SDO HMI 2014-03-11 17:00:29 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.51 | 177.95 | 16.28 | 89.11 | -10.08 | 357.94 | 6.45 | 239.71 | 0.1432 | 409.0 | 350.3 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-03-11 17:00:29 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 | 0.52 | 0.00 | 0.26 | -13.94 | 0.62 | 9.12 | 232.39 | 0.1952 | 15.0 | 13.3 | |
| 0.00 | 0.69 | 0.00 | 0.35 | -7.05 | 0.21 | 8.72 | 270.54 | 0.1511 | 852.0 | 770.9 | |
| 7.89 | 72.38 | 3.96 | 36.30 | -10.03 | 0.22 | 8.72 | 251.30 | 0.1584 | 1372.4 | 481.5 | |
| 0.00 | 1.91 | 0.00 | 0.96 | -6.13 | 0.14 | 8.64 | 276.69 | 0.1511 | 1061.0 | 907.3 | |
| 0.00 | 2.34 | 0.00 | 1.17 | -8.24 | 0.11 | 8.62 | 262.56 | 0.1503 | 1015.0 | 854.1 | |
| 0.00 | 3.90 | 0.00 | 1.95 | -8.01 | 0.05 | 8.55 | 264.11 | 0.1487 | 1218.0 | 941.8 | |
| 7.37 | -3.00 | 3.69 | -3.00 | -9.82 | 0.06 | 8.56 | 252.28 | 0.1547 | 1401.3 | 999999 | |
| 0.00 | 2.34 | 0.00 | 1.17 | -7.47 | 0.01 | 8.51 | 267.72 | 0.1476 | 885.0 | 808.2 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -6.34 | 359.96 | 8.46 | 275.42 | 0.1476 | 877.0 | 781.9 | |
| 0.00 | 2.17 | 0.00 | 1.08 | -7.68 | 359.77 | 8.27 | 266.19 | 0.1436 | 996.0 | 892.9 | |
| 17.25 | 22.02 | 8.63 | 11.02 | -9.32 | 359.59 | 8.09 | 254.68 | 0.1447 | 1185.9 | 731.5 | |
| 0.00 | 0.95 | 0.00 | 0.48 | -7.51 | 359.55 | 8.06 | 267.38 | 0.1398 | 850.0 | 657.3 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -8.65 | 359.27 | 7.78 | 258.96 | 0.1369 | 848.0 | 619.4 | |
| 0.00 | 1.73 | 0.00 | 0.87 | -7.25 | 359.12 | 7.63 | 269.27 | 0.1323 | 832.0 | 674.1 | |
| 0.00 | 7.63 | 0.00 | 3.81 | -7.55 | 359.07 | 7.57 | 266.99 | 0.1315 | 969.0 | 870.7 | |
| 0.00 | 2.25 | 0.00 | 1.13 | -7.99 | 358.98 | 7.49 | 263.52 | 0.1305 | 921.0 | 716.2 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -7.67 | 358.83 | 7.33 | 265.95 | 0.1274 | 792.0 | 518.6 | |
| 0.00 | 2.69 | 0.00 | 1.34 | -8.50 | 358.75 | 7.26 | 259.35 | 0.1277 | 1173.0 | 985.3 | |
| 0.00 | 1.91 | 0.00 | 0.96 | -14.20 | 358.89 | 7.40 | 225.49 | 0.1758 | 816.0 | 634.3 | |
| 0.00 | 1.56 | 0.00 | 0.78 | -7.34 | 358.70 | 7.21 | 268.51 | 0.1251 | 675.0 | 581.2 | |
| 0.00 | 1.47 | 0.00 | 0.74 | -8.60 | 358.42 | 6.92 | 258.14 | 0.1224 | 847.0 | 633.7 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -8.42 | 358.23 | 6.74 | 259.31 | 0.1187 | 933.0 | 790.4 | |
| 0.00 | 1.91 | 0.00 | 0.95 | -6.64 | 358.03 | 6.53 | 274.68 | 0.1139 | 983.0 | 720.8 | |
| 0.00 | 2.51 | 0.00 | 1.25 | -6.43 | 358.02 | 6.53 | 276.50 | 0.1143 | 917.0 | 752.2 | |
| 0.00 | 1.30 | 0.00 | 0.65 | -12.16 | 357.05 | 5.56 | 227.49 | 0.1291 | 956.0 | 780.7 | |
