SDO HMI 2014-09-25 09:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 84.72 | 451.09 | 44.55 | 237.63 | -11.00 | 265.10 | 6.12 | 199.42 | 0.3407 | 293.7 | 55.3 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.53 | 0.00 | 0.30 | -18.05 | 276.53 | 17.56 | 214.50 | 0.5084 | 587.0 | 577.8 | |
| 0.00 | 1.50 | 0.00 | 0.80 | -7.46 | 274.43 | 15.46 | 227.24 | 0.3616 | 901.0 | 597.2 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -10.48 | 273.14 | 14.17 | 219.13 | 0.3830 | 769.0 | 672.2 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -8.62 | 272.78 | 13.81 | 221.70 | 0.3563 | 907.0 | 755.1 | |
| 0.00 | 2.39 | 0.00 | 1.27 | -10.06 | 272.77 | 13.80 | 219.10 | 0.3741 | 822.0 | 647.9 | |
| 0.00 | 0.71 | 0.00 | 0.37 | -6.05 | 272.14 | 13.17 | 225.61 | 0.3185 | 780.0 | 669.0 | |
| 0.00 | 2.30 | 0.00 | 1.26 | -14.64 | 271.42 | 12.45 | 209.74 | 0.4223 | 783.0 | 661.5 | |
| 18.66 | 155.82 | 9.80 | 81.83 | -8.59 | 270.63 | 11.66 | 216.97 | 0.3336 | 1297.2 | 375.7 | |
| 14.94 | -8.00 | 7.84 | -8.00 | -8.67 | 270.23 | 11.25 | 215.86 | 0.3308 | 1319.4 | 999999 | |
| 0.00 | 1.33 | 0.00 | 0.75 | -20.08 | 270.13 | 11.16 | 201.89 | 0.4894 | 655.0 | 553.6 | |
| 0.00 | 1.33 | 0.00 | 0.69 | -8.50 | 269.54 | 10.57 | 214.47 | 0.3220 | 952.0 | 696.7 | |
| 0.00 | 1.06 | 0.00 | 0.55 | -8.08 | 269.22 | 10.25 | 214.38 | 0.3133 | 856.0 | 620.8 | |
| 17.07 | 23.08 | 8.93 | 12.08 | -8.98 | 269.00 | 10.03 | 212.24 | 0.3238 | 1133.3 | 683.9 | |
| 0.62 | 2.56 | 0.32 | 1.35 | -9.67 | 268.83 | 9.86 | 210.70 | 0.3320 | 953.3 | 765.3 | |
| 1.06 | 9.37 | 0.55 | 4.89 | -8.63 | 268.77 | 9.80 | 212.23 | 0.3169 | 1142.4 | 920.6 | |
| 0.00 | 0.62 | 0.00 | 0.31 | -1.68 | 268.55 | 9.58 | 228.28 | 0.2238 | 813.0 | 598.0 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -10.36 | 268.66 | 9.69 | 209.25 | 0.3405 | 712.0 | 604.5 | |
| 0.00 | 2.12 | 0.00 | 1.10 | -7.76 | 268.60 | 9.62 | 213.30 | 0.3031 | 850.0 | 718.3 | |
| 0.00 | 11.41 | 0.00 | 5.97 | -9.32 | 268.63 | 9.66 | 210.75 | 0.3254 | 891.0 | 852.4 | |
| 1.95 | -15.00 | 1.01 | -15.00 | -8.60 | 268.58 | 9.61 | 211.80 | 0.3148 | 1180.6 | 999999 | |
| 0.00 | 1.86 | 0.00 | 0.98 | -10.92 | 268.65 | 9.68 | 208.41 | 0.3485 | 779.0 | 550.3 | |
| 0.00 | 1.24 | 0.00 | 0.65 | -8.82 | 268.56 | 9.59 | 211.36 | 0.3176 | 876.0 | 692.9 | |
| 0.80 | 2.21 | 0.42 | 1.16 | -9.63 | 268.55 | 9.58 | 210.04 | 0.3291 | 703.3 | 530.6 | |
| 0.00 | 1.15 | 0.00 | 0.60 | -8.10 | 268.48 | 9.51 | 212.38 | 0.3068 | 928.0 | 823.8 | |
| 0.00 | 0.62 | 0.00 | 0.32 | -7.88 | 268.41 | 9.44 | 212.58 | 0.3031 | 780.0 | 588.6 | |
| 0.00 | 1.15 | 0.00 | 0.60 | -9.62 | 268.24 | 9.27 | 209.24 | 0.3265 | 760.0 | 509.1 | |
| 0.00 | 3.10 | 0.00 | 1.62 | -9.15 | 268.23 | 9.26 | 209.94 | 0.3197 | 449.0 | 495.9 | |
