2.7.0 spase://ESA/NumericalData/SolarOrbiter/PHI/HRT/BINC/PT60S ESA NumericalData Solar Orbiter PHI HRT Continuum Intensity 2025-02-04T00:08:46 2025-05-02T00:08:46 Updated the Contact Magnetic field inclination computed by the RTE inversion Solar Orbiter is a space mission of international collaboration between ESA and NASA, operated by ESA. We are grateful to the ESA SOC and MOC teams for their support. The German contribution to SO/PHI is funded by the BMWi through DLR and by MPG central funds. The Spanish contribution is funded by AEI/MCIN/10.13039/501100011033/ and European Union “NextGenerationEU”/PRTR” (RTI2018-096886-C5, PID2021-125325OB-C5, PCI2022-135009-2, PCI2022-135029-2) and ERDF “A way of making Europe”; “Center of Excellence Severo Ochoa” awards to IAA-CSIC (SEV-2017-0709, CEX2021-001131-S); and a Ramón y Cajal fellowship awarded to D. Orozco Suárez. The French contribution is funded by CNES. spase://SMWG/Person/Joachim.Woch ProjectManager spase://SMWG/Person/Sami.K.Solanki PrincipalInvestigator spase://SMWG/Person/Gherardo.Valori CoPI The SO/PHI Instrument paper https://doi.org/10.1051/0004-6361/201935325 The SO/PHI Website https://www.mps.mpg.de/solar-physics/solar-orbiter-phi spase://ESA/Repository/SolarOrbiterArchive Online Open Solar Orbiter Archive https://soar.esac.esa.int/soar/ FITS spase://SMWG/Repository/SDAC Online Open https://umbra.nascom.nasa.gov/solar_orbiter/science/PHI/L2/ FITS Calibrated spase://ESA/Instrument/SolarOrbiter/PHI Magnetogram Sun.Photosphere FITS Data Array Magnetic field inclination DirectionAngle Magnetic Cartesian HPC Array size: 2048x2048 Pixel Resolution: 0.5 arcsec