Questions / Comments: sabrina.savage [at] nasa.gov

HOP INSTRUCTION PAGE



HOP 73, TOO, CORE

CORE Too: Quiescent Prominence Structure and Dynamics

Number of runs (8/24/15):    17

Dates:    Sep-08; Oct-08; Apr-09; May-09; Apr-10; Jun-10

Primary Proposer(s):

Berger -- tberger [at] nso.edu

Co-proposer(s):

Y. Lin -- current email address needed


HOP Productivity:

REFEREED PUBLICATION(s):

Dudik et al. 2013

Hillier, A. et al. 2012, ApJ, 746, 120.

Hillier, A. et al. 2012, ApJ, 756, 110.

Hillier, A. et al. 2012, ApJ, 761, 106.

Berger, T. 2012, "The Prominence/Coronal Cavity System", PASP, 463, 147.

Berger, T. 2012, "Solar Promience fine structure and dynamics", IAUS 300 Proceedings, 15.

Berlicki et al. 2012.

Labrosse et al. 2012.

Parenti et al. 2012.

Hillier, A. et al. 2011, ApJ, 736, L1.

Hillier, A. et al. 2011, PASJ, 63, L19.

Berger, T. et al. 2011, Nature, 472, 197.

Berger, T. et al. 2010, ApJ, 716, 1288.

Schmieder et al. 2010.

Berger, T. et al. 2008, ApJ, 676, L89.

Heinzel et al. 2008.

EPO:

Berger, T., "Our Explosive Sun", public outreach lecture given at numerous events incl. AAS/SPD Bozeman, 2013.

OTHER OUTPUT(s):

Berger, T. et al., ApJ follow-on to 2010 paper

Hillier, A. et al., review paper on magnetic Rayleigh-Taylor instability in solar prominences.

ADDITIONAL COMMENTS:

Gunar et al. and Schwartz et al. provided by Schmieder without year.