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

HOP INSTRUCTION PAGE



HOP Proposer:    De Luca

deluca [at] head.cfa.harvard.edu


As Primary Proposer:

HOP 121:

No HOP productivity information provided.

HOP 136:

REFEREED PUBLICATION(s):

Engell et al. 2011, ApJ, 726: doi:10.1088/0004-637X/726/1/12.

Sylwester et al. 2011, Central European Astrophysical Bulletin, 35, 171.

ADDITIONAL COMMENTS:

The loss of the Russian spacecraft limited future collaborative efforts. TESIS had a very short active lifetime.



* As Co-Proposer:

* HOP 122:

No HOP productivity information provided.

* HOP 232:

No HOP productivity information provided.

* HOP 270:

REASON FOR LACK OF PRODUCTIVITY:

No output. Key EIS line Si VII 275.35 doesn't have enough S/N even with 150s exposure in the coronal hole. We are currently analyzing the SOT/NFI data to study the evolution of underlying magnetic field for network jets observed with IRIS. We'll investigate several other datasets as well and aim at a paper discussing the relationship between network jet occurrence and magnetic field evolution.