Magnetic field fluctuation measurements in the solar orbiter project

V. Krasnoselskikh; J. L. Pinçon; T. Dudok De Wit; P. Fergeau; G. Jannet; T. Chust; C. Coillot; M. Maksimovic

Magnetic field fluctuation measurements in the solar orbiter project

V. Krasnoselskikh, J. L. Pinçon, T. Dudok De Wit, P. Fergeau, G. Jannet, T. Chust, C. Coillot, M. Maksimovic

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

Abstract

Although the wave activity observed in the solar wind near the terrestrial orbit is rather well understood, many questions remain concerning waves that occur much closer to the Sun. The measurements closest to the Sun have so far been obtained by the Helios 1 and 2 spacecraft at approximately 0.3 AU. Based on these observations, we present the characteristics of the waves that are expected to occur near 0.2 AU and discuss the magnetic field sensors that are required to measure them. The Search Coil Magnetometer (SCM) we propose is the part of the Radio and plasma wave experiment that is described in Maksimovic et al., 2006.

Original language	English
Title of host publication	Proceedings of the Second Solar Orbiter Workshop
Edition	SP-641
Publication status	Published - 1 Oct 2006
Externally published	Yes
Event	2nd Solar Orbiter Workshop - Athens, Greece Duration: 16 Oct 2006 → 20 Oct 2006

Publication series

Name	European Space Agency, (Special Publication) ESA SP
Number	SP-641
ISSN (Print)	0379-6566

Conference

Conference	2nd Solar Orbiter Workshop
Country/Territory	Greece
City	Athens
Period	16/10/06 → 20/10/06

Cite this

@inproceedings{1d77844f2bf04dacb4a9e83d2b42c123,

title = "Magnetic field fluctuation measurements in the solar orbiter project",

abstract = "Although the wave activity observed in the solar wind near the terrestrial orbit is rather well understood, many questions remain concerning waves that occur much closer to the Sun. The measurements closest to the Sun have so far been obtained by the Helios 1 and 2 spacecraft at approximately 0.3 AU. Based on these observations, we present the characteristics of the waves that are expected to occur near 0.2 AU and discuss the magnetic field sensors that are required to measure them. The Search Coil Magnetometer (SCM) we propose is the part of the Radio and plasma wave experiment that is described in Maksimovic et al., 2006.",

author = "V. Krasnoselskikh and Pin{\c c}on, \{J. L.\} and \{De Wit\}, \{T. Dudok\} and P. Fergeau and G. Jannet and T. Chust and C. Coillot and M. Maksimovic",

year = "2006",

month = oct,

day = "1",

language = "English",

isbn = "9290922052",

series = "European Space Agency, (Special Publication) ESA SP",

number = "SP-641",

booktitle = "Proceedings of the Second Solar Orbiter Workshop",

edition = "SP-641",

note = "2nd Solar Orbiter Workshop ; Conference date: 16-10-2006 Through 20-10-2006",

}

Magnetic field fluctuation measurements in the solar orbiter project. / Krasnoselskikh, V.; Pinçon, J. L.; De Wit, T. Dudok et al.
Proceedings of the Second Solar Orbiter Workshop. SP-641. ed. 2006. (European Space Agency, (Special Publication) ESA SP; No. SP-641).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

TY - GEN

T1 - Magnetic field fluctuation measurements in the solar orbiter project

AU - Krasnoselskikh, V.

AU - Pinçon, J. L.

AU - De Wit, T. Dudok

AU - Fergeau, P.

AU - Jannet, G.

AU - Chust, T.

AU - Coillot, C.

AU - Maksimovic, M.

PY - 2006/10/1

Y1 - 2006/10/1

N2 - Although the wave activity observed in the solar wind near the terrestrial orbit is rather well understood, many questions remain concerning waves that occur much closer to the Sun. The measurements closest to the Sun have so far been obtained by the Helios 1 and 2 spacecraft at approximately 0.3 AU. Based on these observations, we present the characteristics of the waves that are expected to occur near 0.2 AU and discuss the magnetic field sensors that are required to measure them. The Search Coil Magnetometer (SCM) we propose is the part of the Radio and plasma wave experiment that is described in Maksimovic et al., 2006.

AB - Although the wave activity observed in the solar wind near the terrestrial orbit is rather well understood, many questions remain concerning waves that occur much closer to the Sun. The measurements closest to the Sun have so far been obtained by the Helios 1 and 2 spacecraft at approximately 0.3 AU. Based on these observations, we present the characteristics of the waves that are expected to occur near 0.2 AU and discuss the magnetic field sensors that are required to measure them. The Search Coil Magnetometer (SCM) we propose is the part of the Radio and plasma wave experiment that is described in Maksimovic et al., 2006.

M3 - Conference contribution

AN - SCOPUS:34249699673

SN - 9290922052

SN - 9789290922056

T3 - European Space Agency, (Special Publication) ESA SP

BT - Proceedings of the Second Solar Orbiter Workshop

T2 - 2nd Solar Orbiter Workshop

Y2 - 16 October 2006 through 20 October 2006

ER -

Magnetic field fluctuation measurements in the solar orbiter project

Abstract

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