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.

    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.