Program

MondayTuesdayWednesdayThursdayFriday
MorningOpening TalksTalksTalksWorking group summariesYellowstone National Park Day Excursion
BreakPostersPostersPostersYellowstone National Park Day Excursion
MorningTalksTalksWorking group 1: Tracking solar features and eruptive events in space, time, and wavelength

Working group 2: Reconstruction of the three-dimensional structure of the corona

Working group 3: Solar information processing techniques

Working group 4: Accessing, browsing, retrieving data
ClosingYellowstone National Park Day Excursion
AfternoonTalksWorking group 1: Tracking solar features and eruptive events in space, time, and wavelength

Working group 2: Reconstruction of the three-dimensional structure of the corona

Working group 3: Solar information processing techniques

Working group 4: Accessing, browsing, retrieving data
Working group 1: Tracking solar features and eruptive events in space, time, and wavelength

Working group 2: Reconstruction of the three-dimensional structure of the corona

Working group 3: Solar information processing techniques

Working group 4: Accessing, browsing, retrieving data
Yellowstone National Park Day Excursion
BreakPostersPostersPostersYellowstone National Park Day Excursion
AfternoonTalksWorking group 1: Tracking solar features and eruptive events in space, time, and wavelength

Working group 2: Reconstruction of the three-dimensional structure of the corona

Working group 3: Solar information processing techniques

Working group 4: Accessing, browsing, retrieving data
Working group 1: Tracking solar features and eruptive events in space, time, and wavelength

Working group 2: Reconstruction of the three-dimensional structure of the corona

Working group 3: Solar information processing techniques

Working group 4: Accessing, browsing, retrieving data
Yellowstone National Park Day Excursion
EveningReceptionDinnerYellowstone National Park Day Excursion

Morning

8:50 – 9:00 am Welcome Address Ireland, J., and Martens, P.
Chair: J. Ireland
Session 1: Instrumentation and solar image processing

9:00 – 9:40 Image Processing and Feature Recognition for High-Resolution Solar Imaging Reardon, K.
9:40 – 10:00 Mainstreaming High-Energy Solar Data Csillaghy, A.
10:20 – 10:40 Identifying Transient Features in the Solar Atmosphere From Multiple Sources Kirk, M.
10:40 – 11:00 Revealing structures and dynamic phenomena on ground-based coronagraph observations via a multi-resolution approach Lopez, F.

11:00 – 11:30 Coffee Break / Poster Session

Chair: Barbara Thompson
Session 2: Reconstruction of three dimensional structure of the solar atmosphere

11:30 – 12:10 3D reconstruction of coronal mass ejections: where are we? Mierla, M.
12:10 – 12:30 Toward Tomographic Reconstruction of CMEs With a Phase Field Method Hewett, R.

Afternoon

12:30 – 2:00 Lunch

Chair: Barbara Thompson
Session 2 (continued): Reconstruction of three dimensional structure of the solar atmosphere

2:00 – 3:00 Vector Tomography for the Coronal Magnetic Field Kramar, M.
2:20 – 2:40 3D reconstruction of CMEs from 3-viewpoints, method comparisons and applications Feng, L.
2:40 – 3:00 CME Reconstruction from Three Viewpoints Via Simulation Morphing Frazin, R.

3:00 – 3:15 Challenges in Solar Image Processing Ireland, J.

3:15 – 3:30 Introduction to Working Group 4 Davey, A. R.

3:30 – 4:00 Coffee Break / Poster Session

Working Groups 4:00 – 5:15 Working Groups parallel sessions

Evening

6 pm Welcome Reception at the Alumni Room in the Strand Union Building on the MSU campus.

Morning

Chair: F. Kamalabadi
Session 3: Solar information and image processing techniques
9:00 – 10:00 Graphical modeling for high dimensional data analysis Hero, A.
10:00 – 10:20 Using DEM Algorithms for Coronal Data Plowman, J.
10:20 – 10:40 Multi-order slitless solar spectroscopy: a Parametric Inversion Approach Oktem, S. F.
10:40 – 11:00 CORIMP: Automatically Detecting & Tracking CMEs in Coronagraph Data Byrne, J.

11:00 – 11:30 Coffee Break / Poster Session

11:30 – 11:50 Detection of small-scale features in the solar photosphere using segmentation algorithms Cabello Garcia, I. B.
11:50 – 12:10 Spatio-Temporal Co-occurrence Pattern Mining in Solar Events Ganesan Pillai, K.

