| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 126.99 | 480.60 | 87.34 | 332.55 | -17.87 | 325.04 | 43.86 | 251.35 | 0.6966 | 71.9 | 109.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-03-17 01:00:30 UT
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 | 0.78 | 0.00 | 0.58 | -13.87 | 329.81 | 48.63 | 257.76 | 0.7478 | 366.0 | 392.8 | |
| 0.00 | 1.48 | 0.00 | 1.09 | -13.56 | 329.59 | 48.40 | 258.17 | 0.7451 | 564.0 | 407.2 | |
| 21.66 | 144.98 | 16.17 | 107.96 | -16.83 | 329.84 | 48.65 | 253.81 | 0.7506 | 681.3 | 268.4 | |
| 11.83 | -3.00 | 8.71 | -3.00 | -16.92 | 329.12 | 47.93 | 253.59 | 0.7427 | 846.6 | 999999 | |
| 0.00 | 0.61 | 0.00 | 0.46 | -19.68 | 329.71 | 48.53 | 250.02 | 0.7530 | 533.0 | 472.6 | |
| 0.00 | 0.70 | 0.00 | 0.51 | -18.63 | 328.97 | 47.79 | 251.29 | 0.7434 | 53.0 | 181.9 | |
| 0.00 | 0.87 | 0.00 | 0.62 | -13.41 | 327.19 | 46.00 | 258.21 | 0.7172 | 447.0 | 337.1 | |
| 0.00 | 1.13 | 0.00 | 0.82 | -17.26 | 328.12 | 46.93 | 253.00 | 0.7319 | 182.0 | 264.8 | |
| 0.00 | 0.78 | 0.00 | 0.56 | -16.79 | 327.87 | 46.69 | 253.61 | 0.7285 | 442.0 | 420.3 | |
| 1.13 | 7.65 | 0.81 | 5.45 | -16.52 | 327.38 | 46.20 | 253.90 | 0.7225 | 593.9 | 533.6 | |
| 0.70 | -10.00 | 0.49 | -10.00 | -16.17 | 327.19 | 46.00 | 254.36 | 0.7198 | 712.5 | 999999 | |
| 0.00 | 1.04 | 0.00 | 0.74 | -15.97 | 327.08 | 45.90 | 254.63 | 0.7183 | 242.0 | 293.0 | |
| 15.57 | 49.40 | 11.17 | 35.43 | -17.52 | 327.52 | 46.34 | 252.55 | 0.7255 | 749.0 | 300.8 | |
| 1.48 | 2.78 | 1.05 | 1.97 | -16.50 | 326.93 | 45.74 | 253.87 | 0.7172 | 642.5 | 576.9 | |
| 4.44 | 7.57 | 3.14 | 5.36 | -16.93 | 326.88 | 45.70 | 253.26 | 0.7173 | 735.0 | 573.2 | |
| 0.00 | 1.83 | 0.00 | 1.29 | -16.28 | 326.68 | 45.50 | 254.14 | 0.7140 | 621.0 | 536.6 | |
| 4.35 | 44.09 | 3.05 | 30.67 | -17.45 | 326.24 | 45.05 | 252.44 | 0.7106 | 657.8 | 562.1 | |
| 0.00 | 1.48 | 0.00 | 1.02 | -14.81 | 325.31 | 44.13 | 256.04 | 0.6960 | 486.0 | 501.2 | |
| 0.00 | 0.61 | 0.00 | 0.42 | -16.47 | 325.55 | 44.36 | 253.71 | 0.7009 | 661.0 | 639.6 | |
| 0.00 | 1.83 | 0.00 | 1.25 | -15.12 | 325.18 | 43.99 | 255.57 | 0.6947 | 622.0 | 472.1 | |
| 4.52 | -17.00 | 3.16 | -17.00 | -17.91 | 325.85 | 44.67 | 251.72 | 0.7068 | 676.5 | 999999 | |
| 0.00 | 1.91 | 0.00 | 1.31 | -14.93 | 324.96 | 43.77 | 255.82 | 0.6918 | 728.0 | 616.3 | |
| 0.00 | 1.22 | 0.00 | 0.83 | -14.58 | 324.78 | 43.60 | 256.30 | 0.6893 | 374.0 | 407.1 | |
| 0.00 | 0.87 | 0.00 | 0.59 | -14.84 | 324.63 | 43.45 | 255.91 | 0.6877 | 514.0 | 586.1 | |
