SDO HMI 2011-11-10 01:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 80.93 | 489.63 | 42.89 | 260.70 | 16.60 | 64.70 | -17.22 | 50.84 | 0.3666 | -673.8 | -415.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.47 | 0.00 | 0.77 | 20.35 | 73.38 | -8.54 | 25.58 | 0.3240 | -757.0 | -605.7 | |
| 0.00 | 1.12 | 0.00 | 0.57 | 15.40 | 72.84 | -9.08 | 36.26 | 0.2585 | -790.0 | -649.4 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 15.40 | 72.53 | -9.39 | 37.17 | 0.2616 | -798.0 | -647.2 | |
| 0.00 | 1.64 | 0.00 | 0.85 | 17.05 | 69.86 | -12.07 | 40.26 | 0.3107 | -727.0 | -481.2 | |
| 63.78 | 417.40 | 33.73 | 220.78 | 16.13 | 65.48 | -16.44 | 50.83 | 0.3523 | -1369.8 | -493.6 | |
| 0.00 | 2.50 | 0.00 | 1.31 | 14.55 | 65.51 | -16.41 | 54.56 | 0.3371 | -829.0 | -609.7 | |
| 0.00 | 1.64 | 0.00 | 0.88 | 20.15 | 64.96 | -16.97 | 43.43 | 0.4003 | -549.0 | -464.4 | |
| 0.00 | 1.12 | 0.00 | 0.60 | 19.43 | 64.93 | -16.99 | 44.79 | 0.3928 | -778.0 | -663.5 | |
| 0.00 | 3.36 | 0.00 | 1.79 | 17.62 | 64.86 | -17.06 | 48.56 | 0.3747 | -721.0 | -455.2 | |
| 9.57 | -5.00 | 5.08 | -5.00 | 16.42 | 64.87 | -17.05 | 51.12 | 0.3628 | -871.2 | 999999 | |
| 0.00 | 4.31 | 0.00 | 2.31 | 17.83 | 64.64 | -17.28 | 48.46 | 0.3795 | -747.0 | -605.7 | |
| 0.00 | 2.67 | 0.00 | 1.48 | 23.41 | 63.33 | -18.60 | 40.40 | 0.4535 | -796.0 | -672.0 | |
| 5.77 | 8.70 | 3.09 | 4.66 | 16.62 | 63.78 | -18.14 | 52.33 | 0.3786 | -794.7 | -640.5 | |
| 0.00 | 1.21 | 0.00 | 0.65 | 18.88 | 63.48 | -18.45 | 48.09 | 0.4040 | -916.0 | -652.4 | |
| 0.00 | 1.03 | 0.00 | 0.58 | 25.01 | 62.49 | -19.43 | 39.15 | 0.4795 | -684.0 | -499.8 | |
| 0.00 | 4.40 | 0.00 | 2.35 | 15.85 | 63.30 | -18.62 | 54.71 | 0.3779 | -912.0 | -823.7 | |
| 0.00 | 1.47 | 0.00 | 0.80 | 18.46 | 62.50 | -19.42 | 50.29 | 0.4118 | -681.0 | -526.8 | |
| 1.81 | 4.31 | 0.99 | 2.36 | 17.60 | 60.87 | -21.05 | 54.08 | 0.4246 | 1043.1 | 816.6 | |
| 0.00 | 1.55 | 0.00 | 0.88 | 23.32 | 59.33 | -22.60 | 45.73 | 0.4947 | -812.0 | -555.9 | |
| 0.00 | 1.98 | 0.00 | 1.13 | 23.64 | 59.10 | -22.83 | 45.51 | 0.5002 | -719.0 | -457.7 | |
| 0.00 | 1.29 | 0.00 | 0.72 | 18.21 | 59.04 | -22.88 | 54.97 | 0.4530 | 898.0 | 706.7 | |
| 0.00 | 1.12 | 0.00 | 0.63 | 19.54 | 58.06 | -23.87 | 53.54 | 0.4760 | 919.0 | 783.1 | |
| 0.00 | 1.38 | 0.00 | 0.77 | 17.53 | 57.64 | -24.28 | 57.69 | 0.4660 | 829.0 | 713.8 | |
| 0.00 | 1.21 | 0.00 | 0.68 | 19.64 | 57.18 | -24.75 | 54.25 | 0.4878 | 834.0 | 668.6 | |
| 0.00 | 1.72 | 0.00 | 0.98 | 19.46 | 57.10 | -24.82 | 54.66 | 0.4872 | 817.0 | 655.0 | |
| 0.00 | 1.03 | 0.00 | 0.59 | 20.60 | 56.84 | -25.09 | 52.93 | 0.4995 | 728.0 | 606.5 | |
| 0.00 | 1.90 | 0.00 | 1.06 | 17.33 | 57.02 | -24.91 | 58.65 | 0.4727 | 464.0 | 381.1 | |
| 0.00 | 1.03 | 0.00 | 0.59 | 19.32 | 56.53 | -25.39 | 55.45 | 0.4933 | 754.0 | 570.8 | |
| 0.00 | 2.50 | 0.00 | 1.44 | 20.57 | 55.75 | -26.17 | 54.01 | 0.5124 | 884.0 | 735.1 | |
| 0.00 | 1.81 | 0.00 | 1.04 | 18.86 | 55.56 | -26.36 | 57.14 | 0.5022 | 840.0 | 694.8 | |
| 0.00 | 1.29 | 0.00 | 0.75 | 20.52 | 54.80 | -27.12 | 54.96 | 0.5236 | 825.0 | 627.5 | |
| 0.00 | 1.90 | 0.00 | 1.12 | 22.47 | 54.26 | -27.67 | 52.26 | 0.5447 | 635.0 | 675.1 | |
| 0.00 | 1.72 | 0.00 | 1.02 | 21.89 | 53.62 | -28.30 | 53.74 | 0.5478 | 901.0 | 704.7 | |
| 0.00 | 1.72 | 0.00 | 1.02 | 22.01 | 53.38 | -28.55 | 53.76 | 0.5515 | 860.0 | 613.7 | |
| 0.00 | 0.78 | 0.00 | 0.46 | 22.23 | 53.25 | -28.67 | 53.52 | 0.5545 | 624.0 | 554.1 | |
| 0.00 | 1.12 | 0.00 | 0.66 | 20.79 | 53.53 | -28.40 | 55.59 | 0.5411 | 611.0 | 581.8 | |
| 0.00 | 3.02 | 0.00 | 1.80 | 21.10 | 52.08 | -29.85 | 56.25 | 0.5606 | 713.0 | 616.6 | |
| 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. | |