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Proposal for an Interplanetary Mission to Sound the Outer Regions of the Solar Corona
Published online by Cambridge University Press: 14 August 2015
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The mission of HELIOS had been started in order to investigate in situ the innermost regions of the interplanetary space. The two spacecraft achieved a perihelion of about 0.3 AU solar distance. Fig. 1 is a sketch of the two orbits. The orbital periods are 190 resp. 186 d.
- Type
- Part VII. Future Directions
- Information
- Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 541 - 545
- Copyright
- Copyright © Reidel 1980
References
1
Volland, H., Bird, M.K., Levy, G.S., Stelzried, T.C. and Seidel, B.L.
HELIOS 1 Faraday Rotation Experiment: Results and Interpretations of the Solar Occultation in 1975; J.Geophys.
42, 659, 1977
Google Scholar
2
Edenhofer, P., Esposito, P.B., Hansen, R.T., Lüneburg, E., Martin, W.L. and Zygielbaum, A.I., Time Delay Occultation of Data of the HELIOS Spacecrafts and Preliminary Analysis for Probing the Solar Corona; J. Geophys.
42, 673, 1977
Google Scholar
3
Edenhofer, P., Bird, M.K. and Volland, H., Comparison of Time Delay and Faraday Rotation Measurements from HELIOS Spacecraft; Kleinheubacher Ber.
21, 305–312, 1977 and H. Süss, Privat Communication
Google Scholar
4
Woo, R., Radial Dependence of Solar Wind Properties Deduced from HELIOS 1 and 2 and PIONEER 10/11 Radio Scattering Observations, Astroph. J.
219, 727, 1978
Google Scholar
5
Lüneburg, E. and Esposito, P.B., A Method for the Evaluation of Solar Coronal Plasma Propagation Speeds by Radio Occultation of Space Probes; Nat. Radio Sci. Meeting, U of Washington, Seattle, Wash. 18 - 22 June 1979, p. 284
and JPL - Engineering Memo 315 - 90, 1979
Google Scholar