Superposed epoch analyses have shown that, on average, the interplanetary magnetic field (IMF) turns northward close to substorm onset. This has been commonly accepted as evidence for the substorm onset being triggered by a rapid northward turning of the IMF. Here we show that the tendency arises in any superposed epoch analysis of the IMF in which event onset is biased to occur for southward IMF, irrespective of a coincident rapid northward turning of the IMF. The overall IMF variation found in the largest superposed epoch analysis of this kind is also well reproduced using a Minimal Substorm Model in which substorm onsets are determined without the requirement of a northward IMF turning trigger. We discuss the explanation underlying these...
An outstanding topic in magnetospheric physics is whether substorms are always externally triggered ...
Multispacecraft data from the upstream solar wind, polar cusp, and inner magnetotail are used to sho...
Substorms take place under a variety of solar wind and interplanetary magnetic field (IMF) condition...
Some studies over the last decade have indicated that the instability responsible for substorm expan...
Some studies over the last decade have indicated that the instability responsible for substorm expan...
We re-examine whether substorms are triggered by solar wind fluctuations or an internal magnetospher...
Some studies over the last decade have indicated that the instability responsible for substorm expa...
International audienceBased on 2760 well-defined substorm onsets in the Northern Hemisphere and 1432...
The occurrence rate of magnetic substorms during the northward IMF was investigated statistically. T...
While substorms are known to generally occur under southward IMF conditions, they can sometimes occ...
Based on 2760 well-defined substorm onsets in the Northern Hemisphere and 1432 in the Southern Hemi...
We analyze two substorm onset lists, produced by different methods, and show that the (Bx·vz) produc...
Multispacecraft data from the upstream solar wind, polar cusp, and inner magnetotail are used to sho...
We report a superposed epoch analysis of the hemispheric open magnetic flux, maximum nightside auror...
Abstract The dynamics of substorms are known to be dominated by the North-South (Bz) component of t...
An outstanding topic in magnetospheric physics is whether substorms are always externally triggered ...
Multispacecraft data from the upstream solar wind, polar cusp, and inner magnetotail are used to sho...
Substorms take place under a variety of solar wind and interplanetary magnetic field (IMF) condition...
Some studies over the last decade have indicated that the instability responsible for substorm expan...
Some studies over the last decade have indicated that the instability responsible for substorm expan...
We re-examine whether substorms are triggered by solar wind fluctuations or an internal magnetospher...
Some studies over the last decade have indicated that the instability responsible for substorm expa...
International audienceBased on 2760 well-defined substorm onsets in the Northern Hemisphere and 1432...
The occurrence rate of magnetic substorms during the northward IMF was investigated statistically. T...
While substorms are known to generally occur under southward IMF conditions, they can sometimes occ...
Based on 2760 well-defined substorm onsets in the Northern Hemisphere and 1432 in the Southern Hemi...
We analyze two substorm onset lists, produced by different methods, and show that the (Bx·vz) produc...
Multispacecraft data from the upstream solar wind, polar cusp, and inner magnetotail are used to sho...
We report a superposed epoch analysis of the hemispheric open magnetic flux, maximum nightside auror...
Abstract The dynamics of substorms are known to be dominated by the North-South (Bz) component of t...
An outstanding topic in magnetospheric physics is whether substorms are always externally triggered ...
Multispacecraft data from the upstream solar wind, polar cusp, and inner magnetotail are used to sho...
Substorms take place under a variety of solar wind and interplanetary magnetic field (IMF) condition...