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

HOP INSTRUCTION PAGE



HOP 217, TOO

Determination of the properties of families of solar granules and formation of the photospheric network

Number of runs (8/24/15):    2

Dates:    ToO: Apr-13; May-13

Primary Proposer(s):

Roudier -- troudier [at] irap.omp.eu

Co-proposer(s):

Rieutord -- current email address needed
Meunier -- current email address needed
Malherbe -- jean-marie.malherbe [at] obspm.fr
Molodij -- current email address needed


HOP Productivity:

No productivity information provided.


REASON FOR LACK OF PRODUCTIVITY:

Several observations have done for that HOP 217. That was due to the non continuity of the observation with a regular time step around 45 to 60s. The best sequence has been obtained between 28-29 april 2013 with a duration of 23h58mn at the disc center. The data are calibrated in intensity and the reduced (aligned, k-omega filtered and Families of granule detection. That data are still understudy. We are preparing a paper where we compare the properties of families and photospheric network between 2007 and 2013. We think that results will be published in 2016.