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CHROMOSPHERIC AND CORONAL STRUCTURE OF POLAR PLUMES – I. Magnetic Structure and Radiative Energy Balance

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Abstract

The Multi-Spectral Solar Telescope Array (MSSTA), a rocket-borne solar observatory, was successfully launched from White Sands Missile Range, New Mexico, on May 13, 1991 at 19:05 UT. The telescope systems onboard the MSSTA obtained several full disk solar images in narrow bandpasses centered around strong soft X-ray, EUV, and FUV emission lines. Each telescope was designed to be sensitive to the coronal plasmas at a particular temperature, for seven temperatures ranging from 20000 K to 4000000 K. We report here on the images obtained during the initial flight of the MSSTA, and on the chromospheric and coronal structure of polar plumes observed over both poles of the Sun. We have also co-aligned the MSSTA images with Kitt Peak magnetograms taken on the same day. We are able to positively identify the magnetic structures underlying the polar plumes we analyze as unipolar. We discuss the plume observations and present a radiative energy balance model derived from them.

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Authors and Affiliations

  1. Physics Laboratory, Stanford University, Stanford, CA, 94305–4060, U.S.A

    Maxwell J. Allen, Hakeem M. Oluseyi & Arthur B. C. Walker

  2. Space Science Laboratory, NASA Marshall Space Flight Center, AL, 35812, U.S.A

    Richard B. Hoover

  3. Lawrence Livermore National Laboratory, Livermore, CA, 94550, U.S.A

    Troy W. Barbee Jr.

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  1. Maxwell J. Allen
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  2. Hakeem M. Oluseyi
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  3. Arthur B. C. Walker
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  4. Richard B. Hoover
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  5. Troy W. Barbee Jr.
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Allen, M.J., Oluseyi, H.M., Walker, A.B.C. et al. CHROMOSPHERIC AND CORONAL STRUCTURE OF POLAR PLUMES – I. Magnetic Structure and Radiative Energy Balance. Solar Physics 174, 367–401 (1997). https://doi.org/10.1023/A:1004955129119

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