| 5.91 | -17.00 | 4.09 | -17.00 | -17.55 | 325.35 | 44.16 | 252.13 | 0.7003 | 877.1 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.65 | -15.43 | 324.74 | 43.56 | 255.06 | 0.6898 | 577.0 | 600.4 | |
| 0.00 | 0.35 | 0.00 | 0.23 | -11.82 | 323.80 | 42.61 | 260.27 | 0.6747 | 417.0 | 439.5 | |
| 0.00 | 0.61 | 0.00 | 0.41 | -15.15 | 324.50 | 43.31 | 255.44 | 0.6865 | 518.0 | 468.0 | |
| 0.00 | 0.78 | 0.00 | 0.52 | -12.75 | 322.74 | 41.56 | 258.79 | 0.6619 | 232.0 | 219.8 | |
| 2.44 | 14.70 | 1.63 | 9.84 | -17.54 | 323.24 | 42.05 | 251.71 | 0.6749 | -399.9 | -43.4 | |
| 0.00 | 0.70 | 0.00 | 0.46 | -16.91 | 322.77 | 41.58 | 252.55 | 0.6679 | -448.0 | -440.9 | |
| 0.00 | 13.57 | 0.00 | 9.04 | -17.66 | 322.89 | 41.70 | 251.46 | 0.6710 | -453.0 | -242.3 | |
| 0.00 | 0.52 | 0.00 | 0.35 | -17.26 | 322.57 | 41.38 | 251.99 | 0.6662 | -113.0 | -238.8 | |
| 0.00 | 1.04 | 0.00 | 0.69 | -17.35 | 322.51 | 41.33 | 251.83 | 0.6657 | -411.0 | -292.8 | |
| 2.96 | 43.83 | 1.96 | 29.08 | -17.69 | 322.52 | 41.34 | 251.33 | 0.6665 | -594.3 | -199.7 | |
| 9.91 | -35.00 | 6.55 | -35.00 | -17.95 | 322.30 | 41.12 | 250.89 | 0.6644 | -760.3 | 999999 | |
| 0.00 | 1.22 | 0.00 | 0.80 | -17.33 | 322.09 | 40.90 | 251.78 | 0.6604 | -419.0 | -426.4 | |
| 0.00 | 1.30 | 0.00 | 0.87 | -18.92 | 322.46 | 41.27 | 249.49 | 0.6686 | -505.0 | -431.1 | |
| 0.00 | 0.78 | 0.00 | 0.52 | -19.42 | 322.02 | 40.84 | 248.64 | 0.6645 | -422.0 | -370.8 | |
| 0.61 | 2.44 | 0.40 | 1.61 | -19.61 | 322.00 | 40.81 | 248.35 | 0.6647 | -467.6 | -352.7 | |
| 0.00 | 0.87 | 0.00 | 0.57 | -18.34 | 321.33 | 40.15 | 250.07 | 0.6533 | -554.0 | -480.5 | |
| 0.00 | 0.87 | 0.00 | 0.57 | -19.49 | 321.58 | 40.40 | 248.41 | 0.6594 | -249.0 | -323.6 | |
| 0.00 | 0.70 | 0.00 | 0.45 | -18.50 | 321.21 | 40.03 | 249.79 | 0.6522 | -593.0 | -479.8 | |
| 1.48 | 7.13 | 0.97 | 4.69 | -19.71 | 321.44 | 40.26 | 248.03 | 0.6583 | -727.4 | -537.8 | |
| 0.00 | 0.70 | 0.00 | 0.46 | -19.50 | 321.38 | 40.19 | 248.33 | 0.6569 | -653.0 | -565.8 | |
| 0.00 | 1.04 | 0.00 | 0.68 | -19.54 | 320.89 | 39.71 | 248.13 | 0.6511 | -588.0 | -542.2 | |
| 0.00 | 1.04 | 0.00 | 0.68 | -19.10 | 320.64 | 39.46 | 248.72 | 0.6468 | -566.0 | -586.0 | |
| 0.00 | 0.61 | 0.00 | 0.40 | -19.87 | 320.66 | 39.47 | 247.56 | 0.6492 | -545.0 | -460.7 | |
| 0.00 | 2.44 | 0.00 | 1.58 | -19.69 | 320.49 | 39.30 | 247.77 | 0.6465 | -440.0 | -512.0 | |
| 3.91 | 7.39 | 2.54 | 4.79 | -20.60 | 320.35 | 39.16 | 246.35 | 0.6476 | 632.3 | 400.5 | |
