SDO HMI 2014-05-17 12:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.02 | 378.62 | 40.30 | 248.39 | -13.85 | 229.22 | 39.55 | 250.96 | 0.6554 | 335.7 | 250.8 | |
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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 | 0.72 | 0.00 | 0.66 | -11.38 | 246.63 | 56.96 | 258.00 | 0.8423 | 458.0 | 398.0 | |
| 0.00 | 0.99 | 0.00 | 0.87 | -11.27 | 245.20 | 55.52 | 257.99 | 0.8287 | 459.0 | 366.1 | |
| 0.00 | 0.36 | 0.00 | 0.31 | -11.26 | 243.68 | 54.01 | 257.84 | 0.8139 | 475.0 | 383.2 | |
| 0.00 | 0.90 | 0.00 | 0.75 | -12.24 | 242.81 | 53.13 | 256.53 | 0.8062 | 526.0 | 438.6 | |
| 0.00 | 2.70 | 0.00 | 2.04 | -9.73 | 238.46 | 48.78 | 259.18 | 0.7571 | 668.0 | 495.4 | |
| 0.00 | 0.54 | 0.00 | 0.40 | -13.09 | 237.26 | 47.58 | 254.54 | 0.7483 | 425.0 | 359.5 | |
| 0.00 | 1.98 | 0.00 | 1.44 | -10.74 | 236.58 | 46.91 | 257.58 | 0.7370 | 194.0 | 199.5 | |
| 0.00 | 1.17 | 0.00 | 0.85 | -11.07 | 236.61 | 46.93 | 257.13 | 0.7377 | 584.0 | 502.7 | |
| 0.00 | 1.89 | 0.00 | 1.35 | -5.90 | 235.71 | 46.03 | 264.11 | 0.7220 | 543.0 | 442.7 | |
| 0.00 | 1.71 | 0.00 | 1.24 | -11.02 | 236.28 | 46.60 | 257.14 | 0.7339 | 729.0 | 588.4 | |
| 0.00 | 1.44 | 0.00 | 1.07 | -14.43 | 237.10 | 47.43 | 252.74 | 0.7491 | 217.0 | 265.8 | |
| 0.00 | 0.81 | 0.00 | 0.57 | -7.23 | 234.86 | 45.18 | 262.19 | 0.7126 | 550.0 | 480.3 | |
| 0.00 | 0.90 | 0.00 | 0.63 | -7.61 | 234.69 | 45.01 | 261.65 | 0.7109 | 594.0 | 487.3 | |
| 0.00 | 0.90 | 0.00 | 0.63 | -7.85 | 234.63 | 44.96 | 261.30 | 0.7104 | 614.0 | 523.7 | |
| 0.00 | 1.44 | 0.00 | 1.00 | -6.91 | 234.43 | 44.75 | 262.60 | 0.7071 | 669.0 | 575.7 | |
| 0.00 | 3.15 | 0.00 | 2.26 | -13.67 | 235.35 | 45.68 | 253.36 | 0.7278 | 330.0 | 389.4 | |
| 0.00 | 1.35 | 0.00 | 0.96 | -14.41 | 234.78 | 45.10 | 252.22 | 0.7228 | 632.0 | 427.9 | |
| 0.00 | 0.81 | 0.00 | 0.54 | -14.14 | 230.92 | 41.25 | 251.53 | 0.6764 | -284.0 | -245.0 | |
| 32.89 | 295.39 | 21.80 | 195.26 | -13.25 | 230.32 | 40.65 | 252.65 | 0.6666 | 1119.9 | 389.6 | |
| 0.00 | 0.99 | 0.00 | 0.66 | -14.89 | 230.55 | 40.88 | 250.32 | 0.6740 | 139.0 | 159.7 | |
| 27.14 | -19.00 | 17.92 | -19.00 | -13.85 | 229.95 | 40.28 | 251.65 | 0.6636 | 983.2 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.59 | -15.04 | 229.80 | 40.12 | 249.86 | 0.6652 | 502.0 | 454.7 | |
| 0.00 | 0.81 | 0.00 | 0.53 | -12.85 | 229.18 | 39.51 | 252.91 | 0.6512 | 178.0 | 211.8 | |
| 0.00 | 1.08 | 0.00 | 0.72 | -16.32 | 229.65 | 39.97 | 247.93 | 0.6676 | -348.0 | -464.1 | |
| 0.00 | 1.17 | 0.00 | 0.77 | -15.76 | 229.39 | 39.72 | 248.64 | 0.6626 | 563.0 | 457.8 | |
| 0.00 | 0.63 | 0.00 | 0.41 | -14.25 | 228.93 | 39.26 | 250.72 | 0.6521 | 288.0 | 275.0 | |
| 0.00 | 1.26 | 0.00 | 0.81 | -12.77 | 228.56 | 38.89 | 252.84 | 0.6431 | 731.0 | 658.1 | |
| 0.00 | 0.81 | 0.00 | 0.52 | -12.13 | 228.41 | 38.74 | 253.78 | 0.6394 | -538.0 | -414.1 | |
| 0.00 | 1.35 | 0.00 | 0.85 | -11.35 | 227.34 | 37.66 | 254.67 | 0.6234 | -688.0 | -599.5 | |
