Comparative Analysis of a Transition Region Bright Point with a Blinker and Coronal Bright Point Using Multiple EIS Emission Lines-Reference-Cited by-同舟云学术

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Comparative Analysis of a Transition Region Bright Point with a Blinker and Coronal Bright Point Using Multiple EIS Emission Lines

Published:2013-11-09 Issue:5 Volume:289 Page:1557-1584
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Orange N. Brice,Oluseyi Hakeem M.,Chesny David L.,Patel Maulik,Hesterly Katie,Preuss Lauren,Neira Chantale,Turner Niescja E.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/s11207-013-0423-4.pdf

Reference95 articles.

1. Abramenko, V., Yurchyshyn, V., Goode, P., Kilcik, A.: 2010, Statistical distribution of size and lifetime of bright points observed with the New Solar Telescope. Astrophys. J. Lett. 725, L101 – L105. doi: 10.1088/2041-8205/725/1/L101 .

2. Arnaud, M., Raymond, J.: 1992, Iron ionization and recombination rates and ionization equilibrium. Astrophys. J. 398, 394 – 406. doi: 10.1086/171864 .

3. Athay, R.G., Gurman, J.B., Henze, W.: 1983, Fluid motions in the solar chromosphere–corona transition region. III – Active region flows from wide slit Dopplergrams. Astrophys. J. 269, 706 – 714. doi: 10.1086/161080 .

4. Athay, R.G., Gurman, J.B., Shine, R.A., Henze, W.: 1982, Fluid motions the solar chromosphere–corona transition region. II – Active region flows in C IV from narrow slit Dopplergrams. Astrophys. J. 261, 684 – 699. doi: 10.1086/160379 .

5. Athay, R.G., Gurman, J.B., Henze, W., Shine, R.A.: 1983, Fluid motions in the solar chromosphere–corona transition region. I – Line widths and Doppler shifts for C IV. Astrophys. J. 265, 519 – 529. doi: 10.1086/160695 .

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