Questions / Comments: sabrina.savage [at] nasa.gov
HOP INSTRUCTION PAGE
HOP Proposer: De Pontieu
bdp [at] lmsal.com
As Primary Proposer:
HOP 126:
REFEREED PUBLICATION(s):
Tian et al. 2012, ApJ, 759, 144
Okamoto & De Pontieu 2011, ApJL, 736, 24
NON-REFEREED PUBLICATION(s):
Tian, McIntosh, & De Pontieu 2012, ASPC, 456, 97
HOP 159:
REFEREED PUBLICATION(s):
Martinez-Sykora et al. 2013, ApJ, 771, 66
Tian et al. 2012, ApJ, 759, 144
McIntosh et al. 2012, ApJ, 749, 60
Tian et al. 2011, ApJ, 738, 18
NON-REFEREED PUBLICATION(s):
Tian, McIntosh, & De Pontieu 2012, ASPC, 456, 97
Sechler et al. 2012, ASPC, 455, 361
HOP 249:
REFEREED PUBLICATION(s):
Skogsrud et al. 2015, ApJ, 806, 170
Rouppe van der Voort et al. 2015, ApJ, 799, 3
HOP 306:
No HOP productivity information provided.
HOP 307:
No HOP productivity information provided.
* As Co-Proposer:
* HOP 63:
No HOP productivity information provided.
* HOP 200:
No HOP productivity information provided.
* HOP 236:
REFEREED PUBLICATION(s):
"Fan-shaped jets above the light bridge of a sunspot driven by reconnection," Robustini et al, Astronomy & Astrophysics, Volume 590, 2016
"On the Active Region Bright Grains Observed in the Transition Region Imaging Channels of IRIS," Skogrud et al, The Astrophysical Journal, Volume 817, 2016.
"Evidence for a Transition Region Response to Penumbral Microjets in Sunspots," Vissers et al, The Astrophysical Journal Letters, Volume 811, 2015
Vissers et al. 2015, ApJ, 812
Skogsrud et al. 2015, ApJ, 806, 170
Martinez-Sykora et al. 2015, ApJ, 803, 44
Rouppe van der Voort et al. 2015, ApJ, 799, 3
Skogsrud, Rouppe van der Voort, & De Pontieu 2014, ApJ, 795, 23
Hansteen et al. 2014, Science, 346, 1255757
De Pontieu et al. 2014, Science, 346, 1255732
ADDITIONAL COMMENTS:
Duplicate output to HOP 257.
* HOP 247:
No HOP productivity information provided.
* HOP 248:
REFEREED PUBLICATION(s):
K. Reeves, P. I. McCauley, H. Tian, ApJ (2015) 807, 7
Antolin P. et al, 2015, ApJ, 806
ADDITIONAL COMMENTS:
In preparation:
Baba et al. (2016)
Antolin et al. (2016)
Liu, Antolin, Xu et al. (2016)
Duplicate output to HOP 262.
* HOP 254:
No HOP productivity information provided.
* 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
* HOP 257:
REFEREED PUBLICATION(s):
"Fan-shaped jets above the light bridge of a sunspot driven by reconnection," Robustini et al, Astronomy & Astrophysics, Volume 590, 2016
"On the Active Region Bright Grains Observed in the Transition Region Imaging Channels of IRIS," Skogrud et al, The Astrophysical Journal, Volume 817, 2016.
"Evidence for a Transition Region Response to Penumbral Microjets in Sunspots," Vissers et al, The Astrophysical Journal Letters, Volume 811, 2015
Vissers et al. 2015, ApJ, 812
Skogsrud et al. 2015, ApJ, 806, 170
Martinez-Sykora et al. 2015, ApJ, 803, 44
Rouppe van der Voort et al. 2015, ApJ, 799, 3
Skogsrud, Rouppe van der Voort, & De Pontieu 2014, ApJ, 795, 23
Hansteen et al. 2014, Science, 346, 1255757
De Pontieu et al. 2014, Science, 346, 1255732
ADDITIONAL COMMENTS:
See also HOP 236.
* HOP 269:
REASON FOR LACK OF PRODUCTIVITY:
During the first run in 2014-Oct, the IRIS slit missed the prominence bubble, although SOT/BFI captured the bubble within its field of view. Data analysis is currently underway. During the second run in 2015-Feb, the target prominence was missed.
* HOP 294:
No HOP productivity information provided.
* HOP 316:
No HOP productivity information provided.
* HOP 323:
No HOP productivity information provided.