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

HOP INSTRUCTION PAGE



HOP 270

Generation and heating of Network Jets

Number of runs (8/24/15):    1

Dates:    Sep-14

Primary Proposer(s):

Tian -- hui.tian [at] cfa.harvard.edu

Co-proposer(s):

Landi -- elandi [at] umich.edu
De Luca -- deluca [at] head.cfa.harvard.edu
Tarbell -- tarbell [at] lmsal.com
Curdt -- current email address needed


HOP Productivity:

No productivity information provided.


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.