A Solar Aspect System for the HEROES Mission

被引:0
作者
Christe, Steven [1 ]
Shih, Albert [1 ]
Rodriguez, Marcello [1 ]
Gregory, Kyle [1 ]
Cramer, Alexander [1 ]
Edgerton, Melissa [1 ]
Gaskin, Jessica [2 ]
O'Connor, Brian [2 ]
Sobey, Alexander [2 ]
机构
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] NASA, George C Marshall Space Flight Ctr, Huntsville, AL 35811 USA
来源
2014 IEEE AEROSPACE CONFERENCE | 2014年
关键词
aspect system; high-altitude balloon; solar; Sun; X-ray; DENSITY-FUNCTION;
D O I
暂无
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
A new Solar Aspect System (SAS) has been developed to provide the ability to observe the Sun on an existing balloon payload HERO (short for High Energy Replicated Optics). Developed under the HEROES program (High Energy Replicated Optics to Explore the Sun), the SAS aspect system provides solar pointing knowledge in pitch, yaw, and roll. The required precision of these measurements must be better than the HEROES X-ray resolution of similar to 20 arcsec Full Width at Half Maximum (FWHM) so as to not degrade the image resolution. The SAS consists of two separate systems: the Pitch-Yaw Aspect System (PYAS) and the Roll Aspect System (RAS). The PYAS functions by projecting an image of the Sun onto a screen with precision fiducials. A CCD camera takes an image of these fiducials, and an automated algorithm determines the location of the Sun as well as the location of the fiducials. The spacing between fiducials is unique and allows each to be identified so that the location of the Sun on the screen can be precisely determined. The RAS functions by imaging the Earth's horizon in opposite directions using a silvered prism imaged by a CCD camera. The design and first results of the performance of these systems during the HEROES flight which occurred in September 2013 are presented here.
引用
收藏
页数:9
相关论文
共 12 条
  • [1] Christe S., 2013, SPIE OPTICAL ENG APP
  • [2] Christe S., 2013, AM ASTRONOMICAL SOC, V44
  • [3] RHESSI aspect reconstruction
    Fivian, M
    Hemmeck, R
    Mchedlishvili, A
    Zehnder, A
    [J]. SOLAR PHYSICS, 2002, 210 (1-2) : 87 - 99
  • [4] Gaskin J., 2013, AER C 2013 IEEE, P1
  • [5] The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO)
    Lemen, James R.
    Title, Alan M.
    Akin, David J.
    Boerner, Paul F.
    Chou, Catherine
    Drake, Jerry F.
    Duncan, Dexter W.
    Edwards, Christopher G.
    Friedlaender, Frank M.
    Heyman, Gary F.
    Hurlburt, Neal E.
    Katz, Noah L.
    Kushner, Gary D.
    Levay, Michael
    Lindgren, Russell W.
    Mathur, Dnyanesh P.
    McFeaters, Edward L.
    Mitchell, Sarah
    Rehse, Roger A.
    Schrijver, Carolus J.
    Springer, Larry A.
    Stern, Robert A.
    Tarbell, Theodore D.
    Wuelser, Jean-Pierre
    Wolfson, C. Jacob
    Yanari, Carl
    Bookbinder, Jay A.
    Cheimets, Peter N.
    Caldwell, David
    Deluca, Edward E.
    Gates, Richard
    Golub, Leon
    Park, Sang
    Podgorski, William A.
    Bush, Rock I.
    Scherrer, Philip H.
    Gummin, Mark A.
    Smith, Peter
    Auker, Gary
    Jerram, Paul
    Pool, Peter
    Soufli, Regina
    Windt, David L.
    Beardsley, Sarah
    Clapp, Matthew
    Lang, James
    Waltham, Nicholas
    [J]. SOLAR PHYSICS, 2012, 275 (1-2) : 17 - 40
  • [6] Optimal edge-based shape detection
    Moon, H
    Chellappa, R
    Rosenfeld, A
    [J]. IEEE TRANSACTIONS ON IMAGE PROCESSING, 2002, 11 (11) : 1209 - 1227
  • [7] O'Connor B. F., 2013, 43 INT C ENV SYST RE
  • [8] ESTIMATION OF A PROBABILITY DENSITY-FUNCTION AND MODE
    PARZEN, E
    [J]. ANNALS OF MATHEMATICAL STATISTICS, 1962, 33 (03): : 1065 - &
  • [9] First images from HERO, a hard X-ray focusing telescope
    Ramsey, BD
    Alexander, CD
    Apple, JA
    Benson, CM
    Dietz, KL
    Elsner, RF
    Engelhaupt, DE
    Ghosh, KK
    Kolodziejczak, JJ
    O'Dell, SL
    Speegle, CO
    Swartz, DA
    Weisskopf, MC
    [J]. ASTROPHYSICAL JOURNAL, 2002, 568 (01) : 432 - 435
  • [10] REMARKS ON SOME NONPARAMETRIC ESTIMATES OF A DENSITY-FUNCTION
    ROSENBLATT, M
    [J]. ANNALS OF MATHEMATICAL STATISTICS, 1956, 27 (03): : 832 - 837