... Ie>2 - the maximum intensity of a flux of electrons in geostationary orbits in days according to GOES 15 in (electrons/cm2-s-sr) for events > 1000 p.f.u. THE GREATER THAN 2 MeV ELECTRON FLUX AT GEOSTATIONARY ORBIT VERY HIGH LEVEL BEGINING 5.08/1325 UT AND ...
... Ie>2 - the maximum intensity of a flux of electrons in geostationary orbits in days according to GOES 15 in (electrons/cm2-s-sr) for events > 1000 p.f.u. THE GREATER THAN 2 MeV ELECTRON FLUX AT GEOSTATIONARY ORBIT VERY HIGH LEVEL NOT OBSERVED. ...
... observatory; EE-date of possible geomag. disturbance in the Earth's environment ... FROM 12.03/08 UT THE EARTH IS IN "-" SECTOR OF THE INTERPLANETARY MAG- NETIC FIELD. ... THE FOLLOWING SECTOR BOUNDARY -/+ THE EARTH HAS TO PASS 27.04. ...
... Ie>2 - the maximum intensity of a flux of electrons in geostationary orbits in days according to GOES 15 in (electrons/cm2-s-sr) for events > 1000 p.f.u. THE GREATER THAN 2 MeV ELECTRON FLUX AT GEOSTATIONARY ORBIT VERY HIGH LEVEL OBSERVED 29.07 AND 1.08. ...
... observatory; EE-date of possible geomag. disturbance in the Earth's environment ... FROM 20.04/14 UT THE EARTH IS IN "+" SECTOR OF THE INTERPLANETARY MAG- NETIC FIELD. ... THE FOLLOWING SECTOR BOUNDARY +/- THE EARTH HAS TO PASS 7.05. ...
... observatory; EE-date of possible geomag. disturbance in the Earth's environment ... FROM 20.04/14 UT THE EARTH IS IN "+" SECTOR OF THE INTERPLANETARY MAG- NETIC FIELD. ... THE FOLLOWING SECTOR BOUNDARY +/- THE EARTH HAS TO PASS 7.05. ...
... observatory; EE-date of possible geomag. disturbance in the Earth's environment ... AFTER 30.10/16 UT THE EARTH IS IN "-" SECTOR OF THE INTERPLANETARY MAGNETIC FIELD. ... THE FOLLOWING SECTOR BOUNDERY - /+ THE EARTH HAS TO PASS 14.11. ...
... observatory; EE-date of possible geomag. disturbation in the Earth's environment ... AFTER 15.06/05 UT EARTH IS IN "-" SECTOR OF THE INTERPLANETARY MAGNETIC FIELD. ... THE FOLLOWING SECTOR BOUNDARY -/+ THE EARTH SHOULD TO PASS 28.06. ...
... Ie>2 - the maximum intensity of a flux of electrons in geostationary orbits in days according to GOES 15 in (electrons/cm2-s-sr) for events > 1000 p.f.u. THE GREATER THAN 2 MeV ELECTRON FLUX AT GEOSTATIONARY ORBIT VERY HIGH LEVEL WAS NOT OBSERVED. ...