Abstract
We determine a simple expression for the ramp width of a collisionless fast shock, based upon the relationship between the noncoplanar and main magnetic field components. By comparing this predicted width with that measured during a shock observation, the shock velocity can be determined from a single spacecraft. For a range of low-Mach, low-β bow shock observations made by ISEE-1 and -2, ramp widths determined from two-spacecraft comparison and from this noncoplanar component relationship agree within 30%. When two-spacecraft measurements are not available or are inefficient, this technique provides a reasonable scale size estimation for low Mach shocks.
Original language | English |
---|---|
Article number | 97GL01977 |
Pages (from-to) | 1975-1978 |
Number of pages | 4 |
Journal | Geophysical Research Letters |
Volume | 24 |
Issue number | 16 |
DOIs | |
State | Published - 1 Jan 1997 |
ASJC Scopus subject areas
- Geophysics
- General Earth and Planetary Sciences