Evidence of high-latitude reconnecting during northward IMF: Hawkeye observations
| Autor: | T. E. Eastman, Lun C. Tan, Scott A. Boardsen, R. L. Kessel, James L. Green, S.-H. Chen, L. A. Frank, Shing F. Fung, John D. Craven |
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| Rok vydání: | 1996 |
| Předmět: |
Physics
Field (physics) Magnetic reconnection Geophysics Physics::Geophysics Magnetic field Particle acceleration Solar wind High latitude Physics::Space Physics Astrophysics::Solar and Stellar Astrophysics General Earth and Planetary Sciences Magnetopause Interplanetary magnetic field Astrophysics::Galaxy Astrophysics |
| Zdroj: | Geophysical Research Letters. 23:583-586 |
| ISSN: | 0094-8276 |
| Popis: | Reconnection is accepted as an important process for driving the solar wind/magnetospheric interaction although it is not fully understood. In particular, reconnection for northward interplanetary magnetic field (IMF) at high-latitudes tailward of the cusp, has received little attention in comparison with equatorial reconnection for southward IMF. Using Hawkeye data we present the first direct observations of reconnection at the high-latitude magnetopause (75°) during northward IMF in the form of sunward flowing protons. This flow is nearly field aligned, approximately Alfvenic, and roughly obeys tangential momentum balance. The magnetic field shear is large at the magnetopause and there is a non-zero BN component suggesting the existence of a rotational discontinuity and reconnection. The Hawkeye observations support several recent simulations at least qualitatively in terms of flow directions expected for high-latitude reconnection during northward IMF. |
| Databáze: | OpenAIRE |
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