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Abstract
in image in SECCHI Tool utilizing a series of Tool utilizing a series of LOS’s LOS’s from two views to define two views to shape, and velocity of 3D Structure of 3D Structure CMEsCMEs Program to compare analysis of SECCHI images on the internal Program to compare analysis of SECCHI images on the internal magnetic field configuration & near magnetic field configuration & near--Sun evolution of Sun evolution of CMEsCMEs with models based on SOHO observations. with models based on SOHO observations. Forecast flux rope structure; 3D visualization of Forecast flux rope structure; 3D visualization of CMEsCMEs. 2D maps each STEREO. 2D maps each STEREO. Tool for detecting and characterizing solar filaments and Tool for detecting and characterizing solar filaments and sigmoidssigmoids Recognition & Classification in solar images. Goal is to meas. m Recognition & Classification in solar images. Goal is to meas. magnetic agnetic helicityhelicity parameters & forecast eruptions using filaments & parameters & forecast eruptions using filaments & sigmoidssigmoids.. The Wang--SheeleySheeley--ArgeArge and ENLIL 3D MHD solar wind models will be integrated and ENLIL 3D MHD solar wind models will be integrated Provide routine predictions of vector Provide routine predictions of vector s.ws.w. velocity, polarity, . velocity, polarity, s.ws.w. density & temp. . density & temp. anywhere you like anywhere you like Produce simulations to show model Produce simulations to show model CMEsCMEs can be identified & tracked with the can be identified & tracked with the HIsHIs.. Use triangulation to measure speed & direction of Use triangulation to measure speed & direction of CMEsCMEs & forecast their Earth & forecast their Earth arrival. arrival. Use analyses of SMEI images to provide structural context of the Use analyses of SMEI images to provide structural context of the heliosphereheliosphere for for Also provide complementary observations of transient disturbance Also provide complementary observations of transient disturbances.s. Construct acceleration profiles of fast Construct acceleration profiles of fast ICMEsICMEs over a large heliocentric range over a large heliocentric range using multi using multi--point HI to understand the forces acting on point HI to understand the forces acting on ejectaejecta.. Improve predictions of arrival times of Improve predictions of arrival times of ICMEsICMEs at Earth. Earth. Assess the potential Assess the potential geoeffectivenessgeoeffectiveness of of CMEsCMEs based their association with based their association with magnetic clouds. magnetic clouds. What particular characteristics lead to production of a magnetic What particular characteristics lead to production of a magnetic cloud?cloud?