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

HOP INSTRUCTION PAGE



HOP Proposer:    Orozco Suarez

dorozco [at] iac.es


As Primary Proposer:

HOP 213:

No HOP productivity information provided.

HOP 258:

No HOP productivity information provided.



* As Co-Proposer:

* HOP 151:

REFEREED PUBLICATION(s):

del Moro et al. 2015, A&A, 576, A47, 6

Gosic et al. 2014, ApJ, 797, 49

Giannattasio et al. 2014, A&A, 569, A121

Giannattasio et al. 2014, ApJ, 788, L37

Giannattasio et al. 2013, ApJ, 770, L36.

Orozco-Suarez, Katsukawa, & Bellot Rubio 2012, ApJ, 758, L38

EPO:

PhD Thesis of Milan Gosic, University of Granada (Spain), to be defended Dec 2015.

Giannattasio, F., University di Tor Vergata, Italy, 2014

Master Thesis of Milan Gosic, University of Granada (Spain), 2012.

ADDITIONAL COMMENTS:

Gosic et al., ApJ, under review "The solar internetwork. II. Flux appearance and disappearance rates"

This HOP has been very successful, except for the fact that we were unable to complete the planned 40 hours of continuous monitoring of the quiet Sun. HOP 151 gathered a unique dataset in terms of sensitivity, duration and cadence. It remains unique, since no similar observations have been performed so far.