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

HOP INSTRUCTION PAGE



HOP Proposer:    Malherbe

jean-marie.malherbe [at] obspm.fr


As Primary Proposer:

HOP 95:

No HOP productivity information provided.

HOP 210:

No HOP productivity information provided.



* As Co-Proposer:

* HOP 21:

No HOP productivity information provided.

* HOP 167:

REFEREED PUBLICATION(s):

Roudier et al. 2009, A&A, 495, 945.

Roudier et al. 2009, ASPC, 415, 203.

ADDITIONAL COMMENTS:

During the last year we analysed the sequence 29 30 31 August 2007. We showed the importance of the families to built the quiet magnetic network via the horizontal flows that they generate. A paper will be submited in the next 3 monthes and its drafting is well advanced. Lot of movies have been also done and will be put on a web page soon.

* HOP 217:

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.

* HOP 295:

REFEREED PUBLICATION(s):

Roudier, T., Malherbe, J.~M., Rieutord, M., Frank, Z.: 2016, ÒRelation between trees of fragmenting granules and supergranulation evolutionÓ 2016, A&A, Volume 590, id.A121

Malherbe, J.-M., Roudier, T., Frank, Z., and Rieutord, M.: 2015, "Families of Granules, Flows, and Acoustic Events in the Solar Atmosphere from Hinode Observations," Solar Physics 290, 321

* HOP 312:

No HOP productivity information provided.