The Mees Solar Observatory of the University of Hawaii regularly archives solar observation data. The archive includes solar active region maps, white light telescope images, imaging vector magnetograph images, and Haleakala Stokes Polarimeter Magnetograms. Data from instruments like the Dual Coronagraph and the P-Mode Oscillations Instrument are also available.
Use Cases
- Analyze solar active region evolution based on active region maps
- Study solar magnetic fields based on imaging vector magnetograph images and Stokes polarimeter magnetograms
- Monitor solar oscillations based on P-mode oscillation images
- Observe solar corona features based on dual coronagraph images
- Track daily scintillation patterns based on daily scintillometer plots
Strengths
- Data originates from a dedicated solar observatory, the University of Hawaii Mees Solar Observatory
- The description lists multiple specific instrument outputs, including magnetograms and coronagraph images
Limitations
- Row count, file formats, and sample data are unknown, which may limit suitability assessment
- Column-level documentation is absent; field semantics must be inferred after download
- Last update date is unknown; freshness unverified
Provenance
- Source
- University of Hawaii Mees Solar Observatory
- Collection Method
- Regular observations from solar telescopes and instruments.