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

HOP INSTRUCTION PAGE



HOP Proposer:    Doyle

jgd [at] star.arm.ac.uk


As Primary Proposer:

HOP 19:

No HOP productivity information provided.

HOP 32:

No HOP productivity information provided.

HOP 33:

No HOP productivity information provided.

HOP 99:

No HOP productivity information provided.

HOP 112:

No HOP productivity information provided.

HOP 113:

No HOP productivity information provided.

HOP 174:

REFEREED PUBLICATION(s):

Long et al. 2013, Solar Phys., 288, 567.

Harra et al. 2011, ApJ, 737, L4.

Veronig et al. 2011, ApJ, 743, L10.

HOP 215:

No HOP productivity information provided.



* As Co-Proposer:

* HOP 93:

REFEREED PUBLICATION(s):

Banarjee et al. 2012, A&A, 548, 62.

Subramanian 2010, A&A, 516, 50.

Perez-Suarez et al. 2008, A&A, 492, 575.

Innes et al. 2008, Solar Phys., 252, 283.

* HOP 94:

REFEREED PUBLICATION(s):

Subramanian et al. 2012, A&A, 538, 50.

EPO:

Perez-Suarez 2011, PhD Thesis, "Multi-layer Analysis of a Coronal bright Point"

Subramanian 2011, PhD Thesis, "Small Scale EUV and X-ray Transient Brightenings in the Solar Atmosphere"

* HOP 144:

REFEREED PUBLICATION(s):

Madjarska et al. 2011, A&A, 532, 1.

EPO:

Vanninathan 2013, PhD Thesis, "The role of chromospheric jet-like events in coupling the chromosphere and corona: A multi-instrument approach"

* HOP 156:

No HOP productivity information provided.

* HOP 228:

REFEREED PUBLICATION(s):

Huang et al. 2012, A&A, 548, 62.

Madjarska et al. 2012, A&A, 545, 67.


EPO:

Huang 2013, PhD Thesis, "Evolution of Bright Points, X-ray jets, their physical parameters and magnetic field in and around Coronal Holes"