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  The High-Resolution Coronal Imager, Flight 2.1

Rachmeler, L. A., Winebarger, A. R., Savage, S. L., Golub, L., Kobayashi, K., Vigil, G. D., et al. (2019). The High-Resolution Coronal Imager, Flight 2.1. Solar Physics, 294(12): 174. doi:10.1007/s11207-019-1551-2.

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Item Permalink: http://hdl.handle.net/21.11116/0000-0006-68AC-4 Version Permalink: http://hdl.handle.net/21.11116/0000-0006-68AD-3
Genre: Journal Article

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 Creators:
Rachmeler, Laurel A., Author
Winebarger, Amy R., Author
Savage, Sabrina L., Author
Golub, Leon, Author
Kobayashi, Ken, Author
Vigil, Genevieve D., Author
Brooks, David H., Author
Cirtain, Jonathan W., Author
Pontieu, Bart De, Author
McKenzie, David E., Author
Morton, Richard J., Author
Peter, Hardi1, Author              
Testa, Paola, Author
Tiwari, Sanjiv K., Author
Walsh, Robert W., Author
Warren, Harry P., Author
Alexander, Caroline, Author
Ansell, Darren, Author
Beabout, Brent L., Author
Beabout, Dyana L., Author
Bethge, Christian W., AuthorChampey, Patrick R., AuthorCheimets, Peter N., AuthorCooper, Mark A., AuthorCreel, Helen K., AuthorGates, Richard, AuthorGomez, Carlos, AuthorGuillory, Anthony, AuthorHaight, Harlan, AuthorHogue, William D., AuthorHolloway, Todd, AuthorHyde, David W., AuthorKenyon, Richard, AuthorMarshall, Joseph N., AuthorMcCracken, Jeff E., AuthorMcCracken, Kenneth, AuthorMitchell, Karen O., AuthorOrdway, Mark, AuthorOwen, Tim, AuthorRanganathan, Jagan, AuthorRobertson, Bryan A., AuthorPayne, M. Janie, AuthorPodgorski, William, AuthorPryor, Jonathan, AuthorSamra, Jenna, AuthorSloan, Mark D., AuthorSoohoo, Howard A., AuthorSteele, D. Brandon, AuthorThompson, Furman V., AuthorThornton, Gary S., AuthorWatkinson, Benjamin, AuthorWindt, David, Author more..
Affiliations:
1Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289              

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 Abstract: The third flight of the High-Resolution Coronal Imager (Hi-C 2.1) occurred on May 29, 2018; the Sounding Rocket was launched from White Sands Missile Range in New Mexico. The instrument has been modified from its original configuration (Hi-C 1) to observe the solar corona in a passband that peaks near 172 Å, and uses a new, custom-built low-noise camera. The instrument targeted Active Region 12712, and captured 78 images at a cadence of 4.4 s (18:56:22 – 19:01:57 UT; 5 min and 35 s observing time). The image spatial resolution varies due to quasi-periodic motion blur from the rocket; sharp images contain resolved features of at least 0.47 arcsec. There are coordinated observations from multiple ground- and space-based telescopes providing an unprecedented opportunity to observe the mass and energy coupling between the chromosphere and the corona. Details of the instrument and the data set are presented in this paper.

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Language(s): eng - English
 Dates: 2019
 Publication Status: Published in print
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1007/s11207-019-1551-2
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Title: Solar Physics
  Other : Sol. Phys.
Source Genre: Journal
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Publ. Info: Dordrecht, Holland : Kluwer, etc.
Pages: - Volume / Issue: 294 (12) Sequence Number: 174 Start / End Page: - Identifier: ISSN: 0038-0938
CoNE: https://pure.mpg.de/cone/journals/resource/954925445694