Afternoon

12:10 – 1:30 Lunch

Working Groups 1:30 – 3:30 Working Groups parallel sessions
3:30 – 4:00 Coffee Break / Poster Session
Working Groups 4:00 – 5:15 Working Groups parallel sessions
Demos from WG 4 in Reid Hall Table 1 Table 2
4:00-4:20 Analysis of SDO Data for propagation of waves and other features using a graphical user interface based IDL package by L. Jeska Expanding the Helioviewer Project by J. Ireland
4:20-4:40 SunPy: Python for Solar Physics Data Analysis by V. Hughitt The Virtual Solar Observatory by J. Sattelberger
4:40-5:00 HELIO – All the heliosphere in your hands by D. Perez-Suarez Heliophysics Event Knowledgebase for the Solar Dynamics Observatory and Beyond by R. Timmons

Evening

nothing scheduled

Morning

Chair: A. Csillaghy
Session 3: continued

9:00 – 10:00 Learning with entropic graphs Hero, A.
10:00 – 10:20 Towards the Pseudo-Automatic Characterization of the Morphological and Kinematical Properties of Coronal Mass Ejections using a texture-based Technique Stenborg, G.
10:20 – 10:40 Filament and Sigmoid Statistics Gathered by Newly Developed Automated Feature Finding Modules Martens, P.
10:40 – 11:00 An overview of tools and techniques for parallel computation in solar image processing De Visscher, R.

11:00 – 11:30 Coffee Break / Poster Session

11:30 – 11:50 Principle Component Analysis of the solar background and sunspot magnetic fields in the cycle 21-23. Zharkov, S.
11:50 – 12:10 Poisson noise reduction with non‐local PCA Salmon, J.

Afternoon

12:10 – 1:30 Lunch

Working Groups 1:30 – 3:00 Problem solving sessions – big challenges in Solar Image Processing
3:00 – 3:30 Coffee Break / Poster Session
Working Groups 3:30 – 5:15 Working Groups parallel sessions

Evening

6:00 – 11:00 Conference Dinner at the Emerson Center in downtown Bozeman

Morning
Chair: V. Delouille (9:00 – 11:00), D. Lamb (11.30 – 12:30)
Session 4: Segmentation and tracking of solar features.

9:00 – 9:40 A systematic look at sunspots from space: 1996-2011 Watson, F.
9:40 – 10:00 SWAMIS Emerging Flux Detection and Magnetic Feature Tracking for SDO Lamb, D.
10:00 – 10:20 Image Processing and Pattern Recognition: General Approaches and Application to Solar Data Boucheron, L.
10:20 – 10:40 Spatio-Temporal Evolution Tracking of Solar Flares Aschwanden, M.

10:40 – 11:10 Coffee Break / Poster Session

11:10 – 11:30 Tracking the Elusive Polar Coronal Hole Pesnell, W. D.
11:30 – 11:50 Segmentation of Coronal Holes Using Active Contours and Detection of Small Boundary Flashes Valluri, M.
11:50 – 12:10 Coronal Hole Detection on SDO images Delouille, V.

Afternoon

12:10 – 1:30 Lunch

Working Groups 1:30 – 3:00 Reports from the Working Groups and Closing Remarks

Evening

7:30 – 8:30 (approx) Free celestial-themed jazz concert at the Reynolds Recital Hall on MSU Campus with Jeni Fleming (http://www.montanapbs.org/11thGrantwithEricFunk/episode101/)

  1. Automated and Interactive Image Analysis at NOAA’s Space Weather Prediction Center Hill, S.
  2. Automatic Classification and Tracking of Solar Features Stenning, D.
  3. Evaluating Automated Solar Event Detection Schuh, M.
  4. Dimming and EIT wave detection on SDO/AIA: first results by NEMO Kraaikamp, E.
  5. The Coronal Pulse Identification and Tracking Algorithm (CorPITA) for automated detection of “EIT Waves” Perez-Suarez, D.
  6. Polarity Inversion Line Module Engell, A.
  7. Automatic finding, tracking, and analysing sunspots and white light faculae Gyori, L.
  8. Automated Classification of Flaring  Behavior in Solar Active Regions Al-Ghraibah, A.
  9. Quantitative Heliospheric Imaging: how to separate 99.9% of your data (and have something left) DeForest, C.
  10. On the use of the Dual Tree Complex Wavelet Transform on white light coronal images Stenborg, G.
  11. Analysis of SDO Data for propagation of waves and other features using a graphical user interface based IDL package. Jeska, L.
  12. Applying Computer Vision to SDO/AIA images Felix, S.
  13. Calibration of Hinode/XRT for Coalignment Yoshimura, K.
  14. Polarization Fringe Removal Using Wavelet Analysis Harker, B.
  15. Compressing SDO’s FITS image files, a study from an image-processing perspective Banda, J.
  16. How SDO Changed Solar Physics? Davey, A.
  17. SunPy: Python for Solar Physics Data Analysis Hughitt, V.
  18. Extending the usage of the Helioviewer Project Ireland, J.
  19. HELIO – All the heliosphere in your hands. Perez-Suarez, D.
  20. The Virtual Solar Observatory Sattelberger, J.
  21. Heliophysics Event Knowledgebase for the Solar Dynamics Observatory and Beyond Timmons, R.
  22. Feature Recognition in Heliophysics Integrated Observatory Zharkov, S.