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| The second release of HMI vector magnetic field data can be found in the following JSOC data series: '''hmi.B_720s_e15w1332_cutout''' ([http://jsoc.stanford.edu/ajax/lookdata.html?ds=hmi.B_720s_e15w1332_cutout click here for data]) and '''hmi.B_720s_e15w1332_CEA''' ([http://jsoc.stanford.edu/ajax/lookdata.html?ds=hmi.B_720s_e15w1332_CEA click here for data]). |
The second release of HMI vector magnetic field data can be found in the following two JSOC data series: '''[http://jsoc.stanford.edu/ajax/lookdata.html?ds=hmi.B_720s_e15w1332_cutout hmi.B_720s_e15w1332_cutout]''' and '''[http://jsoc.stanford.edu/ajax/lookdata.html?ds=hmi.B_720s_e15w1332_CEA hmi.B_720s_e15w1332_CEA]'''. The first series is a "cutout" from the full-disk image; the second a cylindrical equal area projected map. |
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| This page contains a summary and links to the second release for HMI vector magnetic field data in several active regions. The Milne-Eddington inversion result prior to disambiguation, see the release notes for VFISV. | This page contains a brief summary of the included regions. The list will be updated as more regions are processed. |
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| The data are published | The reduction procedures for these data sets are identical to the first release (NOAA AR 11158). For detailed format, technical specification, and user guide, please refer to the previous documentation '''ReleaseNotes''' and '''VectorPaper'''. |
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| The data reduction procedures are identical to the first release for AR 11158. Please refer to the previous '''ReleaseNotes''' and '''VectorPaper''' for technical specification and user guide. Please contact the HMI vector team if you have any question or suggestion. | A synoptic data set of the full-disk Milne-Eddington inversion (without azimuthal ambiguity resolution) is available at a 12-hour cadence. You can find links to the data and release notes in the '''[http://jsoc.stanford.edu/jsocwiki/ME720se15w1332 ME720se15w1332]''' page. |
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| === Data Summary === | |
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| === Example === {{{ xxx }}} === Display === xxx |
|| '''Date''' || '''NOAA''' || '''Frames''' || '''Position''' || '''Notes''' || '''Image''' || '''Movie''' || '''Cutout''' || '''CEA''' || || 2010.05.20_12:00/6d || 11072 || 719 || || Flux emergence || || || [http://jsoc.stanford.edu/ajax/lookdata.html?ds=hmi.B_720s_e15w1332_cutout%5B11072%5D 512×512] || [http://jsoc.stanford.edu/ajax/lookdata.html?ds=hmi.B_720s_e15w1332_CEA%5B11072%5D 512×512] || || 2010.07.02_00:00/1d || 11084 || 120 || || Stable sunspot || || || [http://jsoc.stanford.edu/ajax/lookdata.html?ds=hmi.B_720s_e15w1332_cutout%5B11084%5D 512×512] || [http://jsoc.stanford.edu/ajax/lookdata.html?ds=hmi.B_720s_e15w1332_cutout%5B11084%5D 512×512] || || || 2011.02.12_00:00/5d || 11158 || 600 || || X-class flare (1st release) || || || [http://jsoc.stanford.edu/ajax/lookdata.html?ds=hmi.B_720s_e15w1332_cutout%5B11158%5D 650×600] || [http://jsoc.stanford.edu/ajax/lookdata.html?ds=hmi.B_720s_e15w1332_cutout%5B11158%5D 600×600] || || || 2011.03.06_00:00/5d || 11166 || 600 || || X-class flare || || || [http://jsoc.stanford.edu/ajax/lookdata.html?ds=hmi.B_720s_e15w1332_cutout%5B11166%5D 600×600] || [http://jsoc.stanford.edu/ajax/lookdata.html?ds=hmi.B_720s_e15w1332_cutout%5B11166%5D 600×600] || || || 2011.09.03_12:00/5d || 11283 || 600 || || X-class flare || || || [http://jsoc.stanford.edu/ajax/lookdata.html?ds=hmi.B_720s_e15w1332_cutout%5B11283%5D 600×512] || [http://jsoc.stanford.edu/ajax/lookdata.html?ds=hmi.B_720s_e15w1332_cutout%5B11283%5D 600×512] || || || 2010.05.20_12:00/5d || 11072 || 719 || || xxxxx || || || 512×512 || 512×512 || || |
Release Notes on HMI Vector Magnetic Field Data in Several Active Regions
The second release of HMI vector magnetic field data can be found in the following two JSOC data series: [http://jsoc.stanford.edu/ajax/lookdata.html?ds=hmi.B_720s_e15w1332_cutout hmi.B_720s_e15w1332_cutout] and [http://jsoc.stanford.edu/ajax/lookdata.html?ds=hmi.B_720s_e15w1332_CEA hmi.B_720s_e15w1332_CEA]. The first series is a "cutout" from the full-disk image; the second a cylindrical equal area projected map.
This page contains a brief summary of the included regions. The list will be updated as more regions are processed.
The reduction procedures for these data sets are identical to the first release (NOAA AR 11158). For detailed format, technical specification, and user guide, please refer to the previous documentation ReleaseNotes and VectorPaper.
A synoptic data set of the full-disk Milne-Eddington inversion (without azimuthal ambiguity resolution) is available at a 12-hour cadence. You can find links to the data and release notes in the [http://jsoc.stanford.edu/jsocwiki/ME720se15w1332 ME720se15w1332] page.