Abstract
The main objective of the Mutual Impedance Probe (MIP), part of the Rosetta Plasma Consortium (RPC), is to measure the electron density and temperature of Comet 67P/Churyumov-Gerasimenko’s coma, in particular inside the contact surface. Furthermore, MIP will determine the bulk velocity of the ionised outflowing atmosphere, define the spectral distribution of natural plasma waves, and monitor dust and gas activities around the nucleus. The MIP instrumentation consists of an electronics board for signal processing in the 7 kHz to 3.5 MHz range and a sensor unit of two receiving and two transmitting electrodes mounted on a 1-m long bar. In addition, the Langmuir probe of the RPC/LAP instrument that is at about 4 m from the MIP sensor can be used as a transmitter (in place of the MIP ones) and MIP as a receiver in order to have access to the density and temperature of plasmas at higher Debye lengths than those for which the MIP is originally designed.
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Béghin, C., Karczewski, J.F., Poirier, B., Debrie, R., and Massevitch, N.: 1982, Ann. Geophysicae 38, 615.
Béghin, C.: 1995, Radio Sci. 30, 307.
Béghin, C., and Kolesnikova, E.: 1998, Radio Sci. 33, 503.
Chasseriaux, J.M., Debrie, R., and Renard, C.: 1972, J. Plasma Phys. 8, 231.
Décréau, P.M.E., Béghin, C., and Parrot, M.: 1978, Space Sci. Rev. 22, 581.
Geiswiller, J., Béghin, C., Kolesnikova, E., Lagoutte, D., Michau, J. L., and Trotignon, J. G.: 2001a, Planet. Space Sci. 49, 633.
Geiswiller, J., Trotignon, J.G., Béghin, C., and Kolesnikova, E.: 2001b, Astrophys. Space Sci. 277, 317.
Gombosi, T.I., De Zeeuw, D.L., Häberli, R.M., and Powell, K.G.: 1996, J. Geophys. Res. 101, 15, 233.
Grard, R., Scarf, F., Trotignon, J.G., and Mogilevsky, M.: 1987, Eur. Space Agency Spec. Publ., ESA SP-278, 97.
Grard, R., Laakso, H., Pedersen, A., Trotignon, J.G., and Mikhaïlov, Y.: 1989, Ann. Geophysicae 7, 141.
Grün, E.: 1981, Eur. Space Agency Spec. Publ., ESA SP-155, 81.
Gurnett, D.A., Averkamp, T.F., Scarf, F.L., and Grün, E.: 1986, Geophys. Res. Lett. 13, 291.
Gurnett, D.A., Kurth, W.S., Steinberg, J.T., and Shawhan, S.D.: 1988, Geophys. Res. Lett. 15, 760.
Kolesnikova, E., and C. Béghin, C.: 1998, Radio Sci. 33, 491.
Laakso, H., Grard, R., Pedersen, A., and Schwehm, G.: 1989, Adv. Space Res. 9, 269.
Lebreton, J.P., and Henry, D.: 1980, Phys. Letters 76A, 49.
Meyer-Vernet, N., Couturier, P., Hoang, S., Perche, C., and Steinberg, J. L.: 1986, Geophys. Res. Lett. 13, 279.
Michel, E.: 1976, J. Plasma Phys. 15, 395.
Oberc, P.: 1993, Planet. Space Sci. 41, 609.
Rooy, B., Feix, M.R., and Storey, L.R.O.: 1972, Plasma Phys. 14, 275.
Scarf, F.L., Coroniti, F.V., Kennel, C.F., Gurnett, D.A., Ip, W.H., and Smith, E.J.: 1986, Sci. 232, 377.
Trotignon, J.G., Béghin, C., Grard, R., Pedersen, A., Formisano, V., Mogilevsky, M., and Mikhaïlov, Y.: 1987, Astron. Astrophys. 187, 83.
Trotignon, J.G., Grard, R., and Mogilevsky, M.: 1989, Ann. Geophysicae 7, 331.
Trotignon, J.G., Béghin, C., Grard, R., Pedersen, A., Mogilevsky, M., and Mikhaïlov, Y.: 1991, in A. D. Johnstone (ed.), Cometary Plasma Processes, Geophys. Monogr. Ser., vol. 61, AGU, Washington, D.C., p. 179.
Trotignon, J.G., Boström, R., Burch, J.L., Glassmeier, K.-H., Lundin, R., Norberg, O., Balogh, A., Szegö, K., Musmann, G., Coates, A., Åhlén, L., Carr, C., Eriksson, A., Gibson, W., Kuhnke, F., Lundin, K., Michau, J.L., and Szalai, S.: 1999, Adv. Space Res. 24(9), 1149.
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Trotignon, J.G., Michau, J.L., Lagoutte, D. et al. RPC-MIP: the Mutual Impedance Probe of the Rosetta Plasma Consortium. Space Sci Rev 128, 713–728 (2007). https://doi.org/10.1007/s11214-006-9005-1
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DOI: https://doi.org/10.1007/s11214-006-9005-1