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

HOP INSTRUCTION PAGE



HOP Proposer:    Tarbell

tarbell [at] lmsal.com


As Primary Proposer:

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 243:

No HOP productivity information provided.

HOP 251:

REFEREED PUBLICATION(s):

Kleint, L., Battaglia, M., Reardon, K., Sainz Dalda, A., Young, P.R., Krucker, S., "THE FAST FILAMENT ERUPTION LEADING TO THE X-FLARE ON 2014 MARCH 29", 2015, ApJ 806, 9

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 323:

No HOP productivity information provided.



* As Co-Proposer:

* HOP 100:

REASON FOR LACK OF PRODUCTIVITY:

(Engineering Test) The one run of this HOP listed on the HOP pages did not actually run the SOT programs requested in the HOP proposal, nor was the target appropriate. So no good data was collected.

* HOP 249:

REFEREED PUBLICATION(s):

Skogsrud et al. 2015, ApJ, 806, 170

Rouppe van der Voort et al. 2015, ApJ, 799, 3

* HOP 250:

OTHER OUTPUT(s):

Y. Katsukawa et al. "Study of High-Speed Flows Associated with Chromospheric Transients around a Sunspot", poster presentation in LWS/Hinode/IRIS workshop

Y. Katsukawa et al. "IRIS observation of penumbral microjets in the chromosphere and their transition region counterpart", oral presentation in the IRIS-4 workshop

* HOP 252:

No HOP productivity information provided.

* 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 270:

REASON FOR LACK OF PRODUCTIVITY:

No output. Key EIS line Si VII 275.35 doesn't have enough S/N even with 150s exposure in the coronal hole. We are currently analyzing the SOT/NFI data to study the evolution of underlying magnetic field for network jets observed with IRIS. We'll investigate several other datasets as well and aim at a paper discussing the relationship between network jet occurrence and magnetic field evolution.

* HOP 306:

No HOP productivity information provided.

* HOP 307:

No HOP productivity information provided.