SDO HMI 2014-04-09 17:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.52 | 0.00 | 10.58 | -19.35 | 325.09 | -3.95 | 172.95 | 0.2574 | 278.7 | 194.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.91 | 0.00 | 1.46 | -14.37 | 332.12 | 3.08 | 199.67 | 0.1552 | 940.0 | 793.8 | |
| 0.00 | 1.23 | 0.00 | 0.62 | -15.53 | 332.10 | 3.06 | 197.28 | 0.1740 | 811.0 | 589.9 | |
| 0.00 | 1.32 | 0.00 | 0.66 | -14.25 | 331.81 | 2.77 | 198.06 | 0.1515 | 771.0 | 655.1 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -19.91 | 331.44 | 2.40 | 189.29 | 0.2446 | 838.0 | 698.0 | |
| 0.00 | 1.23 | 0.00 | 0.62 | -16.78 | 331.24 | 2.20 | 191.13 | 0.1913 | 883.0 | 627.0 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -17.92 | 330.25 | 1.20 | 185.53 | 0.2081 | 783.0 | 652.7 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -17.73 | 329.33 | 0.29 | 181.35 | 0.2040 | 802.0 | 655.3 | |
| 0.00 | 2.38 | 0.00 | 1.20 | -17.42 | 328.29 | -0.75 | 176.39 | 0.1991 | 1068.0 | 821.6 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -17.73 | 328.17 | -0.88 | 175.89 | 0.2045 | 768.0 | 609.4 | |
| 0.00 | 1.32 | 0.00 | 0.69 | -21.86 | 320.15 | -8.90 | 152.36 | 0.3108 | -839.0 | -630.2 | |
| 0.00 | 1.32 | 0.00 | 0.69 | -21.54 | 319.64 | -9.40 | 150.53 | 0.3102 | -794.0 | -634.7 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -17.72 | 317.25 | -11.80 | 136.45 | 0.2840 | -757.0 | -612.2 | |
| 0.00 | 2.29 | 0.00 | 1.23 | -24.92 | 315.68 | -13.36 | 147.29 | 0.3896 | -676.0 | -630.2 | |
| 0.00 | 1.76 | 0.00 | 0.99 | -29.17 | 312.04 | -17.00 | 147.27 | 0.4741 | -696.0 | -582.8 | |
| 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. | |