| 0.00 | 2.61 | 0.00 | 1.63 | -10.07 | 226.84 | 37.17 | 256.58 | 0.6138 | -618.0 | -469.1 | |
| 0.00 | 1.08 | 0.00 | 0.68 | -11.33 | 226.79 | 37.11 | 254.54 | 0.6161 | -501.0 | -531.1 | |
| 0.00 | 0.99 | 0.00 | 0.62 | -15.62 | 226.07 | 36.40 | 247.50 | 0.6208 | -555.0 | -460.5 | |
| 0.00 | 1.26 | 0.00 | 0.77 | -14.46 | 223.69 | 34.02 | 248.27 | 0.5854 | -678.0 | -510.9 | |
| 0.00 | 1.17 | 0.00 | 0.71 | -14.15 | 223.60 | 33.93 | 248.73 | 0.5830 | -690.0 | -625.0 | |
| 0.00 | 2.43 | 0.00 | 1.50 | -17.49 | 223.90 | 34.22 | 243.51 | 0.6016 | -669.0 | -553.9 | |
| 0.00 | 2.61 | 0.00 | 1.56 | -12.78 | 222.79 | 33.11 | 250.68 | 0.5667 | -644.0 | -524.9 | |
| 0.00 | 0.90 | 0.00 | 0.55 | -15.79 | 222.80 | 33.12 | 245.63 | 0.5794 | -630.0 | -470.4 | |
| 0.00 | 0.72 | 0.00 | 0.43 | -14.52 | 222.31 | 32.64 | 247.48 | 0.5674 | -665.0 | -502.0 | |
| 0.00 | 2.25 | 0.00 | 1.36 | -18.52 | 221.34 | 31.66 | 240.32 | 0.5750 | -715.0 | -494.7 | |
| 0.00 | 1.53 | 0.00 | 0.96 | -24.71 | 221.43 | 31.75 | 231.13 | 0.6163 | 491.0 | 392.1 | |
| 0.00 | 3.41 | 0.00 | 1.98 | -14.28 | 219.13 | 29.46 | 246.11 | 0.5233 | -538.0 | -485.2 | |
| 0.00 | 2.07 | 0.00 | 1.20 | -14.50 | 218.98 | 29.31 | 245.62 | 0.5224 | -714.0 | -684.2 | |
| 0.00 | 1.08 | 0.00 | 0.65 | -20.55 | 219.96 | 30.29 | 236.13 | 0.5709 | -457.0 | -448.7 | |
| 0.00 | 1.71 | 0.00 | 1.01 | -19.02 | 218.43 | 28.75 | 237.39 | 0.5420 | -668.0 | -525.4 | |
| 0.00 | 0.90 | 0.00 | 0.52 | -19.20 | 217.33 | 27.66 | 236.19 | 0.5297 | -575.0 | -546.7 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -15.23 | 216.45 | 26.78 | 242.49 | 0.4921 | -682.0 | -469.2 | |
| 0.00 | 1.08 | 0.00 | 0.63 | -19.50 | 216.48 | 26.81 | 234.94 | 0.5214 | -801.0 | -696.2 | |
| 0.00 | 1.08 | 0.00 | 0.63 | -21.90 | 216.35 | 26.68 | 230.94 | 0.5386 | -433.0 | -362.7 | |
| 0.00 | 0.90 | 0.00 | 0.53 | -21.78 | 216.11 | 26.44 | 230.91 | 0.5348 | -608.0 | -556.8 | |
| 0.00 | 1.35 | 0.00 | 0.78 | -21.21 | 215.74 | 26.07 | 231.46 | 0.5259 | -760.0 | -628.1 | |
| 0.99 | 6.92 | 0.58 | 4.03 | -21.53 | 215.70 | 26.02 | 230.90 | 0.5280 | -921.2 | -728.5 | |
| 0.00 | 0.72 | 0.00 | 0.42 | -21.24 | 215.57 | 25.90 | 231.23 | 0.5241 | -720.0 | -693.0 | |
| 0.00 | 2.07 | 0.00 | 1.20 | -21.47 | 215.36 | 25.69 | 230.66 | 0.5236 | -890.0 | -702.0 | |
| 0.00 | 1.35 | 0.00 | 0.78 | -21.25 | 215.25 | 25.57 | 230.91 | 0.5204 | -901.0 | -724.4 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -22.67 | 212.67 | 22.99 | 225.88 | 0.5041 | -593.0 | -509.2 | |
| 0.00 | 0.99 | 0.00 | 0.58 | -25.68 | 213.10 | 23.43 | 221.97 | 0.5378 | -650.0 | -537.8 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -18.50 | 211.70 | 22.03 | 231.77 | 0.4547 | -763.0 | -568.7 | |
| 0.00 | 2.61 | 0.00 | 1.40 | -13.22 | 209.74 | 20.07 | 240.35 | 0.3861 | -835.0 | -663.4 | |
| 0.00 | 1.17 | 0.00 | 0.61 | -19.31 | 199.95 | 10.28 | 210.00 | 0.3381 | -923.0 | -808.2 | |
| 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. | |