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Open questions on prominences from coordinated observations by IRIS, Hinode, SDO/AIA, THEMIS, and the Meudon/MSDP
DOI: 10.1051/0004-6361/201423922 Bibcode: 2014A&A...569A..85S

Golub, L.; Schmieder, B.; Tian, H. +5 more

Context. A large prominence was observed by multiple instruments on the ground and in space during an international campaign on September 24, 2013, for three hours (12:12 UT -15:12 UT). Instruments used in the campaign included the newly launched (June 2013) Interface Region Imaging Spectrograph (IRIS), THEMIS (Tenerife), the Hinode Solar Optical …

2014 Astronomy and Astrophysics
Hinode IRIS 72
On the formation of Mg ii h and k lines in solar prominences
DOI: 10.1051/0004-6361/201322886 Bibcode: 2014A&A...564A.132H

Heinzel, P.; Vial, J. -C.; Anzer, U.


Aims: With the recent launch of the IRIS mission, it has become urgent to develop the spectral diagnostics using the Mg ii resonance h and k lines. In this paper, we aim to demonstrate the behavior of these lines under various prominence conditions. Our results serve as a basis for analysis of new IRIS data and for more sophisticated prominen…

2014 Astronomy and Astrophysics
IRIS 59
Conversion from mutual helicity to self-helicity observed with IRIS
DOI: 10.1051/0004-6361/201424377 Bibcode: 2014A&A...570A..93L

Peter, H.; Zhang, J.; Li, L. P. +1 more

Context. In the upper atmosphere of the Sun observations show convincing evidence for crossing and twisted structures, which are interpreted as mutual helicity and self-helicity.
Aims: We use observations with the new Interface Region Imaging Spectrograph (IRIS) to show the conversion of mutual helicity into self-helicity in coronal structure…

2014 Astronomy and Astrophysics
IRIS 35
Molecular absorption in transition region spectral lines
DOI: 10.1051/0004-6361/201424432 Bibcode: 2014A&A...569L...7S

Peter, H.; Curdt, W.; Innes, D. +3 more


Aims: We present observations from the Interface Region Imaging Spectrograph (IRIS) of absorption features from a multitude of cool atomic and molecular lines within the profiles of Si IV transition region lines. Many of these spectral lines have not previously been detected in solar spectra.
Methods: We examined spectra taken from deep …

2014 Astronomy and Astrophysics
IRIS 16