SDO HMI 2013-03-30 14:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.95 | 253.03 | 24.91 | 140.09 | 14.90 | 255.18 | 15.52 | 324.51 | 0.4472 | -924.4 | -351.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.31 | 0.00 | 0.75 | 17.20 | 257.02 | 17.36 | 324.44 | 0.4920 | -888.0 | -726.8 | |
| 0.00 | 1.66 | 0.00 | 0.91 | 12.08 | 255.52 | 15.85 | 319.80 | 0.4155 | -800.0 | -640.2 | |
| 23.22 | 223.45 | 12.88 | 123.86 | 14.92 | 255.68 | 16.02 | 323.67 | 0.4519 | -1186.4 | -319.6 | |
| 0.00 | 2.10 | 0.00 | 1.15 | 12.86 | 255.25 | 15.58 | 321.49 | 0.4224 | -793.0 | -654.8 | |
| 0.00 | 1.05 | 0.00 | 0.58 | 14.55 | 255.27 | 15.60 | 323.88 | 0.4436 | -889.0 | -719.8 | |
| 1.84 | -3.00 | 1.02 | -3.00 | 14.87 | 255.20 | 15.53 | 324.44 | 0.4469 | -1110.6 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 12.88 | 255.00 | 15.33 | 321.98 | 0.4202 | -853.0 | -750.8 | |
| 0.00 | 11.30 | 0.00 | 6.15 | 12.60 | 254.94 | 15.28 | 321.64 | 0.4161 | -610.0 | -762.2 | |
| 0.00 | 1.40 | 0.00 | 0.76 | 12.43 | 254.65 | 14.98 | 321.93 | 0.4112 | -750.0 | -571.4 | |
| 19.89 | -3.00 | 11.01 | -3.00 | 15.21 | 254.77 | 15.11 | 325.64 | 0.4474 | -1194.6 | 999999 | |
| 0.00 | 1.75 | 0.00 | 1.00 | 19.31 | 255.10 | 15.43 | 329.90 | 0.5027 | -729.0 | -623.8 | |
| 0.00 | 1.66 | 0.00 | 0.91 | 13.60 | 254.60 | 14.93 | 323.76 | 0.4254 | -890.0 | -664.9 | |
| 0.00 | 0.96 | 0.00 | 0.54 | 17.94 | 254.48 | 14.81 | 329.43 | 0.4802 | -745.0 | -618.5 | |
| 0.00 | 1.66 | 0.00 | 0.90 | 11.80 | 253.47 | 13.81 | 323.21 | 0.3918 | -840.0 | -641.0 | |
| 0.00 | 1.14 | 0.00 | 0.63 | 16.82 | 251.87 | 12.21 | 332.87 | 0.4457 | 808.0 | 631.6 | |
| 0.00 | 0.96 | 0.00 | 0.52 | 14.80 | 251.59 | 11.92 | 331.15 | 0.4157 | 730.0 | 592.3 | |
| 0.00 | 1.49 | 0.00 | 0.81 | 14.56 | 250.82 | 11.15 | 332.46 | 0.4066 | 847.0 | 627.0 | |
| 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. | |