| 0.00 | 3.63 | 0.00 | 1.89 | -8.78 | 268.10 | 9.12 | 210.18 | 0.3131 | 1051.0 | 970.6 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -7.22 | 267.94 | 8.97 | 212.45 | 0.2895 | 862.0 | 687.9 | |
| 0.00 | 7.43 | 0.00 | 3.87 | -8.55 | 267.84 | 8.87 | 209.85 | 0.3078 | 490.0 | 395.0 | |
| 0.00 | 1.41 | 0.00 | 0.74 | -8.77 | 267.85 | 8.88 | 209.51 | 0.3110 | 1029.0 | 795.9 | |
| 0.00 | 1.95 | 0.00 | 1.01 | -8.31 | 266.52 | 7.55 | 206.38 | 0.2939 | -900.0 | -709.4 | |
| 0.00 | 1.06 | 0.00 | 0.55 | -8.15 | 264.44 | 5.47 | 199.94 | 0.2778 | 1003.0 | 820.6 | |
| 0.00 | 2.56 | 0.00 | 1.33 | -9.71 | 264.21 | 5.24 | 197.47 | 0.3014 | -788.0 | -675.0 | |
| 0.00 | 2.21 | 0.00 | 1.14 | -9.08 | 263.78 | 4.81 | 196.70 | 0.2891 | -747.0 | -747.2 | |
| 0.00 | 1.06 | 0.00 | 0.55 | -11.37 | 262.64 | 3.67 | 191.30 | 0.3216 | -904.0 | -733.2 | |
| 0.00 | 1.86 | 0.00 | 0.97 | -10.98 | 262.36 | 3.39 | 190.68 | 0.3145 | -749.0 | -676.6 | |
| 0.00 | 0.53 | 0.00 | 0.29 | -17.51 | 262.42 | 3.45 | 187.90 | 0.4195 | 735.0 | 685.7 | |
| 0.00 | 1.33 | 0.00 | 0.69 | -11.46 | 262.24 | 3.27 | 190.05 | 0.3219 | -616.0 | -555.0 | |
| 0.00 | 4.51 | 0.00 | 2.35 | -11.17 | 262.15 | 3.18 | 189.92 | 0.3169 | -886.0 | -782.3 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -18.13 | 261.92 | 2.95 | 186.59 | 0.4283 | 605.0 | 429.6 | |
| 0.00 | 0.71 | 0.00 | 0.37 | -12.85 | 261.42 | 2.45 | 187.02 | 0.3427 | -814.0 | -691.9 | |
| 0.00 | 1.50 | 0.00 | 0.84 | -20.47 | 261.00 | 2.03 | 184.12 | 0.4636 | -711.0 | -450.1 | |
| 0.00 | 1.15 | 0.00 | 0.61 | -14.58 | 260.91 | 1.94 | 185.10 | 0.3700 | -863.0 | -697.9 | |
| 0.00 | 1.50 | 0.00 | 0.79 | -13.49 | 260.07 | 1.10 | 183.05 | 0.3511 | -716.0 | -493.1 | |
| 0.00 | 3.10 | 0.00 | 1.65 | -14.84 | 259.89 | 0.92 | 182.38 | 0.3731 | 715.0 | 633.4 | |
| 0.00 | 3.45 | 0.00 | 1.85 | -15.55 | 259.70 | 0.73 | 181.84 | 0.3846 | 944.0 | 813.8 | |
| 11.85 | 161.47 | 6.26 | 85.50 | -13.48 | 259.08 | 0.11 | 180.30 | 0.3506 | -1412.7 | -419.3 | |
| 16.18 | -48.00 | 8.58 | -48.00 | -13.90 | 258.99 | 0.01 | 180.04 | 0.3575 | -1149.3 | 999999 | |
| 0.00 | 0.80 | 0.00 | 0.42 | -12.08 | 258.89 | -0.08 | 179.77 | 0.3274 | -682.0 | -547.3 | |
| 0.00 | 1.86 | 0.00 | 0.99 | -15.19 | 258.86 | -0.11 | 179.71 | 0.3785 | -845.0 | -676.6 | |
| 0.53 | 6.01 | 0.28 | 3.14 | -11.69 | 258.68 | -0.29 | 179.11 | 0.3211 | -1044.3 | -721.8 | |
| 0.53 | 1.50 | 0.28 | 0.78 | -11.38 | 258.41 | -0.57 | 178.24 | 0.3160 | -1036.8 | -906.1 | |
| 0.00 | 1.59 | 0.00 | 0.86 | -16.04 | 258.29 | -0.68 | 178.34 | 0.3924 | -983.0 | -678.1 | |
| 0.53 | 2.83 | 0.28 | 1.48 | -11.60 | 257.82 | -1.15 | 176.46 | 0.3201 | -1010.2 | -791.2 | |
| 0.00 | 1.86 | 0.00 | 0.98 | -12.91 | 257.66 | -1.31 | 176.24 | 0.3418 | 800.0 | 588.7 | |
| 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. | |