SDO HMI 2014-03-29 05:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67.82 | 355.75 | 39.16 | 205.43 | 10.04 | 146.65 | 25.89 | 302.85 | 0.5135 | -509.0 | -330.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.26 | 0.00 | 0.15 | 4.96 | 150.53 | 29.77 | 290.68 | 0.5308 | -598.0 | -491.7 | |
| 0.00 | 1.14 | 0.00 | 0.68 | 9.63 | 150.85 | 30.09 | 298.26 | 0.5633 | -674.0 | -518.0 | |
| 0.00 | 0.53 | 0.00 | 0.31 | 5.01 | 149.91 | 29.15 | 291.21 | 0.5225 | -501.0 | -596.7 | |
| 0.00 | 2.02 | 0.00 | 1.17 | 4.82 | 149.80 | 29.03 | 290.95 | 0.5199 | -836.0 | -644.5 | |
| 0.00 | 0.26 | 0.00 | 0.16 | 9.61 | 150.04 | 29.28 | 298.90 | 0.5529 | -446.0 | -528.3 | |
| 0.00 | 3.42 | 0.00 | 2.02 | 10.03 | 149.14 | 28.38 | 300.35 | 0.5445 | -609.0 | -571.6 | |
| 5.70 | 9.64 | 3.36 | 5.69 | 10.46 | 149.08 | 28.32 | 301.09 | 0.5469 | -818.8 | -578.8 | |
| 1.23 | 3.33 | 0.72 | 1.96 | 10.50 | 148.71 | 27.94 | 301.50 | 0.5425 | -805.4 | -607.2 | |
| 1.58 | 297.48 | 0.93 | 172.19 | 10.83 | 148.40 | 27.63 | 302.31 | 0.5411 | -633.2 | -348.0 | |
| 0.00 | 2.10 | 0.00 | 1.23 | 10.52 | 148.36 | 27.60 | 301.84 | 0.5384 | -747.0 | -702.8 | |
| 3.24 | -9.00 | 1.89 | -9.00 | 9.91 | 148.20 | 27.44 | 301.02 | 0.5318 | -557.5 | 999999 | |
| 0.00 | 1.31 | 0.00 | 0.77 | 10.63 | 148.14 | 27.37 | 302.24 | 0.5364 | -841.0 | -619.8 | |
| 1.14 | -9.00 | 0.66 | -9.00 | 9.89 | 147.79 | 27.03 | 301.37 | 0.5264 | -750.6 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.67 | 10.58 | 147.82 | 27.06 | 302.46 | 0.5321 | -819.0 | -569.5 | |
| 0.00 | 1.23 | 0.00 | 0.72 | 11.00 | 147.49 | 26.72 | 303.47 | 0.5313 | 298.0 | 81.6 | |
| 26.11 | -9.00 | 15.10 | -9.00 | 9.65 | 147.26 | 26.50 | 301.48 | 0.5178 | -1215.6 | 999999 | |
| 1.75 | -9.00 | 1.01 | -9.00 | 10.19 | 146.97 | 26.20 | 302.68 | 0.5184 | -926.9 | 999999 | |
| 0.61 | -9.00 | 0.35 | -9.00 | 10.73 | 146.58 | 25.81 | 303.96 | 0.5179 | 426.1 | 999999 | |
| 17.88 | -9.00 | 10.30 | -9.00 | 10.41 | 146.34 | 25.58 | 303.67 | 0.5123 | -500.6 | 999999 | |
| 0.00 | 1.31 | 0.00 | 0.76 | 11.35 | 146.40 | 25.64 | 305.15 | 0.5208 | 795.0 | 641.3 | |
| 3.68 | -9.00 | 2.11 | -9.00 | 10.57 | 145.72 | 24.95 | 304.60 | 0.5059 | 655.3 | 999999 | |
| 0.96 | 6.66 | 0.54 | 3.76 | 10.02 | 144.24 | 23.47 | 305.35 | 0.4829 | -978.4 | -759.7 | |
| 0.00 | 1.40 | 0.00 | 0.78 | 7.74 | 143.91 | 23.15 | 301.65 | 0.4595 | -752.0 | -632.8 | |
| 0.00 | 1.05 | 0.00 | 0.60 | 12.13 | 144.19 | 23.42 | 308.87 | 0.5012 | -639.0 | -436.0 | |
| 0.00 | 0.88 | 0.00 | 0.49 | 9.74 | 143.39 | 22.62 | 305.86 | 0.4698 | -694.0 | -523.0 | |
| 2.28 | 4.99 | 1.27 | 2.79 | 10.80 | 142.02 | 21.26 | 309.43 | 0.4631 | -925.3 | -691.7 | |
| 1.66 | 3.94 | 0.92 | 2.17 | 9.99 | 140.54 | 19.77 | 310.08 | 0.4373 | 875.5 | 749.0 | |
| 0.00 | 1.31 | 0.00 | 0.72 | 10.64 | 140.32 | 19.56 | 311.53 | 0.4413 | 614.0 | 404.5 | |
| 0.00 | 1.58 | 0.00 | 0.86 | 9.51 | 140.22 | 19.45 | 309.69 | 0.4286 | 843.0 | 640.5 | |
| 0.00 | 0.88 | 0.00 | 0.48 | 9.44 | 139.99 | 19.22 | 309.89 | 0.4251 | 804.0 | 673.4 | |
| 0.00 | 1.58 | 0.00 | 0.86 | 9.27 | 139.82 | 19.05 | 309.85 | 0.4214 | 841.0 | 671.7 | |
| 0.00 | 2.54 | 0.00 | 1.39 | 10.41 | 139.44 | 18.67 | 312.47 | 0.4287 | 462.0 | 553.2 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 7.25 | 138.60 | 17.83 | 307.78 | 0.3860 | -726.0 | -499.5 | |
| 0.00 | 1.84 | 0.00 | 1.01 | 11.88 | 138.38 | 17.61 | 316.62 | 0.4329 | 914.0 | 792.4 | |
| 0.00 | 0.79 | 0.00 | 0.43 | 12.04 | 138.39 | 17.62 | 316.86 | 0.4348 | 527.0 | 463.0 | |
| 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. | |