| 0.00 | 1.56 | 0.00 | 0.78 | -12.04 | 356.87 | 5.37 | 227.23 | 0.1254 | 897.0 | 715.0 | |
| 0.00 | 1.13 | 0.00 | 0.56 | -13.69 | 356.53 | 5.04 | 216.99 | 0.1425 | 955.0 | 741.7 | |
| 0.00 | 1.47 | 0.00 | 0.74 | -13.40 | 356.25 | 4.76 | 216.73 | 0.1355 | 958.0 | 801.6 | |
| 0.00 | 1.65 | 0.00 | 0.82 | -13.28 | 356.06 | 4.57 | 216.19 | 0.1320 | 1094.0 | 855.4 | |
| 0.00 | 1.91 | 0.00 | 0.95 | -13.40 | 355.88 | 4.39 | 214.55 | 0.1319 | 909.0 | 772.4 | |
| 0.00 | 1.13 | 0.00 | 0.57 | -15.90 | 355.37 | 3.88 | 203.28 | 0.1654 | -905.0 | -739.2 | |
| 0.00 | 1.13 | 0.00 | 0.56 | -14.18 | 355.34 | 3.85 | 208.16 | 0.1385 | 875.0 | 607.7 | |
| 0.00 | 1.73 | 0.00 | 0.87 | -15.72 | 354.50 | 3.01 | 198.83 | 0.1572 | -1085.0 | -865.5 | |
| 0.00 | 1.30 | 0.00 | 0.65 | -15.90 | 354.16 | 2.67 | 196.50 | 0.1584 | -895.0 | -765.5 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -15.45 | 354.00 | 2.51 | 196.40 | 0.1501 | -970.0 | -758.1 | |
| 0.00 | 0.78 | 0.00 | 0.39 | -15.63 | 353.97 | 2.48 | 195.88 | 0.1530 | -828.0 | -609.2 | |
| 0.00 | 1.73 | 0.00 | 0.87 | -15.51 | 353.79 | 2.29 | 194.95 | 0.1502 | -868.0 | -697.3 | |
| 0.00 | 3.47 | 0.00 | 1.72 | -8.37 | 353.16 | 1.67 | 234.92 | 0.0354 | -910.0 | -676.8 | |
| 0.00 | 1.39 | 0.00 | 0.69 | -13.57 | 352.12 | 0.62 | 185.45 | 0.1116 | -989.0 | -779.1 | |
| 0.00 | 0.87 | 0.00 | 0.43 | -11.11 | 350.38 | -1.11 | 164.38 | 0.0709 | -1001.0 | -815.5 | |
| 0.00 | 1.13 | 0.00 | 0.56 | -10.81 | 349.81 | -1.68 | 155.30 | 0.0694 | -988.0 | -700.8 | |
| 0.00 | 1.47 | 0.00 | 0.73 | -9.89 | 349.66 | -1.83 | 146.03 | 0.0565 | -1028.0 | -846.7 | |
| 0.00 | 1.99 | 0.00 | 0.99 | -9.50 | 349.55 | -1.95 | 139.98 | 0.0524 | -942.0 | -763.4 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -9.20 | 349.55 | -1.95 | 136.02 | 0.0485 | -950.0 | -717.2 | |
| 0.00 | 1.30 | 0.00 | 0.65 | -15.81 | 349.46 | -2.04 | 167.13 | 0.1541 | -875.0 | -705.2 | |
| 0.00 | 2.69 | 0.00 | 1.35 | -16.01 | 348.43 | -3.06 | 161.47 | 0.1622 | -861.0 | -741.2 | |
| 0.00 | 0.95 | 0.00 | 0.48 | -12.94 | 347.04 | -4.45 | 142.92 | 0.1261 | -918.0 | -703.5 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -13.71 | 346.26 | -5.24 | 142.03 | 0.1448 | -989.0 | -843.2 | |
| 0.00 | 0.87 | 0.00 | 0.43 | -13.32 | 346.27 | -5.23 | 140.32 | 0.1395 | -855.0 | -730.7 | |
| 0.00 | 1.30 | 0.00 | 0.66 | -19.22 | 345.43 | -6.06 | 154.46 | 0.2323 | -836.0 | -607.5 | |
| 0.00 | 1.30 | 0.00 | 0.65 | -10.23 | 345.57 | -5.92 | 117.70 | 0.1153 | -819.0 | -681.3 | |
| 0.00 | 1.39 | 0.00 | 0.70 | -12.11 | 340.45 | -11.05 | 115.04 | 0.2077 | -749.0 | -520.4 | |
| 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. | |