Elementary Loop Structures in the Solar Corona Analyzed from TRACE Triple-Filter Images
By Markus J. Aschwanden, R. Nightingale. 2005
136 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/dbb4539bc4dc3ab8d4f606c216048b2c705a79cb
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
- Fabio Reale
- J. Klimchuk
- Markus J. Aschwanden
- C. Schrijver
- G. D. Zanna
- Tongjiang Wang
- T. Van Doorsselaere
- S. Solanki
In Molecular Biology
- Fabio Reale
- C. Schrijver
- J. Klimchuk
- Markus J. Aschwanden
- G. D. Zanna
- J. Laming
- Monica G. Bobra
- S. Couvidat
Citations in the corpus
- A SYSTEMATIC SURVEY OF HIGH-TEMPERATURE EMISSION IN SOLAR ACTIVE REGIONS (2012, background): “Coronal loops observed at temperatures near 1 MK, for example, often have very narrow temperature distributions (Aschwanden & Nightingale 2005; Tripathi et al. 2009; Warren et al. 2008) and are evolving (e.g., Winebarger et al. 2003; Ugarte-Urra et al. 2009; Tripathi et al. 2010; Mulu-Moore et al.…”
- On Solving the Coronal Heating Problem (2005, background): “…the case has been actively debated (e.g., Nitta, 2000; Schmelz et al., 2001; Schmelz, 2002; DelZanna and Mason, 2003; Nagata et al., 2003; Landi and Landini, 2004; Schmieder et al., 2004; Aschwanden and Nightingale, 2005; Aschwanden, 2005; Reale and Ciaravella, 2005; Schmelz and Martens, 2005).”
- CORONAL LOOP OSCILLATIONS OBSERVED WITH ATMOSPHERIC IMAGING ASSEMBLY—KINK MODE WITH CROSS-SECTIONAL AND DENSITY OSCILLATIONS (2011, methodology): “…side), which corresponds to a near-isothermal temperature distribution at the limit of the temperature resolution Δ log(T ) ≈ 0.3 of the AIA filters, similar to that found for a statistical set of other loops analyzed from TRACE (Aschwanden & Nightingale 2005) or AIA (Aschwanden & Boerner 2011).”
- Coronal Loops: Observations and Modeling of Confined Plasma (2010, background): “These loops would be much less visible in the X-rays and thus would not be cospatial with hot loops, and would also be much less multithermal (Di Giorgio et al., 2003; Landi and Landini, 2004; Aschwanden and Nightingale, 2005; Noglik et al., 2008); iii) warm loops might be globally cooling from a st”