And for shorter intervals for FAST and
Akebono
Interball Aurora
Interball Tail
Equator-S
NOTE The POLAR project maintains a list of times of Exceptional Southern Oval Viewing . Selected times from that list are noted below.
Link to the
Polar Image Pointing Plan Page
Period of 98 101-107 one exceptional FAST conjunction interval 98106 0712-0718 FAST footprint in VIS fov ~3mlt oval, 0716 FAST footprint in UVI fov ~3mlt oval, oval not sunlite. 98107 0054-0100 FAST footprint in VIS fov post midnight oval, 0057 both POLAR and FAST footprints in UVI fov ~22 mlt oval, oval not sunlite. *****
98073 1716-1722 FAST fp in VIS fov in polar/prenoon oval, 1718- both FAST fp and POLAR fp in VIS fov in polar cap **. 98072 0550-0554 FAST fp in VIS fov in post midnight oval. 98072 2332-2339 FAST fp in VIS fov in evening oval/polar cap, 2335 FAST fp in UVI fov in polarcap. 98071 1206-1210 FAST fp in VIS fov in polcar cap/oval. 1208 FAST fp in UVI fov in 7mlt oval. 98070 0037-0045 FAST fp in VIS fov in polar cap/oval, 0040 FAST fp in UVI fov in 22mlt oval. 98070 1824-1829 FAST fp in VIS fov in polar cap/prenoon oval.
When two satellites:
The ascii files of magnetic conjunction times pointed too below were caluclated using NASA supplied SSC software. The size of the magnetic conjunction box is indicated at the head of each file.
NOTE. Orbital predictions for low perigee satellites, such as FAST (350 km) can not take into account the significant and variable drag forces caused by ionospheric heating associated with geomagnetic activity. The magnitude of the problem has been illustrated by Sardi Parthasarathy of the NSSDC.
Yeh-Kai Tung (U.C. Berekely) maintains a page that identifies the most promising predicted POLAR/FAST conjunctions. Last Updated in Late 1997.