Questions / Comments: sabrina.savage [at] nasa.gov
HOP INSTRUCTION PAGE
HOP Proposer: Young
pyoung9 [at] gmu.edu
As Primary Proposer:
HOP 58:
No HOP productivity information provided.
HOP 59:
No HOP productivity information provided.
HOP 177:
REFEREED PUBLICATION(s):
Young, P. R., 2015, ApJ 801, 124
Young & Muglach 2014a, Solar Phys., 289, 3313.
NON-REFEREED PUBLICATION(s):
Young & Muglach 2014b, PASJ special issue (Proc. of 7th Hinode Science Meeting)
HOP 266:
No HOP productivity information provided.
HOP 267:
No HOP productivity information provided.
HOP 268:
No HOP productivity information provided.
* As Co-Proposer:
* HOP 154:
No HOP productivity information provided.
* HOP 162:
No HOP productivity information provided.
* HOP 232:
No HOP productivity information provided.
* HOP 241:
REASON FOR LACK OF PRODUCTIVITY:
The IRIS portions of IHOP 241 observations of an M7 flare
in AR 12036 on 2014 April 18 in ApJ 810, 45 (J. W. Brosius and A. N. Daw, 2015). The paper is called "Quasi-Periodic Fluctuations and
Chromospheric Evaporation in a Solar Flare Ribbon Observed by
IRIS." We have coordinated EIS observations of the same event,
which I have talked about at two flare meetings at Goddard and at
the IRIS Workshop in Boulder last May. I am planning to write up
the EIS observations (which also show quasi-periodic fluctuations)
of this flare over the next few months (with A. N. Daw and A. Inglis).
* HOP 247:
No HOP productivity information provided.
* HOP 306:
No HOP productivity information provided.
* HOP 316:
No HOP productivity information provided.