TY - JOUR
T1 - Effects of dipole tilt angle on geomagnetic activity
AU - Nowada, M.
AU - Shue, J. H.
AU - Russell, C. T.
N1 - Funding Information:
This work was supported in part by National Science Council Grant NSC-96-2811-M-008-002 and National Space Organization Grant 97-NSPO(B)-SP-FA07-01 to National Central University and in part by Ministry of Education under the Aim for Top University program at National Central University. We thank J.T. Gosling, A.J. Lazarus, R.P. Lepping for the use of IMP 8 magnetic field and plasma data via NSSDC website. We also thank World Data Center for Magnetism, Kyoto University, for the use of both AL and AU indices. M.N. thank W.-C. Hsieh for helping the IDL computer programming. The work at UCLA was supported by the National Science Foundation under Grant ATM-04-02213.
PY - 2009/9
Y1 - 2009/9
N2 - The relationship between the orientation of the interplanetary magnetic field (IMF), represented by the clock angle which is the angle defined by IMF-By and -Bz components, and the AL and AU indices is examined at various dipole tilt angles for the period of 1978-1988. We use the IMF data obtained from the IMP 8 satellite, AL and AU indices with corrected seasonal variations, and the dipole tilt angle, which is the dipole magnetic latitude of the subsolar point calculated as a function of the day of year and universal time. For both positive (dipole tilted to the Sun) and negative dipole tilt angles, the values of | AL | and AU decrease as the IMF clock angle moves away from 180{ring operator}, becoming more northward. The indices also tend to become smaller for larger dipole tilt angle, either toward or away from the Sun. This dependence on dipole tilt angle enhances the semiannual variation of geomagnetic activity.
AB - The relationship between the orientation of the interplanetary magnetic field (IMF), represented by the clock angle which is the angle defined by IMF-By and -Bz components, and the AL and AU indices is examined at various dipole tilt angles for the period of 1978-1988. We use the IMF data obtained from the IMP 8 satellite, AL and AU indices with corrected seasonal variations, and the dipole tilt angle, which is the dipole magnetic latitude of the subsolar point calculated as a function of the day of year and universal time. For both positive (dipole tilted to the Sun) and negative dipole tilt angles, the values of | AL | and AU decrease as the IMF clock angle moves away from 180{ring operator}, becoming more northward. The indices also tend to become smaller for larger dipole tilt angle, either toward or away from the Sun. This dependence on dipole tilt angle enhances the semiannual variation of geomagnetic activity.
KW - Dipole tilt
KW - Geomagnetic activity
KW - Interplanetary magnetic field
KW - Magnetic reconnection
KW - Semiannual variation
UR - http://www.scopus.com/inward/record.url?scp=68949115947&partnerID=8YFLogxK
U2 - 10.1016/j.pss.2009.04.007
DO - 10.1016/j.pss.2009.04.007
M3 - 期刊論文
AN - SCOPUS:68949115947
SN - 0032-0633
VL - 57
SP - 1254
EP - 1259
JO - Planetary and Space Science
JF - Planetary and Space Science
IS - 11
ER -