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

HOP INSTRUCTION PAGE



HOP Proposer:    Grigis

Current email address needed


As Primary Proposer:

HOP 91:

REASON FOR LACK OF PRODUCTIVITY:

Proposer left the field (Grigis).



* As Co-Proposer:

* HOP 97:

REFEREED PUBLICATION(s):

Otsuji et al. 2011, PASJ, 63, 1047.

ADDITIONAL COMMENTS:

One run captured the initial phase of the EFR development in the quiet Sun.The proposers have not yet published the data because two of them (Grigis, Kamio) left from solar physics. However, I [Shimizu] encouraged Otsuji to use the data including the emerging flux successfully captured by HOP97 for his emerging flux studies.