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DOI:10.1088/0004-637X/757/2/168 - Corpus ID: 119197765
@article{Su2012OBSERVATIONSAM, title={OBSERVATIONS AND MAGNETIC FIELD MODELING OF A SOLAR POLAR CROWN PROMINENCE}, author={Yingna Su and Adriaan van Ballegooijen}, journal={The Astrophysical Journal}, year={2012}, volume={757}, url={https://api.semanticscholar.org/CorpusID:119197765}}- Yingna Su, A. van Ballegooijen
- Published 7 August 2012
- Physics, Environmental Science
- The Astrophysical Journal
We present observations and magnetic field modeling of the large polar crown prominence that erupted on 2010 December 6. Combination of Solar Dynamics Observatory (SDO)/Atmospheric Imaging Assembly (AIA) and STEREO_Behind/EUVI allows us to see the fine structures of this prominence both at the limb and on the disk. We focus on the structures and dynamics of this prominence before the eruption. This prominence contains two parts: an active region part containing mainly horizontal threads and a…
73 Citations
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73 Citations
- Yingna SuA. A. BallegooijenP. McCauleyH. JiK. ReevesE. DeLuca
- 2015
Physics
We present an investigation of the polar crown prominence that erupted on 2012 March 12. This prominence is observed at the southeast limb by the Solar Dynamics Observatory (SDO)/Atmospheric Imaging…
- 54 [PDF]
- N. PanesarD. InnesD. SchmitS. Tiwari
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Physics, Environmental Science
Polar crown prominences, that partially circle the Sun’s poles between 60° and 70° latitude, are made of chromospheric plasma. We aim to diagnose the 3D dynamics of a polar crown prominence using…
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- N. PanesarD. InnesD. SchmitS. K. Tiwari
- 2014
Physics, Environmental Science
Solar Physics
Polar crown prominences, that partially circle the Sun’s poles between 60° and 70° latitude, are made of chromospheric plasma. We aim to diagnose the 3D dynamics of a polar crown prominence using…
- PDF
- S. GunárP. SchwartzJ. DudíkB. SchmiederP. HeinzelJ. Jurčák
- 2014
Physics
Aims. The aim of this work is to analyse the multi-instrument observations of the June 22, 2010 prominence to study its structure in detail, including the prominence-corona transition region and the…
- 32
- PDF
- Yingna SuA. van Ballegooijen
- 2013
Physics
A large polar-crown prominence composed of different segments spanning nearly the entire solar disk erupted on 2010 December 6. Prior to the eruption, the filament in the active region part split…
- 25 [PDF]
- P. JibbenK. ReevesYingna Su
- 2016
Physics
Front. Astron. Space Sci.
Coronal cavities are regions of low coronal emission that usually sit above solar prominences. These systems can exist for days or months before erupting. The magnetic structure of the…
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- PDF
- D. MackayB. SchmiederA. AristeY. Su
- 2020
Physics, Environmental Science
Context. Direct magnetic field measurements in solar prominences occur infrequently and are difficult to make and interpret. As a consequence, alternative methods are needed to derive the main…
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- Andrew HillierA. van Ballegooijen
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Physics
The dense prominence material is believed to be supported against gravity through the magnetic tension of dipped coronal magnetic field. For quiescent prominences, which exhibit many gravity-driven…
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- J. DudíkG. AulanierB. SchmiederM. ZapiórP. Heinzel
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Physics
We study a polar-crown prominence with a bubble and its plume observed in several coronal filters by the SDO/AIA and in Hα by the MSDP spectrograph in Białków (Poland) to address the following…
- 54
- PDF
- Yajie ChenH. Tian Yu Liang
- 2018
Physics, Environmental Science
We present an investigation of a coronal cavity observed above the western limb in the coronal red line Fe x 6374 Å using a telescope of Peking University and in the green line Fe xiv 5303 Å using a…
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