48 | 29.20 | 299.45 | 0.5539 | -816.0 | -665.9 | |
| 0.00 | 0.79 | 0.00 | 0.47 | 9.31 | 144.38 | 29.10 | 298.53 | 0.5484 | -706.0 | -619.0 | |
| 0.00 | 1.23 | 0.00 | 0.73 | 10.09 | 144.39 | 29.11 | 299.77 | 0.5539 | -697.0 | -640.6 | |
| 0.00 | 1.40 | 0.00 | 0.82 | 10.15 | 142.63 | 27.35 | 301.45 | 0.5322 | 135.0 | 177.7 | |
| 0.00 | 1.75 | 0.00 | 1.02 | 10.67 | 142.34 | 27.06 | 302.56 | 0.5325 | -871.0 | -620.3 | |
| 0.00 | 1.58 | 0.00 | 0.91 | 9.96 | 140.85 | 25.57 | 302.90 | 0.5083 | 658.0 | 593.2 | |
| 0.00 | 1.84 | 0.00 | 1.06 | 10.68 | 140.88 | 25.60 | 304.06 | 0.5145 | 575.0 | 416.5 | |
| 0.00 | 1.23 | 0.00 | 0.70 | 10.24 | 140.74 | 25.45 | 303.48 | 0.5091 | 639.0 | 544.0 | |
| 1.49 | 5.08 | 0.85 | 2.91 | 9.98 | 140.62 | 25.33 | 303.18 | 0.5055 | 913.5 | 699.3 | |
| 0.00 | 1.84 | 0.00 | 1.06 | 10.57 | 140.53 | 25.25 | 304.25 | 0.5093 | 690.0 | 579.0 | |
| 0.00 | 1.66 | 0.00 | 0.95 | 9.91 | 140.37 | 25.09 | 303.31 | 0.5018 | 856.0 | 853.4 | |
| 0.00 | 1.40 | 0.00 | 0.80 | 10.43 | 139.48 | 24.20 | 305.16 | 0.4950 | 753.0 | 574.6 | |
| 0.00 | 0.88 | 0.00 | 0.50 | 10.06 | 139.05 | 23.77 | 305.03 | 0.4866 | 871.0 | 714.5 | |
| 0.00 | 0.53 | 0.00 | 0.30 | 12.84 | 138.60 | 23.32 | 310.08 | 0.5064 | 532.0 | 495.8 | |
| 0.00 | 1.14 | 0.00 | 0.66 | 14.30 | 138.55 | 23.27 | 312.33 | 0.5199 | 566.0 | 530.2 | |
| 0.00 | 1.66 | 0.00 | 0.94 | 10.55 | 138.16 | 22.88 | 306.91 | 0.4799 | 792.0 | 770.3 | |
| 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. | |