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Magnetopause Stand-off Distance Monitor[Overview] [Realtime Monitor] [Stand-off Distance Data Archive]
This monitor provides magnetopause stand-off distance (geocentric distance to the magnetopause subsolar point, Rss) calculated in accordance with the [Shue et al., 1998] model:
Rss = (10.22+1.29*tanh(0.184*(8.14+bz)))*p-1./6.6
Also there is a database of subsolar point calculated in accordance with the [Kuznetsov-Suvorova, 1998] model:
Rss = 8.6*(1 + 0.407*exp( - (|Bz| - Bz)2/200/p0.15))*p-0.19
There is a database of subsolar point calculated in accordance with the [Alexeev-Kalegaev-Lyutov, 1999] model:
Rss = (11.3 + 0.39*Bz)*(p/2.63)-1/6, bz < 0
Rss = (11.3 + 0.09*Bz)*(p/2.47)-1/6, bz > 0 Bz [nT] (interplanetary magnetic field z-component is GSM coordinates) and P [nPa] (solar wind dynamic pressure) are measured by ACE spacecraft at UTACE time instant. Highlighted rows in the source data table indicate the solar wind conditions that are estimated to be bound to the Earth's magnetosphere at current UT=20:57. The corresponding magnetopause stand-off distance overage value is Rss=DB fails Special thanks to the ACE team (http://www.sec.noaa.gov/ace/) for providing real-time solar wind and magnetic field data. Magnetopause stand-off distance calculated using solar wind data measured by ACE spacecraft
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