DOCFM Community Presentations 




 2014 Fall AGU (San Francisco) 


  • POSTER: "FORWARD" SolarSoft IDL Codes, Gibson  (also presented at IAUS305)


     2015 SPD (TESS) (Indianapolis)
    

  • POSTER: Observations of a coronal cavity and prominence with Hinode, IRIS, and AIA, Jibben and Reeves


     2015 IAU General Assembly (Honolulu)
    

  • TALK: Magnetism Matters: Coronal Magnetometry Using Multiwavelength Polarimetry,
Gibson et al. (also presented at 2015 IUGG)


     2015 Fall AGU (San Francisco)
    

  • TALK:  Towards a Data-Optimized Coronal Magnetic Field Model (DOC-FM): 
Synthetic Testbeds and Multiwavelength Forward Modeling, Gibson et al.


  • POSTER: Towards a Data-Optimized Coronal Magnetic Field Model (DOC-FM): 
Statistical Method for Diagnosing the Coronal Magnetic Field, Dalmasse et al(also SPD2016).


  • POSTER: Towards a Data-Optimized Coronal Magnetic Field Model (DOC-FM):
Simulating Flux Ropes with the Flux Rope Insertion Method, Savcheva et al.


     2016 NCAR Discovery Days (Boulder) 
    

  • TALK: Data-Optimized Coronal Magnetic Field Model (DOCFM), an HAO-CISL collaboration, Gibson and Nychka


     2016 SPD meeting (Boulder) 
    

  • TALK: CoMP linear polarization as a probe of coronal magnetic topology, Gibson et al.


  • TALK: Hinode and IRIS Observations of a Prominence-Cavity System, Jibben et al.


  • TALK:  An Airborne Infrared Spectrometer (AIR-Spec) for Solar Eclipse Observations, Samra et al.


  • POSTER:  Stability study of coronal cavities and prominences, de Toma and Gibson


  • POSTER: Simulating Idealized Flux Ropes with the Flux Rope Insertion Method: A Parameter Space 
Exploration of Currents and Topology, Savcheva et al.


  • POSTER: MHD simulation of the initiation of the 2006 December 13 coronal mass ejection
in AR 10930: the structure of the erupting flux rope, Fan



     2016 AGU Chapman conference (Croatia) 
    

  • POSTER: Simulating Idealized Flux Ropes with the Flux Rope Insertion Method: A Parameter Space 
Exploration of Currents and Topology, Savcheva et al.


     2016 SHINE meeting 
    

  • POSTER: Constraining coronal magnetic field models using coronal polarimetry, Dalmasse et al.


     2016 BZ team meeting (Albuquerque) 
    

  • TALK: Towards a Data-Optimized Coronal Field Model, Gibson et al.


     2016 Meteo Space conference (Nice) 
    

  • TALK: Constraining the coronal magnetic field from ground- and space-based observations, Dalmasse et al.


     2016 Ball Aerospace colloquium (Boulder) 
    

  •  TALK: Magnetism across time and space, Gibson


     2016: IRAP colloquium (Toulouse)
    

  •  TALK: Towards improved space weather forecasts, Dalmasse et al.


     2017: SolarNet 4 (Lanzarote)
    

  • TALK: Dynamics and diagnostics of the solar corona: Unchained magnetism", Gibson et al.


     2017: LESIA colloquium (Meudon)
    

  •  TALK: Constraining coronal magnetic field reconstructions using coronal polarimetry, Dalmasse et al.


     2017: NSO Solar Focus talk (Boulder)
    

  • TALK: Dynamics and diagnostics of the solar corona: unchained magnetism, Gibson et al.


     2017 BZ team meeting (Washington DC)
    

  • TALK: Space weather prediction through the observation and modeling of coronal magnetism, Gibson et al.


     2017: SPD (Portland)
    

  • TALK: MHD simulations of the eruption of prominence hosting coronal flux ropes, Fan


     2017: SPD (Portland)
    

  • TALK: Nonlinear force free field modeling for a pseudostreamer, Karna et al.


     2017: SPD (Portland)
    

  • TALK: Evolution of the Topology, Electric Currents, and Ribbons during an X-class Flare, Savcheva et al.


     2017: IAGA-IAMAS-IAPSO (Capetown)
    

  • TALK: Space weather prediction through the observation and modeling of coronal magnetism, Gibson et al.

  • TALK: Coronal magnetometry, Gibson et al.


     2017: Into the Red Dragon's Lair (Cardiff) 
    

  • TALK:  Space weather prediction through the observation and modeling of coronal magnetism, Gibson et al.


