SDO HMI 2014-08-30 01:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.80 | 147.75 | 23.68 | 107.84 | -15.96 | 205.12 | -41.54 | 119.65 | 0.7356 | -57.1 | -222.3 | |
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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 | 1.25 | 0.00 | 0.89 | -18.19 | 208.31 | -38.35 | 124.34 | 0.7162 | 499.0 | 407.9 | |
| 2.24 | 4.39 | 1.58 | 3.10 | -17.87 | 208.19 | -38.47 | 123.87 | 0.7154 | 781.0 | 570.2 | |
| 0.00 | 1.61 | 0.00 | 1.09 | -14.30 | 209.01 | -37.65 | 119.93 | 0.6853 | 52.0 | 137.8 | |
| 0.00 | 1.88 | 0.00 | 1.29 | -15.10 | 208.72 | -37.94 | 120.77 | 0.6932 | 816.0 | 566.4 | |
| 3.67 | 10.75 | 2.60 | 7.62 | -17.62 | 207.97 | -38.69 | 123.42 | 0.7162 | 839.8 | 589.0 | |
| 2.06 | -5.00 | 1.46 | -5.00 | -17.80 | 207.76 | -38.90 | 123.50 | 0.7194 | 604.1 | 999999 | |
| 0.54 | 3.14 | 0.38 | 2.24 | -17.58 | 207.32 | -39.34 | 122.94 | 0.7224 | 575.8 | 417.6 | |
| 0.00 | 2.06 | 0.00 | 1.46 | -16.54 | 207.05 | -39.61 | 121.51 | 0.7191 | 224.0 | 241.0 | |
| 0.00 | 1.16 | 0.00 | 0.86 | -18.69 | 205.97 | -40.69 | 123.42 | 0.7422 | 660.0 | 532.2 | |
| 1.08 | 2.60 | 0.77 | 1.86 | -16.56 | 206.47 | -40.19 | 121.17 | 0.7252 | 599.9 | 504.9 | |
| 5.20 | 38.71 | 3.67 | 27.43 | -14.98 | 206.56 | -40.10 | 119.27 | 0.7156 | 696.7 | -86.1 | |
| 0.54 | -11.00 | 0.38 | -11.00 | -14.67 | 206.43 | -40.23 | 118.79 | 0.7153 | 625.8 | 999999 | |
| 3.40 | -11.00 | 2.41 | -11.00 | -14.53 | 206.21 | -40.45 | 118.48 | 0.7168 | 557.2 | 999999 | |
| 0.00 | 1.16 | 0.00 | 0.83 | -14.23 | 205.95 | -40.71 | 117.95 | 0.7180 | 245.0 | 123.0 | |
| 1.43 | 4.57 | 1.03 | 3.30 | -15.65 | 205.57 | -41.09 | 119.51 | 0.7295 | 169.9 | -233.5 | |
| 0.00 | 1.08 | 0.00 | 0.77 | -15.18 | 205.44 | -41.22 | 118.85 | 0.7284 | -621.0 | -528.2 | |
| 0.00 | 1.08 | 0.00 | 0.77 | -15.05 | 205.43 | -41.23 | 118.68 | 0.7278 | -242.0 | -236.9 | |
| 0.00 | 1.08 | 0.00 | 0.78 | -15.81 | 205.24 | -41.42 | 119.51 | 0.7338 | -113.0 | -47.1 | |
| 0.00 | 2.78 | 0.00 | 2.09 | -18.46 | 204.37 | -42.29 | 122.18 | 0.7564 | -580.0 | -480.0 | |
| 0.00 | 1.16 | 0.00 | 0.85 | -16.13 | 204.99 | -41.67 | 119.76 | 0.7380 | -143.0 | -74.9 | |
| 0.63 | 1.61 | 0.45 | 1.15 | -13.91 | 205.48 | -41.18 | 117.28 | 0.7214 | 612.1 | 464.6 | |
| 0.00 | 1.61 | 0.00 | 1.18 | -15.42 | 204.83 | -41.83 | 118.80 | 0.7360 | -384.0 | -342.6 | |
