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The High-resolution coronal imager (Hi-C)

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The High-resolution coronal imager (Hi-C). / Kobayashi, Ken; Cirtain, Jonathan; Winebarger, Amy R. et al.
In: Solar Physics, Vol. 289, No. 11, 25.07.2014, p. 4393-4412.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

Kobayashi, K, Cirtain, J, Winebarger, AR, Korreck, K, Golub, L, Walsh, RW, De Pontieu, B, DeForest, C, Title, A, Kuzin, S, Savage, S, Beabout, D, Beabout, B, Podgorski, W, Caldwell, D, McCracken, K, Ordway, M, Bergner, H, Gates, R, McKillop, S, Cheimets, P, Platt, S, Mitchell, N & Windt, D 2014, 'The High-resolution coronal imager (Hi-C)', Solar Physics, vol. 289, no. 11, pp. 4393-4412. https://doi.org/10.1007/s11207-014-0544-4

APA

Kobayashi, K., Cirtain, J., Winebarger, A. R., Korreck, K., Golub, L., Walsh, R. W., De Pontieu, B., DeForest, C., Title, A., Kuzin, S., Savage, S., Beabout, D., Beabout, B., Podgorski, W., Caldwell, D., McCracken, K., Ordway, M., Bergner, H., Gates, R., ... Windt, D. (2014). The High-resolution coronal imager (Hi-C). Solar Physics, 289(11), 4393-4412. https://doi.org/10.1007/s11207-014-0544-4

Vancouver

Kobayashi K, Cirtain J, Winebarger AR, Korreck K, Golub L, Walsh RW et al. The High-resolution coronal imager (Hi-C). Solar Physics. 2014 Jul 25;289(11):4393-4412. doi: 10.1007/s11207-014-0544-4

Author

Kobayashi, Ken ; Cirtain, Jonathan ; Winebarger, Amy R. et al. / The High-resolution coronal imager (Hi-C). In: Solar Physics. 2014 ; Vol. 289, No. 11. pp. 4393-4412.

Bibtex

@article{535d05225f6d47e18cfffc63b621f68c,
title = "The High-resolution coronal imager (Hi-C)",
abstract = "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 (≈0.3 – 0.4˝), high-cadence (≈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 4096×4096 camera with a plate scale of 0.1˝ 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.",
author = "Ken Kobayashi and Jonathan Cirtain and Winebarger, {Amy R.} and Kelly Korreck and Leon Golub and Walsh, {Robert W.} and {De Pontieu}, Bart and Craig DeForest and Alan Title and Sergey Kuzin and Sabrina Savage and Dyana Beabout and Brent Beabout and William Podgorski and David Caldwell and Kenneth McCracken and Mark Ordway and Henry Bergner and Richard Gates and Sean McKillop and Peter Cheimets and Simon Platt and Nick Mitchell and David Windt",
year = "2014",
month = jul,
day = "25",
doi = "10.1007/s11207-014-0544-4",
language = "English",
volume = "289",
pages = "4393--4412",
journal = "Solar Physics",
issn = "0038-0938",
publisher = "Springer Netherlands",
number = "11",

}

RIS

TY - JOUR

T1 - The High-resolution coronal imager (Hi-C)

AU - Kobayashi, Ken

AU - Cirtain, Jonathan

AU - Winebarger, Amy R.

AU - Korreck, Kelly

AU - Golub, Leon

AU - Walsh, Robert W.

AU - De Pontieu, Bart

AU - DeForest, Craig

AU - Title, Alan

AU - Kuzin, Sergey

AU - Savage, Sabrina

AU - Beabout, Dyana

AU - Beabout, Brent

AU - Podgorski, William

AU - Caldwell, David

AU - McCracken, Kenneth

AU - Ordway, Mark

AU - Bergner, Henry

AU - Gates, Richard

AU - McKillop, Sean

AU - Cheimets, Peter

AU - Platt, Simon

AU - Mitchell, Nick

AU - Windt, David

PY - 2014/7/25

Y1 - 2014/7/25

N2 - 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 (≈0.3 – 0.4˝), high-cadence (≈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 4096×4096 camera with a plate scale of 0.1˝ 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.

AB - 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 (≈0.3 – 0.4˝), high-cadence (≈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 4096×4096 camera with a plate scale of 0.1˝ 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.

U2 - 10.1007/s11207-014-0544-4

DO - 10.1007/s11207-014-0544-4

M3 - Journal article

AN - SCOPUS:85027922312

VL - 289

SP - 4393

EP - 4412

JO - Solar Physics

JF - Solar Physics

SN - 0038-0938

IS - 11

ER -