     2017: Into the Red Dragon's Lair (Cardiff) 
    

  • TALK: Designing a new coronal magnetic field energy diagnostic to enhance space weather predictions, Corchado Albelo et al.


     2017: AGU Fall meeting (New Orleans)
    

  • POSTER: Numerical MHD coronal simulations: Energy statistics and FORWARD analysis, Nimmo et al.


     2018: NSO Solar Focus talk (Boulder)
    

  • TALK: MHD simulations of coronal mass ejections and prominence eruptions, Fan


     2018: Modeling And Data Analysis Working Group meeting (Toulouse)
    

  • TALK: Non-radial magnetic expansion inferred from off-limb coronal polarimetry, Dalmasse et al.


     2018: SPD Triennial Earth Sun Summit (Leesburg)
    

  • POSTER: Nonlinear force free field modeling of an erupting pseudostreamer, Karna et al. 


     2018: ISSI workshop (Bern)
    

  • TALK: MHD simulations of prominence eruptions, Fan


     2018: COSPAR (Pasadena)
    

  • TALK: The eruption of a prominence-carrying coronal flux rope: forward synthesis of the magnetic field strength measurement by the COronal Solar Magnetism Observatory Large Coronagraph. Fan et al.

  • TALK: Linear line polarimetry: probing the magnetic field mechanisms of energy deposition in the corona, Fineschi et al.

  • POSTER: Pseudostreamer Topology Revealed by CoMP Observations, de Toma et al.

  • POSTER: Simulating the solar minimum corona in UV and visible/IR wavelengths with FORWARD modeling, Zhao et al.

     2018: CoolStars20 (Boston)
    

  • POSTER: Nonlinear force free field modeling of a pseudostreamer before and during eruption, Karna et al. 

     2018: Data-driven modeling workshop (Boulder)
    

  • TALK: Model coupling and data driven simulations of solar eruption: Magnetofrictional Modeling of an erupting Pseudostreamer, Karna et al.

     2018: DOCFM Team meeting (St. Andrews)
    

  • TALK: Coronal polarimetry and motivation for the DOCFM project, Gibson

  • TALK: Current status of the DOCFM project, Dalmasse

  • TALK: MHD simulations of CME initiation and prominence eruption, Fan

  • TALK: Pseudostreamer modeling, Karna

  • TALK: Pseudostreamer observations, de Toma 

  • TALK: Data-driven global models: present capability and flux rope studies, Mackay

  • TALK: Topology, twist, and flux rope detection, Savcheva

  • TALK: Local and global models for the Sun's magnetic carpet, Meyer

  • TALK: Modeling the ICME as a magnetic flux rope, Flyer

  • TALK: Coronal inversion via temperature prescription, Mathews

  • TALK: Data-driven NLFFF models of active regions, Yardley

  • TALK: Milestones and next steps, Gibson 

     2018: DOICMEM workshop (Boulder)
    

  • TALK: Radial-basis-function optimization approximation method,Dalmasse

     2018: AGU Fall meeting (Washington DC)
    

  • TALK: Coronal magnetometry, Gibson

  • POSTER: Designing a new coronal magnetic field energy diagnostic to enhance space weather predictions, Corchado Albelo et al.

  • POSTER: Simulating the solar minimum corona in UV and visible/IR wavelengths with FORWARD modeling, Zhao et al.

  • POSTER: Model coupling and data driven simulations of solar eruption: Magnetofrictional Modeling of an erupting Pseudostreamer, Karna et al.

     2018:  PNST (Sete)
    

  • POSTER: Exploitation of solar coronal spectropolarimetry from CoMP and DKIST, Dalmasse et al.

     2019:  Team seminar (Toulouse)
    

  • TALK: Constraining the solar coronal magnetic field using infrared polarimetry, Dalmasse et al.

     2019:  NOAA/SWPC seminar (Boulder)
    

  • TALK: MHD simulations of prominence eruption and CME initiation, Fan et al.

     2019:  IUGG General Assembly (Montreal)
    

  • POSTER: Data-optimized coronal field model, Dalmasse et al.

  • POSTER: Developing Convolutional Neural Networks for Predicting the Strength of Geomagnetic Storms Caused by Interplanetary Coronal Mass Ejections, Flyer et al.

     2019:  SHINE conference (Boulder)
    

  • POSTER: Linear polarization observations of coronal pseudostreamers, de Toma et al.

  • POSTER: MHD simulation of prominence-cavity system and forward modeling of COSMO/LC line-of-sight magnetic field measurement, Fan et al.

     2019:  ISSI-Beijing international team meeting on erupting filaments (Beijing)
    

  • TALK (remote): Simulations of CME initiation with associated prominence eruption, Fan et al.