2013
DOI: 10.1063/1.4810977
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Modeling the corona and solar wind using ADAPT maps that include far-side observations

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Cited by 94 publications
(79 citation statements)
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“…Synchronic maps are generated by flux transport models that incorporate rotational, meridional, and supergranular diffusive surface transport processes to predict the magnetic field in locations where direct measurements are not available [e.g., Devore et al , ; Sheeley et al , ; Worden and Harvey , ; Schrijver and De Rosa , ; Feng et al , , and references therein]. The magnetic flux transport model used here, as in Henney et al [], is the Air Force Data Assimilative Photospheric Flux Transport (ADAPT) model [ Arge et al , , , ], which utilizes a modified version of the flux transport model by Worden and Harvey []. A primary goal of ADAPT flux transport modeling is to generate global magnetic maps that provide the inner boundary condition for coronal and solar wind models [see, e.g., Lee et al , ; Linker et al , ].…”
Section: Global Solar Magnetic Mapsmentioning
confidence: 99%
“…Synchronic maps are generated by flux transport models that incorporate rotational, meridional, and supergranular diffusive surface transport processes to predict the magnetic field in locations where direct measurements are not available [e.g., Devore et al , ; Sheeley et al , ; Worden and Harvey , ; Schrijver and De Rosa , ; Feng et al , , and references therein]. The magnetic flux transport model used here, as in Henney et al [], is the Air Force Data Assimilative Photospheric Flux Transport (ADAPT) model [ Arge et al , , , ], which utilizes a modified version of the flux transport model by Worden and Harvey []. A primary goal of ADAPT flux transport modeling is to generate global magnetic maps that provide the inner boundary condition for coronal and solar wind models [see, e.g., Lee et al , ; Linker et al , ].…”
Section: Global Solar Magnetic Mapsmentioning
confidence: 99%
“…Recent studies began to take into account of the solar differential rotation when considering the distribution of photospheric magnetic field. Arge et al [] and Hickmann et al [] produced realistic estimates of the instantaneous global photospheric magnetic field distribution by using the Air Force Data Assimilative Photospheric Flux Transport model, which can assimilate helioseismic farside active region data and the evolved magnetic flux when the observation is not available. Lionello et al [] used a global 3‐D MHD model to study the effects of differential rotation on the coronal magnetic field by introducing an artificial differential rotation into a steady corona solution obtained from the time‐relaxation method.…”
Section: Introductionmentioning
confidence: 99%
“…They have also developed forecasts of the solar radio flux at 10.7 cm, known as the F 10.7 flux, using absolute field strengths from their flux-transport modeling, and improved reconstructions of coronal hole boundaries from potential-field sourcesurface models. In a case study, Arge et al (2013) included helioseismic data for active region emergence and development on the far side of the Sun and they reported further improvement in the performance of their model in this case.…”
Section: The Evolving "Synchronic" Synoptic Mapmentioning
confidence: 99%