Search Results - "Mcmullen, Ra"

The Topology and Evolution of the Bastille Day Flare by Aulanier, G, DeLuca, E. E, Antiochos, S. K, McMullen, R. A, Golub, L

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The transition region and coronal explorer by Handy, B N, Acton, L W, Kankelborg, C C, Wolfson, C J, Akin, D J, Bruner, ME, Caravalho, R, Catura, R C, Chevalier, R, Duncan, D W, Edwards, C G, Feinstein, C N, Freeland, S L, Friedlaender, F M, Hoffmann, CH, Hurlburt, N E, Jurcevich, B K, Katz, N L, Kelly, G A, Lemen, J R, Levay, M, Lindgren, R W, Mathur, D P, Meyer, S B, Morrison, S J, Morrison, MD, Nightingale, R W, Pope, T P, Rehse, R A, Schrijver, C J, Shine, R A, Shing, L, Strong, K T, Tarbell, T D, Title, A M, Torgerson, D D, Golub, L, Bookbinder, JA, Caldwell, D, Cheimets, P N, Davis, W N, Deluca, EE, McMullen, R A, Warren, H P, Amato, D, Fisher, R, Maldonado, H, Parkinson, C

“…The Transition Region and Coronal Explorer (TRACE) satellite, launched 2 April 1998, is a NASA Small Explorer (SMEX) that images the solar photosphere,…”
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A new view of the solar outer atmosphere by the Transition Region and Coronal Explorer by Schrijver, Cj, Title, Am, Berger, Te, Fletcher, L, Hurlburt, Ne, Nightingale, Rw, Shine, Ra, Tarbell, Td, Wolfson, J, Golub, L, Bookbinder, Ja, Deluca, Ee, Mcmullen, Ra, Warren, Hp, Kankelborg, Cc, Handy, Bn, De Pontieu, B

“…The Transition Region and Coronal Explorer (TRACE) - described in the companion paper by Handy et al. (1999) - provides an unprecedented view of the solar…”
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On the Tilt and Twist of Solar Active Regions by Holder, Zachary A, Canfield, Richard C, McMullen, Rebecca A, Nandy, Dibyendu, Howard, Robert F, Pevtsov, Alexei A

“…Tilt and twist are two measurable characteristics of solar active regions that can give us information about subsurface physical processes associated with the…”
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The Magnetic Structure of a Coronal X-Ray Bright Point by Brown, Ds, Parnell, Ce, Deluca, Ee, Golub, L, Mcmullen, Ra

“…X-ray bright points are small dynamic loop structures that are observed all over the solar corona. The high spatial and temporal resolution of the TRACE…”
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A Case for Resonant Scattering in the Quiet Solar Corona in Extreme-Ultraviolet Lines with High Oscillator Strengths by Schrijver, Carolus J, McMullen, Rebecca A

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Determination of Flare Heating and Cooling Using the Transition Region and Coronal Explorer by Antiochos, S. K, DeLuca, E. E, Golub, L, McMullen, R. A

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Magnetic structure and reconnection of x-ray bright points in the solar corona by Brown, D.S., Parnell, C.E., DeLuca, E.E, McMullen, R.A., Golub, L., Priest, E.R.

“…The three-dimensional magnetic topology of the solar corona is incredibly complex and its effect on the nature of 3D reconnection is profound. We study the…”
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