SDO HMI 2011-10-19 03:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 110.60 | 538.60 | 127.18 | 632.40 | 11.33 | 305.48 | -65.46 | 80.08 | 0.9047 | -206.5 | 20.2 | |
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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 | 1.57 | 0.00 | 1.51 | 10.27 | 311.58 | -59.36 | 81.37 | 0.8584 | -453.0 | -420.7 | |
| 1.05 | 69.16 | 1.02 | 67.79 | 11.70 | 310.98 | -59.96 | 79.70 | 0.8636 | -855.0 | -349.7 | |
| 12.65 | -2.00 | 12.46 | -2.00 | 11.95 | 310.64 | -60.30 | 79.41 | 0.8665 | -702.4 | 999999 | |
| 0.00 | 1.48 | 0.00 | 1.49 | 11.47 | 310.00 | -60.94 | 79.97 | 0.8719 | -420.0 | -379.1 | |
| 0.96 | 5.49 | 0.96 | 5.45 | 10.69 | 310.15 | -60.79 | 80.86 | 0.8707 | -572.2 | -461.9 | |
| 6.02 | 7.06 | 6.12 | 7.18 | 11.01 | 309.60 | -61.34 | 80.50 | 0.8753 | -548.8 | -468.8 | |
| 0.00 | 3.66 | 0.00 | 3.75 | 11.35 | 309.34 | -61.60 | 80.10 | 0.8774 | -10.0 | -35.0 | |
| 16.13 | 104.92 | 16.35 | 106.29 | 9.39 | 309.75 | -61.19 | 82.36 | 0.8742 | -907.4 | -343.9 | |
| 0.78 | 3.05 | 0.81 | 3.14 | 10.83 | 309.27 | -61.66 | 80.70 | 0.8780 | -524.1 | -365.5 | |
| 4.10 | 5.67 | 4.24 | 5.86 | 10.24 | 309.09 | -61.85 | 81.37 | 0.8795 | -576.9 | -414.6 | |
| 2.88 | -8.00 | 2.96 | -8.00 | 9.80 | 309.24 | -61.70 | 81.88 | 0.8784 | -484.0 | 999999 | |
| 1.92 | 92.45 | 2.05 | 100.07 | 11.85 | 308.09 | -62.85 | 79.53 | 0.8875 | 264.1 | 196.4 | |
| 1.13 | 3.05 | 1.18 | 3.18 | 9.91 | 308.81 | -62.13 | 81.74 | 0.8819 | -465.5 | -426.1 | |
| 0.00 | 4.10 | 0.00 | 4.31 | 10.44 | 308.56 | -62.37 | 81.14 | 0.8838 | -523.0 | -399.6 | |
| 0.44 | -12.00 | 0.46 | -12.00 | 11.49 | 308.10 | -62.84 | 79.94 | 0.8874 | -322.6 | 999999 | |
| 0.00 | 0.52 | 0.00 | 0.55 | 10.04 | 308.57 | -62.37 | 81.58 | 0.8838 | -375.0 | -346.3 | |
| 3.14 | -12.00 | 3.39 | -12.00 | 12.18 | 307.68 | -63.26 | 79.16 | 0.8907 | -613.1 | 999999 | |
| 1.05 | -12.00 | 1.11 | -12.00 | 11.01 | 308.15 | -62.78 | 80.49 | 0.8870 | -182.2 | 999999 | |
| 1.31 | -12.00 | 1.42 | -12.00 | 11.97 | 307.63 | -63.31 | 79.40 | 0.8911 | -692.7 | 999999 | |
| 0.78 | 5.76 | 0.83 | 6.12 | 9.43 | 308.51 | -62.43 | 82.28 | 0.8844 | 303.9 | 216.2 | |
| 0.35 | 1.66 | 0.37 | 1.76 | 10.14 | 308.27 | -62.67 | 81.47 | 0.8862 | -406.5 | -333.8 | |
| 1.05 | 3.14 | 1.11 | 3.33 | 9.59 | 308.26 | -62.68 | 82.09 | 0.8864 | -256.6 | -301.3 | |
| 8.55 | -12.00 | 9.19 | -12.00 | 10.22 | 307.84 | -63.10 | 81.37 | 0.8896 | -284.6 | 999999 | |
| 0.00 | 1.13 | 0.00 | 1.20 | 8.33 | 308.38 | -62.56 | 83.52 | 0.8857 | 298.0 | 278.8 | |
| 1.31 | 3.14 | 1.48 | 3.55 | 12.37 | 306.26 | -64.68 | 78.95 | 0.9015 | -179.2 | -18.3 | |
| 0.00 | 1.48 | 0.00 | 1.69 | 12.66 | 306.12 | -64.82 | 78.62 | 0.9025 | 403.0 | 351.8 | |
