Conformal deprojections, e.g., Mercator, locally preserve angles; scales are ... imposed differential rotation profile; red dots are raw velocities from Mercator ...
Can we extend ILCT to LOS data sets? , where. Near disk center, we can approximate BLOS Bz. ... To decompose ILCT flow, uILCT , into (vx, vy, vz), we need B at ...
We have applied ILCT to IVM data from AR 9026, on 05 Jun 2000. ... ( Mercator?) What formats are most useful to end users? Probably both graphical & numerical. ...
In ideal MHD, photospheric flows move mag-netic flux with a flux ... We used both LCT & ILCT to derive flows between pairs of boxcar- averaged m'grams. ...
A means of specifying the photospheric boundary in a way consistent with the ... assume that ILCT or MEF flows permeate the entire layer, and implicitly solve ...
Time Series of Magnetograms: Evolution, Interpretations, Inferring Flows ... Tracking of white light images underway... Test velocity inversion methods... Data movie ...
Modelers prescribe fields and flows (B, v) to drive eruptions in MHD simulations ... and best guess at initial field topology (also just presented) ...
Yang Liu Stanford University yliu@solar.stanford.edu HMI Science Analysis Plan SDO/HMI Products From Vector Magnetograms Yang Liu Stanford University yliu@ ...
Can we accurately estimate the evolution of free energy? ... use new magnetographs (Solar-B /FPP, SOLIS VSM, SDO/HMI) to predict coronal energy release? ...
Determining electric fields and flows consistent with the ... Local Correlation Tracking' ... determined via local correlation tracking (applied to ...
From 2D data arrays, f1(x1,x2) & f2(x1,x2), find vector flow v(x1,x2) consistent ... (2005, in prep): Use (i) 'minium structure' & (ii) 'coplanarity' assumptions, ...
Big Bear Solar Observatory (NJIT) University of Hawaii. 4 ... CME-producing regions of the Sun ... the ecliptic plane and about 30 west of the Sun-Earth line. ...
Using WSRF to build workflow scripts: Temp files and filters in a Grid environment Michael Grobe Indiana University 1 Introduction Programmers frequently build ...
... evolution of the vector magnetic field in the photosphere. ... Convective granulation pattern small compared to the size scale of AR at the photosphere ...
More about flows in Poster previews! Modelers using these data to simulate eruptions! ... (BACK) Petrinec et al. (1998) Movie of Bow Shock, Magnetopause (BACK) ...
... field are available), chromosphere, transition region and. corona ... photosphere/chromosphere: energetics dominated by optically thick radiative transitions ...
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Temporal evolutions, and. Views from various directions. MHD models can give unobservables ... Synoptic / synchronic maps/frames. Global MHD/non-MHD models. Disk data ...
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HMI Magnetic Products & Pipeline http://jsoc.stanford.edu/jsocwiki/Lev1Doc HMI Magnetic Field Products Line-of-sight magnetic field will be computed from Doppler ...
Azimuth (phi) relative to solar north. Magnetic line-of sight velocity ... The three panels show Inclination, Azimuth & Magnetic Field Strength as observed ...
HMI AIA, M1-H2: Mag. Activity. 2. The Store and Release Paradigm' (cf. ... (More on FLCT in M3: Mag. Data Products, Thurs. ... HMI AIA, M1-H2: Mag. Activity. 5 ...
Evolution of small-scale magnetic elements (coronal heating) ... Connectivity & separatrix. Energy flux through the photosphere. Coronal/Helios. fields. ...
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... and density model to drive the model to obtain the following physical properties. ... This scheme achieves the second order accuracy both temporally and spatially. ...
Quiescent filaments are longer- lived than AR filaments, but can also produce halo CMEs. ... ( Eruptions come days later, or occur without flux emergence. ...
The Use of Vector Magnetogram Data in MHD Models of the Solar Atmosphere and Prospects for an Assimilative Model George H. Fisher Space Sciences Laboratory