| 0.00 | 0.87 | 0.00 | 0.56 | -19.82 | 320.07 | 38.89 | 247.44 | 0.6418 | 296.0 | 339.7 | |
| 0.00 | 1.83 | 0.00 | 1.16 | -18.29 | 319.45 | 38.26 | 249.59 | 0.6297 | -749.0 | -581.0 | |
| 0.00 | 0.96 | 0.00 | 0.62 | -21.71 | 320.41 | 39.22 | 244.71 | 0.6521 | -611.0 | -470.5 | |
| 0.00 | 1.13 | 0.00 | 0.72 | -19.52 | 319.13 | 37.95 | 247.59 | 0.6293 | -498.0 | -473.5 | |
| 0.00 | 0.87 | 0.00 | 0.56 | -20.24 | 319.30 | 38.11 | 246.52 | 0.6337 | -377.0 | -328.4 | |
| 0.00 | 1.65 | 0.00 | 1.05 | -20.10 | 319.14 | 37.95 | 246.68 | 0.6312 | -530.0 | -415.5 | |
| 0.00 | 1.39 | 0.00 | 0.89 | -20.71 | 319.31 | 38.13 | 245.82 | 0.6354 | -605.0 | -387.1 | |
| 0.00 | 1.39 | 0.00 | 0.89 | -21.20 | 319.34 | 38.15 | 245.07 | 0.6374 | -422.0 | -459.8 | |
| 0.00 | 1.39 | 0.00 | 0.88 | -19.33 | 318.76 | 37.58 | 247.75 | 0.6240 | -420.0 | -338.2 | |
| 1.22 | 3.13 | 0.78 | 1.99 | -20.42 | 318.99 | 37.80 | 246.13 | 0.6304 | -533.0 | -437.8 | |
| 25.13 | 50.18 | 15.84 | 31.64 | -20.16 | 318.27 | 37.09 | 246.26 | 0.6207 | -817.9 | -310.7 | |
| 0.00 | 0.78 | 0.00 | 0.49 | -19.15 | 317.84 | 36.66 | 247.71 | 0.6118 | -637.0 | -538.7 | |
| 0.43 | 1.39 | 0.27 | 0.87 | -19.48 | 317.49 | 36.31 | 247.05 | 0.6085 | 532.2 | 484.8 | |
| 0.00 | 0.87 | 0.00 | 0.54 | -19.43 | 317.32 | 36.14 | 247.06 | 0.6062 | 353.0 | 247.5 | |
| 2.96 | 4.78 | 1.86 | 3.01 | -21.25 | 317.74 | 36.56 | 244.35 | 0.6181 | -657.4 | -528.4 | |
| 0.00 | 0.70 | 0.00 | 0.43 | -19.18 | 316.91 | 35.72 | 247.30 | 0.6000 | -642.0 | -548.5 | |
| 0.00 | 0.78 | 0.00 | 0.49 | -20.15 | 317.12 | 35.93 | 245.82 | 0.6062 | -624.0 | -530.0 | |
| 2.09 | 15.31 | 1.30 | 9.51 | -20.74 | 317.12 | 35.94 | 244.89 | 0.6084 | -535.1 | 69.8 | |
| 0.00 | 3.04 | 0.00 | 1.88 | -19.50 | 316.72 | 35.53 | 246.71 | 0.5987 | -646.0 | -538.1 | |
| 0.00 | 2.26 | 0.00 | 1.41 | -21.60 | 317.20 | 36.02 | 243.57 | 0.6128 | -705.0 | -512.1 | |
| 1.04 | 2.44 | 0.65 | 1.52 | -21.18 | 317.04 | 35.86 | 244.16 | 0.6092 | -760.2 | -625.9 | |
| 0.00 | 0.87 | 0.00 | 0.53 | -19.40 | 316.42 | 35.23 | 246.75 | 0.5945 | -622.0 | -615.8 | |
| 1.22 | -68.00 | 0.75 | -68.00 | -20.68 | 316.63 | 35.45 | 244.77 | 0.6020 | 655.0 | 999999 | |
| 0.00 | 1.04 | 0.00 | 0.64 | -19.44 | 316.20 | 35.01 | 246.59 | 0.5918 | -402.0 | -458.2 | |
| 0.00 | 1.48 | 0.00 | 0.88 | -17.22 | 313.74 | 32.55 | 249.36 | 0.5513 | -705.0 | -531.6 | |
| 0.00 | 0.87 | 0.00 | 0.52 | -21.80 | 313.79 | 32.61 | 241.54 | 0.5713 | -606.0 | -464.5 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |