The High-Resolution Coronal Imager (Hi-C)

被引:106
|
作者
Kobayashi, Ken [1 ,2 ]
Cirtain, Jonathan [2 ]
Winebarger, Amy R. [2 ]
Korreck, Kelly [3 ]
Golub, Leon [3 ]
Walsh, Robert W. [4 ]
De Pontieu, Bart [5 ]
DeForest, Craig [6 ]
Title, Alan [5 ]
Kuzin, Sergey [7 ]
Savage, Sabrina [2 ]
Beabout, Dyana [2 ]
Beabout, Brent [2 ]
Podgorski, William [3 ]
Caldwell, David [3 ]
McCracken, Kenneth [3 ]
Ordway, Mark [3 ]
Bergner, Henry [3 ]
Gates, Richard [3 ]
McKillop, Sean [3 ]
Cheimets, Peter [3 ]
Platt, Simon [4 ]
Mitchell, Nick [4 ]
Windt, David [8 ]
机构
[1] Univ Alabama, Ctr Space Plasma & Aeron Res, Huntsville, AL 35805 USA
[2] NASA, George C Marshall Space Flight Ctr, Huntsville, AL 35812 USA
[3] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[4] Univ Cent Lancashire, Preston PR1 2HE, Lancs, England
[5] Lockheed Martin Solar & Astrophys Lab, Palo Alto, CA 94304 USA
[6] Southwest Res Inst, Boulder, CO 80302 USA
[7] Russian Acad Sci, PN Lebedev Phys Inst, Moscow 119991, Russia
[8] Reflect Xray Opt LLC, New York, NY 10027 USA
关键词
Solar corona; Solar instrumentation; Solar imaging; Extreme ultraviolet; SOLAR CORONA; REGION; LOOPS; DYNAMICS; MOSS; RECONNECTION; HINODE; SKYLAB; ENERGY; SCALE;
D O I
10.1007/s11207-014-0544-4
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The High-Resolution Coronal Imager (Hi-C) was flown on a NASA sounding rocket on 11 July 2012. The goal of the Hi-C mission was to obtain high-resolution (a parts per thousand aEuro parts per thousand 0.3 -aEuro parts per thousand 0.4''), high-cadence (a parts per thousand aEuro parts per thousand 5 seconds) images of a solar active region to investigate the dynamics of solar coronal structures at small spatial scales. The instrument consists of a normal-incidence telescope with the optics coated with multilayers to reflect a narrow wavelength range around 19.3 nm (including the Fe xii 19.5-nm spectral line) and a 4096x4096 camera with a plate scale of 0.1''aEuro parts per thousand pixel(-1). The target of the Hi-C rocket flight was Active Region 11520. Hi-C obtained 37 full-frame images and 86 partial-frame images during the rocket flight. Analysis of the Hi-C data indicates the corona is structured on scales smaller than currently resolved by existing satellite missions.
引用
收藏
页码:4393 / 4412
页数:20
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