| 0.00 | 2.70 | 0.00 | 3.05 | 11.01 | 306.42 | -64.52 | 80.46 | 0.9004 | 634.0 | 547.5 | |
| 0.00 | 1.13 | 0.00 | 1.31 | 12.41 | 305.72 | -65.21 | 78.90 | 0.9054 | -337.0 | -161.2 | |
| 2.09 | 31.83 | 2.41 | 37.43 | 11.11 | 305.87 | -65.07 | 80.33 | 0.9044 | 371.3 | 75.1 | |
| 1.22 | 3.31 | 1.42 | 3.87 | 11.72 | 305.53 | -65.41 | 79.65 | 0.9068 | 305.4 | 317.1 | |
| 0.00 | 0.87 | 0.00 | 1.00 | 10.55 | 306.03 | -64.91 | 80.96 | 0.9033 | 136.0 | 112.3 | |
| 12.12 | -29.00 | 14.33 | -29.00 | 11.23 | 305.15 | -65.79 | 80.19 | 0.9096 | -526.6 | 999999 | |
| 3.66 | 5.23 | 4.57 | 6.54 | 13.24 | 303.68 | -67.26 | 77.97 | 0.9196 | -301.1 | -61.4 | |
| 0.00 | 0.61 | 0.00 | 0.77 | 13.49 | 303.37 | -67.57 | 77.70 | 0.9216 | -152.0 | -85.4 | |
| 0.00 | 2.44 | 0.00 | 3.02 | 11.37 | 303.94 | -67.00 | 80.01 | 0.9180 | 506.0 | 480.0 | |
| 2.53 | 11.43 | 3.13 | 14.02 | 10.61 | 303.90 | -67.04 | 80.85 | 0.9184 | 477.4 | 504.4 | |
| 0.00 | 0.87 | 0.00 | 1.10 | 11.63 | 303.41 | -67.53 | 79.72 | 0.9215 | 529.0 | 493.1 | |
| 0.00 | 33.14 | 0.00 | 42.83 | 12.71 | 302.84 | -68.10 | 78.54 | 0.9252 | 660.0 | 537.0 | |
| 0.00 | 1.22 | 0.00 | 1.54 | 11.17 | 303.39 | -67.54 | 80.22 | 0.9217 | 506.0 | 434.4 | |
| 1.83 | 33.32 | 2.37 | 44.09 | 11.82 | 302.82 | -68.12 | 79.50 | 0.9254 | 610.2 | 266.8 | |
| 0.00 | 2.35 | 0.00 | 3.02 | 11.23 | 303.04 | -67.90 | 80.15 | 0.9241 | 517.0 | 437.7 | |
| 2.01 | -40.00 | 2.64 | -40.00 | 11.84 | 302.39 | -68.55 | 79.47 | 0.9282 | 411.0 | 999999 | |
| 2.97 | -40.00 | 3.90 | -40.00 | 11.42 | 302.45 | -68.49 | 79.92 | 0.9279 | -293.5 | 999999 | |
| 2.44 | -40.00 | 3.24 | -40.00 | 11.55 | 302.21 | -68.73 | 79.78 | 0.9294 | 443.1 | 999999 | |
| 0.00 | 1.40 | 0.00 | 1.91 | 11.75 | 301.40 | -69.54 | 79.54 | 0.9343 | 464.0 | 377.0 | |
| 0.00 | 1.22 | 0.00 | 1.75 | 12.40 | 300.47 | -70.47 | 78.82 | 0.9398 | 482.0 | 437.1 | |
| 0.00 | 1.13 | 0.00 | 1.67 | 12.34 | 299.85 | -71.09 | 78.86 | 0.9434 | 374.0 | 350.8 | |
| 1.83 | 5.23 | 2.66 | 7.55 | 11.61 | 300.21 | -70.73 | 79.65 | 0.9414 | 459.1 | 470.7 | |
| 2.09 | 8.81 | 3.11 | 13.05 | 11.84 | 299.69 | -71.25 | 79.39 | 0.9444 | 334.8 | 440.7 | |
| 1.05 | 3.84 | 1.70 | 6.25 | 14.07 | 297.87 | -73.07 | 76.99 | 0.9537 | 179.3 | 178.3 | |
| 3.75 | 63.49 | 5.83 | 101.11 | 12.74 | 298.79 | -72.15 | 78.42 | 0.9491 | 418.8 | -41.6 | |
| 5.41 | -51.00 | 8.36 | -51.00 | 12.41 | 298.92 | -72.02 | 78.76 | 0.9485 | 422.8 | 999999 | |
| 0.00 | 1.05 | 0.00 | 1.55 | 11.11 | 299.74 | -71.20 | 80.16 | 0.9442 | 374.0 | 302.8 | |
| 0.00 | 1.22 | 0.00 | 1.85 | 11.50 | 299.32 | -71.62 | 79.74 | 0.9465 | 165.0 | 115.6 | |
| 0.00 | 2.27 | 0.00 | 3.90 | 13.30 | 296.86 | -74.08 | 77.77 | 0.9589 | -380.0 | -294.8 | |
| 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. | |