SDO HMI 2014-04-06 15:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.67 | 425.45 | 38.13 | 223.30 | 12.63 | 13.53 | 3.79 | 348.72 | 0.3308 | -1058.0 | -391.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.67 | 405.04 | 38.13 | 212.62 | 12.64 | 13.66 | 3.92 | 348.33 | 0.3312 | -1501.8 | -430.0 | |
| 0.00 | 1.06 | 0.00 | 0.56 | 14.62 | 13.48 | 3.74 | 349.94 | 0.3625 | 793.0 | 659.2 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 9.93 | 12.34 | 2.60 | 350.87 | 0.2828 | 808.0 | 731.3 | |
| 0.00 | 1.32 | 0.00 | 0.69 | 13.17 | 12.19 | 2.45 | 352.86 | 0.3359 | -728.0 | -667.9 | |
| 0.00 | 1.32 | 0.00 | 0.69 | 11.65 | 11.62 | 1.88 | 354.02 | 0.3098 | -781.0 | -703.4 | |
| 0.00 | 2.55 | 0.00 | 1.33 | 12.28 | 11.41 | 1.67 | 354.87 | 0.3199 | -559.0 | -506.2 | |
| 0.00 | 0.79 | 0.00 | 0.42 | 14.10 | 11.43 | 1.69 | 355.30 | 0.3498 | -712.0 | -563.6 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 14.58 | 11.24 | 1.50 | 355.91 | 0.3574 | -558.0 | -470.0 | |
| 0.00 | 2.38 | 0.00 | 1.23 | 11.30 | 10.88 | 1.14 | 356.28 | 0.3030 | 788.0 | 657.4 | |
| 0.00 | 2.11 | 0.00 | 1.11 | 12.91 | 10.58 | 0.84 | 357.49 | 0.3295 | 961.0 | 770.8 | |
| 0.00 | 1.23 | 0.00 | 0.64 | 12.22 | 10.37 | 0.63 | 358.06 | 0.3178 | 786.0 | 642.2 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 14.45 | 9.97 | 0.23 | 359.36 | 0.3544 | 731.0 | 579.4 | |
| 0.00 | 1.85 | 0.00 | 0.98 | 14.35 | 9.32 | -0.42 | 1.15 | 0.3529 | 836.0 | 623.0 | |
| 0.00 | 2.29 | 0.00 | 1.18 | 9.21 | 9.23 | -0.51 | 1.88 | 0.2673 | 802.0 | 686.2 | |
| 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. | |