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RSS_AR11147_A-A_L1.1.fits
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RSS_AR11770_A-A_L1.1.fits
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RSS_AR12158_A-A_L1.1.fits
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RSS_AR12420_A-B_L1.1.fits
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RSS_AR12422_A-A_L1.1.fits
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RSS_Documentation_and_Definition.pdf
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http://eprints.org/relation/isVersionOf https://data.lancashire.ac.uk/id/document/388 http://eprints.org/relation/isVolatileVersionOf https://data.lancashire.ac.uk/id/document/388 http://eprints.org/relation/isIndexCodesVersionOf https://data.lancashire.ac.uk/id/document/388 archive 486 disk0/00/00/02/14 2019-12-23 14:30:46 2023-07-24 13:32:39 2019-12-23 14:30:46 data_collection show Brown Daniel Stephen DSBrown@uclan.ac.uk 0000-0002-1618-8816 Walker Andrew Sunspot rotation data: test regions F530 2023sub_E_C_M_P Sun, sunspot, rotation These files contain calculated sunspot torsional rotation profiles for 5 active regions (and 6 sunspots) measured from data acquired by the HMI instrument on NASA's Solar Dynamics Orbiter. Other ancillary data produced as part of the calculations (such as uncertainties, umbral areas, sunspot position, and so on) are also included with the profiles. The five regions were used as testing and development data for validating the approach of Brown and Walker. These are provided as FITS files (one for each active region), and can be easily read into standard analysis packages used within solar physics (directions for doing this for SSWIDL and Scientific Python are given). 10.17030/uclan.data.00000214 dataset ST/M00760X/1 STFC ST/K501943/1 STFC RG_096 rdmsupport@uclan.ac.uk Contributor Brown Daniel Stephen DSBrown@uclan.ac.uk The impact of sunspot rotation on solar flares thesis 23606 http://clok.uclan.ac.uk/23606/ Semi-Automatic Method to Measure the Rotation of Sunspots. Solar Physics . pub http://clok.uclan.ac.uk/35586/ Original data taken from the SDO/HMI instrument. Processed using the method of Brown and Walker to produce bulk rotation profiles and other ancillary data. 2011-01-17 2015-09-30