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

HOP INSTRUCTION PAGE



HOP Proposer:    Schmieder

brigitte.schmieder [at] obspm.fr


As Primary Proposer:

HOP 4:

No HOP productivity information provided.

HOP 111:

REASON FOR LACK OF PRODUCTIVITY:

QS conditions made it difficult to obtain the targets. Still working on the data.

HOP 132:

REFEREED PUBLICATION(s):

Mandrini et al. 2014, Solar Phys., 289, 2041.

Schmieder et al. 2014, A&A, 564, 104.

Schmieder et al. 2013, A&A, 559, 1.

Guo et al. 2013, A&A, 555, 19.

Guo et al. 2010, ApJ, 714, 343.



* As Co-Proposer:

* HOP 255:

REFEREED PUBLICATION(s):

B. Schmieder B, Kucera, T.A, Knizhnik,K, Luna, M., Lopez-Ariste, A. and Toot, D Propagating Waves Transverse to the Magnetic Field in a Solar Prominence_, 2013, ApJ., 777,108

Schmieder B., Tian H., Kucera T., Mein P., Lopez-Ariste A., Mein N., Dalmasse K. Dynamics of a prominence observed in Mg II lines by the IRIS spectrograph_, 2014, A and A, 569, A85

Levens,P, Labrosse, N., Fletcher, L., Schmieder,B.A solar tornado : plasma Diagnostics from IRIS and Hinode, 2015, A&A, in press

NON-REFEREED PUBLICATION(s):

Lopez Ariste 2015, IAU S305 (Ed Nagendra, Bagnulo, Centeno, Martinez Gonzalez), page 207, Pattern recognition techniques in Polarimetry

Schmieder et al 2015, IAU S305 (Ed Nagendra, Bagnulo, Centeno, Martinez Gonzalez), page 275, Polarimetry in tornadoes and prominences with THEMIS

OTHER PRODUCT(s):

2014 Oct.: ESPM Dublin : talk de Levens

2015 January talk of P.Levens at RAS, Londres

2015 May Meeting IRIS at Boulder : talk of P.Levens

2015 Sept. Meeting Hinode6 Belfast : talk on EIS of P.Levens

ADDITIONAL COMMENTS:

Levens, P. , Schmieder, B., Labrosse N., Lopez Ariste A. Structure of prominences legs: Plasma and magnetic field, ApJ, submitted