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

HOP INSTRUCTION PAGE



HOP Proposer:    Landi

elandi [at] umich.edu


As Primary Proposer:

HOP 39:

No HOP productivity information provided.

HOP 107:

No HOP productivity information provided.

HOP 238:

OTHER PRODUCT(s):

Pasachoff, Jay M.; Dantowitz, Ronald; Voulgaris, Aristeidis 2016, American Astronomical Society, AAS Meeting #227, id.125.02, "Structure, Dynamics, and Spectra of the Solar Corona at the 2013 and 2015 Total Eclipses and Plans for 2017's American Totality"

HOP 298:

No HOP productivity information provided.



* As Co-Proposer:

* HOP 162:

No HOP productivity information provided.

* HOP 201:

No HOP productivity information provided.

* HOP 214:

REASON FOR LACK OF PRODUCTIVITY:

Calibration HOP

* HOP 224:

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.

* HOP 278:

No HOP productivity information provided.