Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-22T18:39:20.287Z Has data issue: false hasContentIssue false
  • English
  • Français

Soft X-ray polarimeter-spectrometer SOLPEX

Published online by Cambridge University Press:  09 September 2016

Marek Stȩślicki ,
Janusz Sylwester ,
Stefan Płocieniak ,
Jarosław Bakała ,
Żaneta Szaforz ,
Daniel Ścisłowski ,
Mirosław Kowaliński ,
Jose Hernandez ,
Sergey Kuzin  and
Sergey Shestov
Marek Stȩślicki
Affiliation:
Solar Physics Division, Space Research Centre Polish Academy of Sciences, Kopernika 11, 51-622 Wrocław, Poland email: [email protected]
Janusz Sylwester
Affiliation:
Solar Physics Division, Space Research Centre Polish Academy of Sciences, Kopernika 11, 51-622 Wrocław, Poland email: [email protected]
Stefan Płocieniak
Affiliation:
Solar Physics Division, Space Research Centre Polish Academy of Sciences, Kopernika 11, 51-622 Wrocław, Poland email: [email protected]
Jarosław Bakała
Affiliation:
Solar Physics Division, Space Research Centre Polish Academy of Sciences, Kopernika 11, 51-622 Wrocław, Poland email: [email protected]
Żaneta Szaforz
Affiliation:
Solar Physics Division, Space Research Centre Polish Academy of Sciences, Kopernika 11, 51-622 Wrocław, Poland email: [email protected] Astronomical Institute, University of Wroclaw, Kopernika 11, 51-622 Wrocław, Poland email: [email protected]
Daniel Ścisłowski
Affiliation:
Solar Physics Division, Space Research Centre Polish Academy of Sciences, Kopernika 11, 51-622 Wrocław, Poland email: [email protected]
Mirosław Kowaliński
Affiliation:
Solar Physics Division, Space Research Centre Polish Academy of Sciences, Kopernika 11, 51-622 Wrocław, Poland email: [email protected]
Jose Hernandez
Affiliation:
Solar Physics Division, Space Research Centre Polish Academy of Sciences, Kopernika 11, 51-622 Wrocław, Poland email: [email protected]
Sergey Kuzin
Affiliation:
P.N. Lebedev Physical Institute, Russian Academy of Sciences, Moscow, Russian Federation, email: [email protected]
Sergey Shestov
Affiliation:
P.N. Lebedev Physical Institute, Russian Academy of Sciences, Moscow, Russian Federation, email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present an innovative soft X-ray polarimeter and spectrometer SOLPEX. The instrument is to be mounted aboard the ISS within the Russian science complex KORTES. The measurements to be made by SOLPEX are expected to be of unprecedented quality in terms of sensitivity to detect the soft-X-ray polarization of solar emission emanating from active regions and flares in particular. Simultaneous measurements of the polarization degree and the other characteristics (eg. evolution of the spectra) constitute the last, rather unexplored area of solar X-ray spectroscopy providing substantial diagnostic potential. Second important science task to be addressed are the measurements of Doppler shifts in selected X-ray spectral emission lines formed in hot flaring sources. The novel-type Dopplerometer (flat Bragg crystal drum unit) is planned to be a part of SOLPEX and will allow to measure line Doppler shifts in absolute terms with unprecedented time resolution (fraction of a second) during the impulsive flare phases. We shall present some details of the SOLPEX instrument and discuss observing sequences in a view of science objectives to be reached.

Keywords

solarX-raysspectroscopypolarimetry
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S320: Solar and Stellar Flares and their Effects on Planets , August 2015 , pp. 450 - 455
Copyright
Copyright © International Astronomical Union 2016 

References

Battaglia, M., Kleint, L., Krucker, S., & Graham, D. 2015, ApJ, 813, 113 Google Scholar
Beiersdorfer, P., Vogel, D. A., & Reed, K. J. et al. 1996, Physical Review A, 53, 3974 Google Scholar
Boggs, S. E., Coburn, W., & Kalemci, E. 2006, ApJ, 638, 1129 Google Scholar
Emslie, A. G. & Brown, J. C. 1980, ApJ, 237, 1015 Google Scholar
Jeffrey, N. L. S. & Kontar, E. P. 2011, A& A, 536, 93 Google Scholar
Lin, R. P. 2011, Space Science Reviews, 159, 421 Google Scholar
McConnell, M. L. & Smith, D. M., Emslie, et al. 2003, Proc. SPIE, 4843, 1382 CrossRefGoogle Scholar
Milligan, R. O. & Dennis, B. R. 2009, ApJ, 699, 968 Google Scholar
Nakada, M. P., Neupert, W. M., & Thomas, R. J. 1974, Solar Physics, 37, 429 Google Scholar
Tramiel, L. J., Novick, R., & Chanan, G. A. 1984, ApJ, 280, 440 Google Scholar
Suarez-Garcia, E., Hajdas, W., & Wigger, C et al. 2006, Solar Physics, 239, 149 Google Scholar
Sylwester, J., Kordylewski, Z., & Płocieniak, S. et al. 2015, Solar Physics, 239, 149 Google Scholar
Tindo, I. P., Ivanov, V. D., Mandel'Stam, S. L., & Shuryghin, A. I. 1970, Solar Physics, 14, 204 Google Scholar
Tindo, I. P., Ivanov, V. D., Mandel'Stam, S. L., & Shuryghin, A. I. 1972a, Solar Physics, 24, 429 CrossRefGoogle Scholar
Tindo, I. P., Ivanov, V. D., Valníček, B., & Livshits, M. A. 1972b, Solar Physics, 27, 426 Google Scholar
Tindo, I. P., Shurygin, A. I., & Steffen, W. 1976, Solar Physics, 46, 219 Google Scholar
Zharkova, V. V., Kuznetsov, A. A., & Siversky, T. V. 2010, A& A, 512, 490 Google Scholar
Zhitnik, I. A., Logachev, Yu.I., Bogomolov, A. V., & Denisov, Yu. et al. 2006, Sol. Sys. Res., 40, 93 Google Scholar