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

HOP INSTRUCTION PAGE



HOP Proposer:    Curdt

Current email address needed


As Primary Proposer:



* As Co-Proposer:

* HOP 43:

No HOP productivity information provided.

* HOP 104:

No HOP productivity information provided.

* HOP 105:

No HOP productivity information provided.

* HOP 106:

No HOP productivity information provided.

* HOP 110:

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.