The team will meet twice in Bern:
\nOnce for one week in autumn 2016, and then in early summer 2017.<\/p>\n
The following activities will be carried out: 2. Creation of artificial data sets for validation purposes 1st Team Meeting:<\/strong><\/em> <\/p>\n II. Preparation before the 2nd Team Meeting:<\/strong> 2nd Team Meeting:<\/em><\/strong> The team will meet twice in Bern: Once for one week in autumn 2016, and then in early summer 2017. The following activities will be carried out: I. Preparations before the 1st Team Meeting: 1. Analysis of one common data … Continue reading
\nI. Preparations before the 1st Team Meeting:<\/strong>
\n1. Analysis of one common data set by the various groups
\n1.1 Selection of three data sets from HMI, MDI, and GONG for analysis
\n1.2 Meridional flow estimates with time-distance helioseismology and, global helioseismology, and supergranulation tracking<\/p>\n
\n2.1 Full sphere hydrodynamic numerical simulations of wave advection by a meridional flow with various flow configurations:
\n– single-cell meridional flow and multi-cellular meridional flow<\/p>\n
\n– Presentation of methods used
\n– Compare results from common datasets
\n– Discussion on origin of systematic effects and noise impact
\n– Discussion of further comparison work
\no Requirements on numerical simulations
\no Requirements on instrumental knowledge<\/p>\n
\n1. Setup of improved numerical simulations
\n1.1. Implementation\u00a0of systematic effects
\n1.2. Inclusion of realistic noise properties
\n2. Re-Analysis of selected data sets
\n3. Analysis of 21 years of helioseismic data by the team members<\/p>\n
\n– Discussion of updated results
\n– Conclusions on meridional flow measurements
\n– Preparation of long-term data set for studying temporal variation
\n– Discussion of temporal evolution of meridional flow
\n– Relation of meridional flow variations with variation of differential rotation and solar activity.<\/p>\n","protected":false},"excerpt":{"rendered":"