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5.
| Conf. Talk Image Acquisition
/ Rachmeler, L. A.
Talk presented at ASPIICS SWT 2 on 2015-03-xx
[SIDCimport-1549]
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6.
| Science Article Modeling Eruptive Coronal Magnetohydrodynamic Systems with FLUX
/ Rachmeler, L. A.
published in American Astronomical Society, AAS Meeting #216, #306.02; Bulletin of the American Astronomical Society (2010)
[SIDCimport-1476]
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7.
| Conf. Poster Creating synthetic coronal observational data from MHD models: the forward technique
/ Rachmeler, L. A. ; Gibson, S.E. ; et al
Poster presented at American Geophysical Union, Fall Meeting 2010, abstract #SH31A-1786 on 2010-xx-xx
[SIDCimport-1475]
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8.
| Conf. Poster Comparing Global Coronal Models to CoMP Data
/ Rachmeler, L. A. ; Gibson, S.E. ; et al
Poster presented at American Geophysical Union, Fall Meeting 2011, abstract #SH43B-1941 on 2011-xx-xx
[SIDCimport-1474]
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9.
| Conf. Poster Cavity magnetic observations: A survey using AIA and CoMP data
/ Forland, B. ; Rachmeler, L. A. ; et al
Poster presented at American Geophysical Union, Fall Meeting 2011, abstract #SH43B-1951 on 2011-xx-xx
[SIDCimport-1473]
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10.
| Science Article Recent Results from the Coronal Multi-Channel Polarimeter
/ Tomczyk, S. ; Bethge, C. ; Gibson, S.E. ; McIntosh, P.S. ; et al
published in American Astronomical Society, AAS Meeting #220, #310.01 (2012)
[SIDCimport-1472]
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11.
| Science Article Interpreting Coronal Polarization Observations
/ Rachmeler, L. A. ; Casini, R. ; Gibson, S.E.
published in The Second ATST-EAST Meeting: Magnetic Fields from the Photosphere to the Corona. ASP Conference Proceedings (2012)
[SIDCimport-1471]
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12.
| Conf. Talk Lessons Learned in Five Years of Observations with the EUV Solar Telescope SWAP onboard PROBA2
/ Seaton, D.B. ; Berghmans, D. ; et al
Talk presented at Measurement Techniques in Solar and Space Physics, NCAR, Boulder, Colorado, USA on 2015-04-xx
[SIDCimport-1293]
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13.
| Dataset FORWARD: Forward modeling of coronal observables
/ Gibson, S.E. ; Kucera, T.A. ; et al
[SIDCimport-1240]
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14.
| Conf. Talk PROBA2/SWAP EUV images of the large-scale EUV corona up to 3 solar radii: Can we close the gap in coronal magnetic field structure between 1.3 and 2.5 solar radii?
/ De Groof, A. ; Seaton, D.B. ; et al
Talk presented at Joint American Astronomical Society/American Geophysical Union Triennial Earth-Sun Summit, meeting #1, #409.01 on 2015-xx-xx
[SIDCimport-1199]
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