| 2.24 | 6.18 | 1.63 | 4.50 | -15.19 | 204.85 | -41.81 | 118.53 | 0.7346 | -757.8 | -556.1 | |
| 0.00 | 0.90 | 0.00 | 0.65 | -14.15 | 204.88 | -41.78 | 117.26 | 0.7290 | 263.0 | 183.5 | |
| 0.00 | 0.99 | 0.00 | 0.72 | -15.28 | 204.23 | -42.43 | 118.29 | 0.7414 | -630.0 | -518.2 | |
| 0.00 | 0.63 | 0.00 | 0.46 | -14.52 | 204.42 | -42.24 | 117.45 | 0.7357 | -207.0 | -177.1 | |
| 0.00 | 1.16 | 0.00 | 0.85 | -14.36 | 204.41 | -42.25 | 117.25 | 0.7350 | 99.0 | 88.8 | |
| 0.63 | 36.65 | 0.46 | 27.49 | -15.46 | 204.01 | -42.65 | 118.39 | 0.7446 | -702.9 | -640.8 | |
| 1.79 | -28.00 | 1.33 | -28.00 | -15.84 | 203.79 | -42.88 | 118.73 | 0.7487 | -922.8 | 999999 | |
| 0.00 | 2.33 | 0.00 | 1.71 | -14.23 | 204.02 | -42.64 | 116.88 | 0.7385 | -673.0 | -534.8 | |
| 2.78 | -28.00 | 2.08 | -28.00 | -15.99 | 203.53 | -43.13 | 118.77 | 0.7521 | -870.2 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.73 | -14.63 | 203.88 | -42.78 | 117.30 | 0.7418 | 470.0 | 343.1 | |
| 0.00 | 1.25 | 0.00 | 0.95 | -16.66 | 203.08 | -43.58 | 119.32 | 0.7598 | -715.0 | -572.7 | |
| 2.60 | -28.00 | 1.96 | -28.00 | -15.99 | 203.18 | -43.48 | 118.58 | 0.7556 | -803.9 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.55 | -17.58 | 202.72 | -43.94 | 120.21 | 0.7678 | -434.0 | -420.8 | |
| 0.00 | 0.90 | 0.00 | 0.69 | -17.75 | 202.62 | -44.04 | 120.36 | 0.7696 | -724.0 | -634.1 | |
| 1.97 | -28.00 | 1.49 | -28.00 | -16.15 | 202.87 | -43.79 | 118.61 | 0.7594 | -625.0 | 999999 | |
| 0.00 | 2.15 | 0.00 | 1.67 | -17.84 | 202.32 | -44.34 | 120.31 | 0.7729 | -803.0 | -672.4 | |
| 0.00 | 0.81 | 0.00 | 0.63 | -17.64 | 202.39 | -44.27 | 120.11 | 0.7713 | -465.0 | -498.2 | |
| 0.00 | 1.43 | 0.00 | 1.08 | -15.43 | 202.85 | -43.81 | 117.73 | 0.7562 | -448.0 | -456.8 | |
| 0.00 | 1.34 | 0.00 | 1.05 | -18.02 | 201.86 | -44.80 | 120.27 | 0.7781 | -574.0 | -519.2 | |
| 0.00 | 0.90 | 0.00 | 0.70 | -16.60 | 201.50 | -45.16 | 118.42 | 0.7750 | -457.0 | -355.5 | |
| 0.00 | 1.34 | 0.00 | 1.09 | -19.27 | 200.56 | -46.10 | 121.02 | 0.7960 | -596.0 | -485.1 | |
| 0.00 | 1.70 | 0.00 | 1.39 | -19.45 | 200.40 | -46.26 | 121.15 | 0.7983 | -475.0 | -379.8 | |
| 0.00 | 0.27 | 0.00 | 0.21 | -16.63 | 201.22 | -45.44 | 118.31 | 0.7778 | -369.0 | -359.3 | |
| 0.00 | 1.43 | 0.00 | 1.16 | -17.94 | 200.20 | -46.47 | 119.32 | 0.7933 | -546.0 | -449.3 | |
| 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. | |