Research output: Contribution to journal › Article › peer-review
Testing the accuracy of magnetospheric model field line mapping. / Pulkkinen, TI; Tsyganenko, NA.
In: JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol. 101, No. A12, 01.12.1996, p. 27431-27442.Research output: Contribution to journal › Article › peer-review
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TY - JOUR
T1 - Testing the accuracy of magnetospheric model field line mapping
AU - Pulkkinen, TI
AU - Tsyganenko, NA
PY - 1996/12/1
Y1 - 1996/12/1
N2 - We present a new method to test the statistical accuracy of field-aligned mappings by using a large magnetospheric data set and apply the method to the Tsyganenko [1989] model. The obtained errors in the field-aligned mappings are generally small in the auroral Bone outside the midnight sector but become larger on the nightside and within the polar cap. The model tail field is overstretched near midnight and the model field lines flare out toward the flanks and toward high Z values too much. The results also imply that there is a shear layer between the plasma sheet and lobe that could be indicative of the region I field-aligned current system. The large-scale mapping properties suggest that the magnetotail field is asymmetric with respect to the noon-midnight meridian: the model better represents the evening-sector field configuration, whereas the morning-sector model field lines map too far down the tail.
AB - We present a new method to test the statistical accuracy of field-aligned mappings by using a large magnetospheric data set and apply the method to the Tsyganenko [1989] model. The obtained errors in the field-aligned mappings are generally small in the auroral Bone outside the midnight sector but become larger on the nightside and within the polar cap. The model tail field is overstretched near midnight and the model field lines flare out toward the flanks and toward high Z values too much. The results also imply that there is a shear layer between the plasma sheet and lobe that could be indicative of the region I field-aligned current system. The large-scale mapping properties suggest that the magnetotail field is asymmetric with respect to the noon-midnight meridian: the model better represents the evening-sector field configuration, whereas the morning-sector model field lines map too far down the tail.
KW - MAGNETIC-FIELD
KW - QUANTITATIVE MODELS
KW - GEOMAGNETIC-FIELD
KW - CURRENT SHEET
KW - TAIL
KW - MAGNETOTAIL
KW - PARAMETERS
U2 - 10.1029/96JA02489
DO - 10.1029/96JA02489
M3 - Article
VL - 101
SP - 27431
EP - 27442
JO - Journal of Geophysical Research: Biogeosciences
JF - Journal of Geophysical Research: Biogeosciences
SN - 0148-0227
IS - A12
ER -
ID: 28034857