Abstract
This Chapter describes the physical characteristics of RPS-1 device and some of experimental results of observations onboard CORONAS-F satellite. Semiconductor spectrometer registered x-ray radiation in the range 3–31.5 Kev. Detailed spectral and time characteristics of weak solar flares were obtained for the first time under relatively low solar activity conditions and at the satellite passage outside the Earth Radiation Belts (ERB). It was established that the increase of solar activity was accompanied by the hardening of the background radiation spectra (without flares). Observations of the nighttime Earth atmosphere visualized the ERBs dynamics (disruption of the northern radiation belt in summer 2002) in the period following the cycle maximum. The energy of the nighttime X-ray emission of the upper atmosphere caused by precipitating magnetospheric electrons did not exceed 8 keV. The energy of GCR contribution to this emission did not exceed 5 keV
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
Glyanenko, A.S., Pavlov, A.A., Pankov, V.M., et al.: Calibration of the RPS-1 semi-conductor detector in the \(\ll \) CORONAS-F ≫ project. MEPhI Sci. Sess. 7, 37–38 (2001) (in Russian)
Kotov, Yu.D., Glyanenko, A.S., Arkhangelskii, A.I., Pavlov, A.A.: The results of preparation of the AVS-F experiment. MEPhI Sci. Sess. 7, 33–34 (2001) (in Russian)
Lin, R.P., Schwarz, R.A., Pelling, R.M., Hurley, K.C.: A new component of hard X-rays in solar flares. Astrophys. J. 251, L109–L114 (1981)
Mizera, P.F., et al.: Observation of auroral arcs, electrons, and X-rays from a DMSP satellite. J. Geophys. Res. 83(A12), 5573–5578 (1978)
Pankov, V.M., Prokhin, V.L., Shkurkin, Yu.G., et al.: The X-ray semi-conductor spectrometer (RPS-1) in the \(\ll \) CORONAS-F ≫ project. High-energy cosmic radiation. L: PhTI, pp. 196–199 (1989) (in Russian)
Pankov, V.M., Prokhin, V.L., Shkurkin, Yu.G., et al.: X-ray semiconductor (CdTe) spectrometer for solar flare and preflare studies. Radiophys. Quantum Electron. 34(11–12), 1002–1005 (1996)
Pankov, V.M., Prokhin, V.L., Khavenson, N.G.: The RPS-1 X-ray CdTe spectrometer onboard the CORONAS-F satellite. Sol. Syst. Res. 40(4), 314–318 (2006)
PIXIE_Image: http://muir.spasci.com/pixie/homepage/img_dir/internal/Image_Def_Slide.gif
Pounds, K.A.: The solar X-radiation below 25 Å. Ann. Geophys. 26(2), 555–565 (1970)
Turiel, J., MacCregor, A.: Observation of solar X-rays with a solid-state detector. Astrophys. J. 162, 287–291 (1970)
Voss, H.D., Smith, L.G.: Global zones of energetic particle precipitation. J. Atmos. Terr. Phys. 42(2), 227–239 (1980)
Author information
Authors and Affiliations
Corresponding author
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2014 Springer-Verlag Berlin Heidelberg
About this chapter
Cite this chapter
Pankov, V.M. et al. (2014). RPS-1 Experiment. In: Kuznetsov, V. (eds) The Coronas-F Space Mission. Astrophysics and Space Science Library, vol 400. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-39268-9_16
Download citation
DOI: https://doi.org/10.1007/978-3-642-39268-9_16
Published:
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-642-39267-2
Online ISBN: 978-3-642-39268-9
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)