SDO HMI 2011-06-02 20:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.94 | 266.84 | 21.78 | 146.45 | 17.11 | 20.27 | -18.63 | 45.16 | 0.4313 | -446.9 | -365.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 0.64 | 18.48 | 22.22 | -16.68 | 39.95 | 0.4257 | -627.0 | -512.7 | |
| 0.00 | 1.72 | 0.00 | 0.94 | 18.48 | 21.96 | -16.95 | 40.39 | 0.4285 | -896.0 | -752.2 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 18.97 | 21.30 | -17.61 | 40.67 | 0.4408 | -823.0 | -628.7 | |
| 1.36 | 218.04 | 0.74 | 118.69 | 16.88 | 21.45 | -17.46 | 43.89 | 0.4159 | -720.0 | -502.2 | |
| 19.52 | -4.00 | 10.61 | -4.00 | 16.50 | 21.28 | -17.62 | 44.82 | 0.4135 | -1297.1 | 999999 | |
| 8.76 | -4.00 | 4.79 | -4.00 | 17.07 | 21.06 | -17.84 | 44.16 | 0.4222 | -983.5 | 999999 | |
| 5.69 | -4.00 | 3.10 | -4.00 | 16.60 | 20.94 | -17.97 | 45.18 | 0.4184 | -1047.3 | 999999 | |
| 2.44 | -4.00 | 1.33 | -4.00 | 16.88 | 20.74 | -18.16 | 44.98 | 0.4237 | -924.0 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.56 | 21.93 | 20.15 | -18.76 | 38.04 | 0.4861 | -695.0 | -531.7 | |
| 1.63 | -4.00 | 0.89 | -4.00 | 16.66 | 20.63 | -18.27 | 45.54 | 0.4226 | -752.1 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.75 | 18.58 | 20.09 | -18.81 | 43.10 | 0.4492 | -792.0 | -656.5 | |
| 0.00 | 2.53 | 0.00 | 1.40 | 18.33 | 20.05 | -18.85 | 43.58 | 0.4468 | -910.0 | -757.2 | |
| 0.00 | 2.17 | 0.00 | 1.20 | 18.94 | 19.95 | -18.96 | 42.75 | 0.4546 | -712.0 | -556.2 | |
| 0.00 | 0.90 | 0.00 | 0.50 | 17.81 | 19.50 | -19.40 | 45.22 | 0.4474 | -732.0 | -567.2 | |
| 0.00 | 0.99 | 0.00 | 0.55 | 17.72 | 19.31 | -19.60 | 45.65 | 0.4486 | -764.0 | -561.7 | |
| 0.00 | 0.27 | 0.00 | 0.15 | 17.88 | 19.26 | -19.65 | 45.46 | 0.4508 | -528.0 | -453.3 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 17.30 | 18.98 | -19.92 | 46.81 | 0.4480 | -813.0 | -696.7 | |
| 0.00 | 1.54 | 0.00 | 0.85 | 17.15 | 18.97 | -19.94 | 47.11 | 0.4466 | -769.0 | -579.4 | |
| 0.00 | 1.45 | 0.00 | 0.81 | 17.66 | 18.36 | -20.54 | 47.05 | 0.4587 | -683.0 | -410.0 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 17.60 | 18.24 | -20.67 | 47.33 | 0.4595 | -410.0 | -395.0 | |
| 0.00 | 1.27 | 0.00 | 0.71 | 18.27 | 17.22 | -21.68 | 47.51 | 0.4777 | 868.0 | 655.5 | |
| 0.00 | 1.17 | 0.00 | 0.67 | 18.50 | 16.43 | -22.47 | 48.12 | 0.4888 | -740.0 | -629.9 | |
| 0.00 | 2.35 | 0.00 | 1.34 | 19.15 | 16.31 | -22.60 | 47.24 | 0.4964 | 835.0 | 693.0 | |
| 0.00 | 1.81 | 0.00 | 1.04 | 19.63 | 15.60 | -23.30 | 47.32 | 0.5089 | 849.0 | 658.9 | |
| 0.00 | 0.72 | 0.00 | 0.42 | 21.43 | 14.59 | -24.31 | 45.79 | 0.5368 | 695.0 | 521.6 | |
| 0.00 | 0.81 | 0.00 | 0.47 | 18.83 | 14.99 | -23.92 | 49.27 | 0.5084 | 720.0 | 495.6 | |
| 0.00 | 1.54 | 0.00 | 0.87 | 16.36 | 15.30 | -23.61 | 53.01 | 0.4830 | 888.0 | 723.7 | |
| 0.00 | 0.90 | 0.00 | 0.52 | 17.93 | 15.08 | -23.82 | 50.61 | 0.4992 | 781.0 | 581.6 | |
| 0.00 | 2.98 | 0.00 | 1.73 | 19.80 | 14.73 | -24.18 | 48.05 | 0.5201 | 657.0 | 618.7 | |
| 0.00 | 1.08 | 0.00 | 0.61 | 16.36 | 15.09 | -23.82 | 53.23 | 0.4856 | 852.0 | 734.2 | |
| 0.00 | 1.27 | 0.00 | 0.74 | 21.23 | 14.34 | -24.56 | 46.35 | 0.5376 | 612.0 | 503.3 | |
| 0.00 | 4.25 | 0.00 | 2.51 | 21.76 | 13.96 | -24.95 | 46.01 | 0.5466 | 780.0 | 482.9 | |
| 0.54 | 3.52 | 0.32 | 2.05 | 19.45 | 13.90 | -25.01 | 49.50 | 0.5263 | 965.7 | 690.3 | |
| 0.00 | 3.25 | 0.00 | 1.90 | 19.29 | 13.25 | -25.66 | 50.42 | 0.5323 | 704.0 | 648.1 | |
| 0.00 | 1.99 | 0.00 | 1.16 | 18.74 | 13.34 | -25.57 | 51.18 | 0.5266 | 727.0 | 591.7 | |
| 0.00 | 0.99 | 0.00 | 0.57 | 15.11 | 13.13 | -25.78 | 57.42 | 0.5002 | 662.0 | 506.8 | |
| 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. | |