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Автор H Balsiger
Автор K Altwegg
Автор J Benson
Автор F Buhler
Автор J Fischer
Автор J Geiss
Автор B E Goldstein
Автор R Goldstein
Автор P Hemmerich
Автор G Kulzer
Автор A J Lazarus
Автор A Meier
Автор M Neugebauer
Автор U Rettenmund
Автор H Rosenbauer
Автор K Sager
Автор T Sanders
Автор R Schwenn
Автор E G Shelley
Автор D Simpson
Автор D T Young
Дата выпуска 1987-06-01
dc.description As expected, a wide range of ion species and velocity distributions were found as the Giotto spacecraft traversed the coma of Comet Halley. The outer coma was characterised by the interaction between solar wind and cometary plasmas; the inner coma by the outflow of cometary neutrals and their ionisation products. The resultant demands on instrument dynamic range had precluded the use of a single sensor for measurements of ion composition. The Giotto ion mass spectrometer (IMS) therefore consisted of two sensors: one optimised for the outer coma and the other for the inner coma, with each obtaining complementary information in the region for which it was not optimised. Both sensors featured mass-imaging characteristics, thereby permitting simultaneous measurements of several ion species by means of multi-detector arrays. Resultant mass per charge resolution was >or=20. In addition to mass per charge, the energy per charge and the elevation and azimuth of the incident ions were measured. In-flight data show that the IMS met its scientific goals for the Halley encounter.
Формат application.pdf
Издатель Institute of Physics Publishing
Название The ion mass spectrometer on Giotto
Тип paper
DOI 10.1088/0022-3735/20/6/034
Print ISSN 0022-3735
Журнал Journal of Physics E: Scientific Instruments
Том 20
Первая страница 759
Последняя страница 767
Аффилиация H Balsiger; Phys. Inst., Berne Univ., Switzerland
Аффилиация K Altwegg; Phys. Inst., Berne Univ., Switzerland
Аффилиация J Benson; Phys. Inst., Berne Univ., Switzerland
Аффилиация F Buhler; Phys. Inst., Berne Univ., Switzerland
Аффилиация J Fischer; Phys. Inst., Berne Univ., Switzerland
Аффилиация J Geiss; Phys. Inst., Berne Univ., Switzerland
Аффилиация B E Goldstein; Phys. Inst., Berne Univ., Switzerland
Аффилиация R Goldstein; Phys. Inst., Berne Univ., Switzerland
Аффилиация P Hemmerich; Phys. Inst., Berne Univ., Switzerland
Аффилиация G Kulzer; Phys. Inst., Berne Univ., Switzerland
Аффилиация A J Lazarus; Phys. Inst., Berne Univ., Switzerland
Аффилиация A Meier; Phys. Inst., Berne Univ., Switzerland
Аффилиация M Neugebauer; Phys. Inst., Berne Univ., Switzerland
Аффилиация U Rettenmund; Phys. Inst., Berne Univ., Switzerland
Аффилиация H Rosenbauer; Phys. Inst., Berne Univ., Switzerland
Аффилиация K Sager; Phys. Inst., Berne Univ., Switzerland
Аффилиация T Sanders; Phys. Inst., Berne Univ., Switzerland
Аффилиация R Schwenn; Phys. Inst., Berne Univ., Switzerland
Аффилиация E G Shelley; Phys. Inst., Berne Univ., Switzerland
Аффилиация D Simpson; Phys. Inst., Berne Univ., Switzerland
Аффилиация D T Young; Phys. Inst., Berne Univ., Switzerland
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